{"id":174,"date":"2019-04-05T21:18:41","date_gmt":"2019-04-06T01:18:41","guid":{"rendered":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/?post_type=chapter&#038;p=174"},"modified":"2019-04-10T14:35:13","modified_gmt":"2019-04-10T18:35:13","slug":"chapter-2-review","status":"publish","type":"chapter","link":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/chapter-2-review\/","title":{"raw":"Chapter 2 Review","rendered":"Chapter 2 Review"},"content":{"raw":"<div class=\"os-glossary-container\">\r\n<h3 data-type=\"title\"><span class=\"os-text\">Key Terms<\/span><\/h3>\r\n<dl id=\"fs-id1163709700583\">\r\n \t<dt id=\"38900\">absorber<\/dt>\r\n \t<dd id=\"fs-id1163713194408\">any object that absorbs radiation<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709818708\">\r\n \t<dt id=\"34524\">absorption spectrum<\/dt>\r\n \t<dd id=\"fs-id1163709818714\">wavelengths of absorbed radiation by atoms and molecules<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709837130\">\r\n \t<dt id=\"67087\">Balmer formula<\/dt>\r\n \t<dd id=\"fs-id1163709837136\">describes the emission spectrum of a hydrogen atom in the visible-light range<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709837140\">\r\n \t<dt id=\"70041\">Balmer series<\/dt>\r\n \t<dd id=\"fs-id1163709837145\">spectral lines corresponding to electron transitions to\/from the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-124-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2<\/span><\/span><\/span><span>\u00a0<\/span>state of the hydrogen atom, described by the Balmer formula<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713181127\">\r\n \t<dt id=\"74438\">blackbody<\/dt>\r\n \t<dd id=\"fs-id1163713162382\">perfect absorber\/emitter<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713260316\">\r\n \t<dt id=\"26227\">blackbody radiation<\/dt>\r\n \t<dd id=\"fs-id1163709827773\">radiation emitted by a blackbody<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709679234\">\r\n \t<dt id=\"70475\">Bohr radius of hydrogen<\/dt>\r\n \t<dd id=\"fs-id1163709679239\">radius of the first Bohr\u2019s orbit<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713535514\">\r\n \t<dt id=\"1201\">Bohr\u2019s model of the hydrogen atom<\/dt>\r\n \t<dd id=\"fs-id1163713535519\">first quantum model to explain emission spectra of hydrogen<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713535523\">\r\n \t<dt id=\"89547\">Brackett series<\/dt>\r\n \t<dd id=\"fs-id1163713535528\">spectral lines corresponding to electron transitions to\/from the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-125-Frame\"><span class=\"MathJax_MathContainer\"><span>n=4<\/span><\/span><\/span><span>\u00a0<\/span>state<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709829681\">\r\n \t<dt id=\"87316\">Compton effect<\/dt>\r\n \t<dd id=\"fs-id1163713439061\">the change in wavelength when an X-ray is scattered by its interaction with some materials<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713439065\">\r\n \t<dt id=\"97677\">Compton shift<\/dt>\r\n \t<dd id=\"fs-id1163713494397\">difference between the wavelengths of the incident X-ray and the scattered X-ray<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713277248\">\r\n \t<dt id=\"46976\">Compton wavelength<\/dt>\r\n \t<dd id=\"fs-id1163713256937\">physical constant with the value<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-126-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bbc=2.43pm<\/span><\/span><\/span><\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709827827\">\r\n \t<dt id=\"57397\">cut-off frequency<\/dt>\r\n \t<dd id=\"fs-id1163713294290\">frequency of incident light below which the photoelectric effect does not occur<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713259107\">\r\n \t<dt id=\"67259\">cut-off wavelength<\/dt>\r\n \t<dd id=\"fs-id1163713090752\">wavelength of incident light that corresponds to cut-off frequency<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163710830368\">\r\n \t<dt id=\"82213\">Davisson\u2013Germer experiment<\/dt>\r\n \t<dd id=\"fs-id1163710830374\">historically first electron-diffraction experiment that revealed electron waves<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163711969341\">\r\n \t<dt id=\"56615\">de Broglie wave<\/dt>\r\n \t<dd id=\"fs-id1163711969346\">matter wave associated with any object that has mass and momentum<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163712141867\">\r\n \t<dt id=\"1423\">de Broglie\u2019s hypothesis of matter waves<\/dt>\r\n \t<dd id=\"fs-id1163712189037\">particles of matter can behave like waves<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163711970261\">\r\n \t<dt id=\"8163\">double-slit interference experiment<\/dt>\r\n \t<dd id=\"fs-id1163711970266\">Young\u2019s double-slit experiment, which shows the interference of waves<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163712284810\">\r\n \t<dt id=\"64083\">electron microscopy<\/dt>\r\n \t<dd id=\"fs-id1163712272767\">microscopy that uses electron waves to \u201csee\u201d fine details of nano-size objects<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713513317\">\r\n \t<dt id=\"96405\">emission spectrum<\/dt>\r\n \t<dd id=\"fs-id1163713513322\">wavelengths of emitted radiation by atoms and molecules<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713244844\">\r\n \t<dt id=\"41670\">emitter<\/dt>\r\n \t<dd id=\"fs-id1163713254613\">any object that emits radiation<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713488861\">\r\n \t<dt id=\"35284\">energy of a photon<\/dt>\r\n \t<dd id=\"fs-id1163709786938\">quantum of radiant energy, depends only on a photon\u2019s frequency<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713513327\">\r\n \t<dt id=\"42254\">energy spectrum of hydrogen<\/dt>\r\n \t<dd id=\"fs-id1163713513332\">set of allowed discrete energies of an electron in a hydrogen atom<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713513336\">\r\n \t<dt id=\"84251\">excited energy states of the H atom<\/dt>\r\n \t<dd id=\"fs-id1163713195307\">energy state other than the ground state<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713195311\">\r\n \t<dt id=\"53944\">Fraunhofer lines<\/dt>\r\n \t<dd id=\"fs-id1163713195316\">dark absorption lines in the continuum solar emission spectrum<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713430117\">\r\n \t<dt id=\"69690\">ground state energy of the hydrogen atom<\/dt>\r\n \t<dd id=\"fs-id1163713430122\">energy of an electron in the first Bohr orbit of the hydrogen atom<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163711997462\">\r\n \t<dt id=\"41779\">group velocity<\/dt>\r\n \t<dd id=\"fs-id1163712272028\">velocity of a wave, energy travels with the group velocity<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163712272772\">\r\n \t<dt id=\"14467\">Heisenberg uncertainty principle<\/dt>\r\n \t<dd id=\"fs-id1163711057547\">sets the limits on precision in simultaneous measurements of momentum and position of a particle<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713430127\">\r\n \t<dt id=\"32158\">Humphreys series<\/dt>\r\n \t<dd id=\"fs-id1163713430132\">spectral lines corresponding to electron transitions to\/from the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-127-Frame\"><span class=\"MathJax_MathContainer\"><span>n=6<\/span><\/span><\/span><span>\u00a0<\/span>state<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709831628\">\r\n \t<dt id=\"75762\">hydrogen-like atom<\/dt>\r\n \t<dd id=\"fs-id1163709831633\">ionized atom with one electron remaining and nucleus with charge<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-128-Frame\"><span class=\"MathJax_MathContainer\"><span>+Ze<\/span><\/span><\/span><\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713424856\">\r\n \t<dt id=\"25461\">inelastic scattering<\/dt>\r\n \t<dd id=\"fs-id1163709820901\">scattering effect where kinetic energy is not conserved but the total energy is conserved<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709831646\">\r\n \t<dt id=\"23041\">ionization energy<\/dt>\r\n \t<dd id=\"fs-id1163709831651\">energy needed to remove an electron from an atom<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713557561\">\r\n \t<dt id=\"80790\">ionization limit of the hydrogen atom<\/dt>\r\n \t<dd id=\"fs-id1163713557566\">ionization energy needed to remove an electron from the first Bohr orbit<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713557570\">\r\n \t<dt id=\"99786\">Lyman series<\/dt>\r\n \t<dd id=\"fs-id1163713557576\">spectral lines corresponding to electron transitions to\/from the ground state<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713557580\">\r\n \t<dt id=\"72397\">nuclear model of the atom<\/dt>\r\n \t<dd id=\"fs-id1163713557585\">heavy positively charged nucleus at the center is surrounded by electrons, proposed by Rutherford<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709821220\">\r\n \t<dt id=\"76244\">Paschen series<\/dt>\r\n \t<dd id=\"fs-id1163709821226\">spectral lines corresponding to electron transitions to\/from the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-129-Frame\"><span class=\"MathJax_MathContainer\"><span>n=3<\/span><\/span><\/span><span>\u00a0<\/span>state<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709821239\">\r\n \t<dt id=\"96940\">Pfund series<\/dt>\r\n \t<dd id=\"fs-id1163713513434\">spectral lines corresponding to electron transitions to\/from the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-130-Frame\"><span class=\"MathJax_MathContainer\"><span>n=5<\/span><\/span><\/span><span>\u00a0<\/span>state<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713245842\">\r\n \t<dt id=\"79763\">photocurrent<\/dt>\r\n \t<dd id=\"fs-id1163709681087\">in a circuit, current that flows when a photoelectrode is illuminated<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713168168\">\r\n \t<dt id=\"54615\">photoelectric effect<\/dt>\r\n \t<dd id=\"fs-id1163713483006\">emission of electrons from a metal surface exposed to electromagnetic radiation of the proper frequency<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713425106\">\r\n \t<dt id=\"39602\">photoelectrode<\/dt>\r\n \t<dd id=\"fs-id1163713186641\">in a circuit, an electrode that emits photoelectrons<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713487413\">\r\n \t<dt id=\"78164\">photoelectron<\/dt>\r\n \t<dd id=\"fs-id1163713052088\">electron emitted from a metal surface in the presence of incident radiation<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713265704\">\r\n \t<dt id=\"54813\">photon<\/dt>\r\n \t<dd id=\"fs-id1163713157310\">particle of light<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713284371\">\r\n \t<dt id=\"57522\">Planck\u2019s hypothesis of energy quanta<\/dt>\r\n \t<dd id=\"fs-id1163709749887\">energy exchanges between the radiation and the walls take place only in the form of discrete energy quanta<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713513448\">\r\n \t<dt id=\"80262\">postulates of Bohr\u2019s model<\/dt>\r\n \t<dd id=\"fs-id1163713513454\">three assumptions that set a frame for Bohr\u2019s model<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713195295\">\r\n \t<dt id=\"80462\">power intensity<\/dt>\r\n \t<dd id=\"fs-id1163713087536\">energy that passes through a unit surface per unit time<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709820905\">\r\n \t<dt id=\"87582\">propagation vector<\/dt>\r\n \t<dd id=\"fs-id1163709749388\">vector with magnitude<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-131-Frame\"><span class=\"MathJax_MathContainer\"><span>2\u03c0\/\u03bb<\/span><\/span><\/span><span>\u00a0<\/span>that has the direction of the photon\u2019s linear momentum<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713071482\">\r\n \t<dt id=\"47059\">quantized energies<\/dt>\r\n \t<dd id=\"fs-id1163713310319\">discrete energies; not continuous<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713513459\">\r\n \t<dt id=\"997\">quantum number<\/dt>\r\n \t<dd id=\"fs-id1163713537359\">index that enumerates energy levels<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713033139\">\r\n \t<dt id=\"84074\">quantum phenomenon<\/dt>\r\n \t<dd id=\"fs-id1163713285340\">in interaction with matter, photon transfers either all its energy or nothing<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713275667\">\r\n \t<dt id=\"88162\">quantum state of a Planck\u2019s oscillator<\/dt>\r\n \t<dd id=\"fs-id1163713053248\">any mode of vibration of Planck\u2019s oscillator, enumerated by quantum number<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713282962\">\r\n \t<dt id=\"85834\">reduced Planck\u2019s constant<\/dt>\r\n \t<dd id=\"fs-id1163713443510\">Planck\u2019s constant divided by<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-132-Frame\"><span class=\"MathJax_MathContainer\"><span>2\u03c0<\/span><\/span><\/span><\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713537364\">\r\n \t<dt id=\"24660\">Rutherford\u2019s gold foil experiment<\/dt>\r\n \t<dd id=\"fs-id1163713537369\">first experiment to demonstrate the existence of the atomic nucleus<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713537373\">\r\n \t<dt id=\"91911\">Rydberg constant for hydrogen<\/dt>\r\n \t<dd id=\"fs-id1163713537379\">physical constant in the Balmer formula<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713537383\">\r\n \t<dt id=\"88424\">Rydberg formula<\/dt>\r\n \t<dd id=\"fs-id1163713537388\">experimentally found positions of spectral lines of hydrogen atom<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709826798\">\r\n \t<dt id=\"84253\">scattering angle<\/dt>\r\n \t<dd id=\"fs-id1163713525567\">angle between the direction of the scattered beam and the direction of the incident beam<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709682154\">\r\n \t<dt id=\"49732\">Stefan\u2013Boltzmann constant<\/dt>\r\n \t<dd id=\"fs-id1163709827755\">physical constant in Stefan\u2019s law<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709663034\">\r\n \t<dt id=\"91605\">stopping potential<\/dt>\r\n \t<dd id=\"fs-id1163713120926\">in a circuit, potential difference that stops photocurrent<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713427847\">\r\n \t<dt id=\"41511\">wave number<\/dt>\r\n \t<dd id=\"fs-id1163713267196\">magnitude of the propagation vector<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163712082745\">\r\n \t<dt id=\"84498\">wave quantum mechanics<\/dt>\r\n \t<dd id=\"fs-id1163712082751\">theory that explains the physics of atoms and subatomic particles<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163711057551\">\r\n \t<dt id=\"47746\">wave-particle duality<\/dt>\r\n \t<dd id=\"fs-id1163712273108\">particles can behave as waves and radiation can behave as particles<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713432868\">\r\n \t<dt id=\"72630\">work function<\/dt>\r\n \t<dd id=\"fs-id1163713536679\">energy needed to detach photoelectron from the metal surface<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713120574\">\r\n \t<dt id=\"52612\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-133-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b1<\/span><\/span><\/span>-particle<\/dt>\r\n \t<dd id=\"fs-id1163713120583\">doubly ionized helium atom<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713120587\">\r\n \t<dt id=\"84734\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-134-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b1<\/span><\/span><\/span>-ray<\/dt>\r\n \t<dd id=\"fs-id1163713120595\">beam of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-135-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b1<\/span><\/span><\/span>-particles (alpha-particles)<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163709679224\">\r\n \t<dt id=\"70017\">\u03b2-ray<\/dt>\r\n \t<dd id=\"fs-id1163709679229\">beam of electrons<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1163713195320\">\r\n \t<dt id=\"84006\">\u03b3-ray<\/dt>\r\n \t<dd id=\"fs-id1163713195326\">beam of highly energetic photons<\/dd>\r\n<\/dl>\r\n<\/div>\r\n<div class=\"os-key-equations-container\">\r\n<h3 data-type=\"title\"><span class=\"os-text\">Key Equations<\/span><\/h3>\r\n<section id=\"fs-id1163710783174\" class=\"key-equations\" data-depth=\"1\">\r\n<div class=\"os-table\">\r\n<table id=\"fs-id1172097547296\" class=\"unnumbered unstyled\" summary=\"Table 6.1 \" data-label=\"\">\r\n<tbody>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Wien\u2019s displacement law<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-136-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bbmaxT=2.898\u00d710\u22123m\u22c5K<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Stefan\u2019s law<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-137-Frame\"><span class=\"MathJax_MathContainer\"><span>P(T)=\u03c3AT4<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Planck\u2019s constant<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-138-Frame\"><span class=\"MathJax_MathContainer\"><span>h=6.626\u00d710\u221234J\u22c5s=4.136\u00d710\u221215eV\u22c5s<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Energy quantum of radiation<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-139-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394E=hf<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Planck\u2019s blackbody radiation law<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-140-Frame\"><span class=\"MathJax_MathContainer\"><span>I(\u03bb,T)=2\u03c0hc2\u03bb51ehc\/\u03bbkBT\u22121<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Maximum kinetic energy<span data-type=\"newline\">\r\n<\/span>of a photoelectron<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-141-Frame\"><span class=\"MathJax_MathContainer\"><span>Kmax=e\u0394Vs<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Energy of a photon<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-142-Frame\"><span class=\"MathJax_MathContainer\"><span>Ef=hf<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Energy balance for photoelectron<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-143-Frame\"><span class=\"MathJax_MathContainer\"><span>Kmax=hf\u2212\u03d5<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Cut-off frequency<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-144-Frame\"><span class=\"MathJax_MathContainer\"><span>fc=\u03d5h<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Relativistic invariant<span data-type=\"newline\">\r\n<\/span>energy equation<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-145-Frame\"><span class=\"MathJax_MathContainer\"><span>E2=p2c2+m02c4<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Energy-momentum relation<span data-type=\"newline\">\r\n<\/span>for photon<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-146-Frame\"><span class=\"MathJax_MathContainer\"><span>pf=Efc<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Energy of a photon<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-147-Frame\"><span class=\"MathJax_MathContainer\"><span>Ef=hf=hc\u03bb<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Magnitude of photon\u2019s momentum<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-148-Frame\"><span class=\"MathJax_MathContainer\"><span>pf=h\u03bb<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Photon\u2019s linear<span data-type=\"newline\">\r\n<\/span>momentum vector<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-149-Frame\"><span class=\"MathJax_MathContainer\"><span>p\u2192f=\u210fk\u2192<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">The Compton wavelength<span data-type=\"newline\">\r\n<\/span>of an electron<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-150-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bbc=hm0c=0.00243nm<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">The Compton shift<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-151-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394\u03bb=\u03bbc(1\u2212cos\u03b8)<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">The Balmer formula<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-152-Frame\"><span class=\"MathJax_MathContainer\"><span>1\u03bb=RH(122\u22121n2)<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">The Rydberg formula<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-153-Frame\"><span class=\"MathJax_MathContainer\"><span>1\u03bb=RH(1nf2\u22121ni2),ni=nf+1,nf+2,\u2026<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Bohr\u2019s first quantization condition<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-154-Frame\"><span class=\"MathJax_MathContainer\"><span>Ln=n\u210f,n=1,2,\u2026<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Bohr\u2019s second quantization condition<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-155-Frame\"><span class=\"MathJax_MathContainer\"><span>hf=|En\u2212Em|<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Bohr\u2019s radius of hydrogen<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-156-Frame\"><span class=\"MathJax_MathContainer\"><span>a0=4\u03c0\u03b50\u210f2mee2=0.529\u00c5<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Bohr\u2019s radius of the<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th orbit<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-157-Frame\"><span class=\"MathJax_MathContainer\"><span>rn=a0n2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Ground-state energy value,<span data-type=\"newline\">\r\n<\/span>ionization limit<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-158-Frame\"><span class=\"MathJax_MathContainer\"><span>E0=18\u03b502mee4h2=13.6eV<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Electron\u2019s energy in<span data-type=\"newline\">\r\n<\/span>the<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th orbit<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-159-Frame\"><span class=\"MathJax_MathContainer\"><span>En=\u2212E01n2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Ground state energy of<span data-type=\"newline\">\r\n<\/span>hydrogen<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-160-Frame\"><span class=\"MathJax_MathContainer\"><span>E1=\u2212E0=\u221213.6eV<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">The<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th orbit of<span data-type=\"newline\">\r\n<\/span>hydrogen-like ion<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-161-Frame\"><span class=\"MathJax_MathContainer\"><span>rn=a0Zn2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">The<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th energy<span data-type=\"newline\">\r\n<\/span>of hydrogen-like ion<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-162-Frame\"><span class=\"MathJax_MathContainer\"><span>En=\u2212Z2E01n2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Energy of a matter wave<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-163-Frame\"><span class=\"MathJax_MathContainer\"><span>E=hf<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">The de Broglie wavelength<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-164-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bb=hp<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">The frequency-wavelength relation<span data-type=\"newline\">\r\n<\/span>for matter waves<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-165-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bbf=c\u03b2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr valign=\"top\">\r\n<td data-align=\"left\" data-valign=\"top\">Heisenberg\u2019s uncertainty principle<\/td>\r\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-166-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394x\u0394p\u226512\u210f<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<\/tbody>\r\n<\/table>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-key-concepts-container\">\r\n<h3 data-type=\"title\"><span class=\"os-text\">Summary<\/span><\/h3>\r\n<div class=\"os-key-concepts\">\r\n<div class=\"os-section-area\"><section id=\"fs-id1163709676722\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"88119_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-1-blackbody-radiation\/\"><span class=\"os-number\">2.1<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Blackbody Radiation<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1163709676729\" data-bullet-style=\"bullet\">\r\n \t<li>All bodies radiate energy. The amount of radiation a body emits depends on its temperature. The experimental Wien\u2019s displacement law states that the hotter the body, the shorter the wavelength corresponding to the emission peak in the radiation curve. The experimental Stefan\u2019s law states that the total power of radiation emitted across the entire spectrum of wavelengths at a given temperature is proportional to the fourth power of the Kelvin temperature of the radiating body.<\/li>\r\n \t<li>Absorption and emission of radiation are studied within the model of a blackbody. In the classical approach, the exchange of energy between radiation and cavity walls is continuous. The classical approach does not explain the blackbody radiation curve.<\/li>\r\n \t<li>To explain the blackbody radiation curve, Planck assumed that the exchange of energy between radiation and cavity walls takes place only in discrete quanta of energy. Planck\u2019s hypothesis of energy quanta led to the theoretical Planck\u2019s radiation law, which agrees with the experimental blackbody radiation curve; it also explains Wien\u2019s and Stefan\u2019s laws.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163713129978\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"72890_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-2-photoelectric-effect\/\"><span class=\"os-number\">2.2<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Photoelectric Effect<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1163713120118\" data-bullet-style=\"bullet\">\r\n \t<li>The photoelectric effect occurs when photoelectrons are ejected from a metal surface in response to monochromatic radiation incident on the surface. It has three characteristics: (1) it is instantaneous, (2) it occurs only when the radiation is above a cut-off frequency, and (3) kinetic energies of photoelectrons at the surface do not depend of the intensity of radiation. The photoelectric effect cannot be explained by classical theory.<\/li>\r\n \t<li>We can explain the photoelectric effect by assuming that radiation consists of photons (particles of light). Each photon carries a quantum of energy. The energy of a photon depends only on its frequency, which is the frequency of the radiation. At the surface, the entire energy of a photon is transferred to one photoelectron.<\/li>\r\n \t<li>The maximum kinetic energy of a photoelectron at the metal surface is the difference between the energy of the incident photon and the work function of the metal. The work function is the binding energy of electrons to the metal surface. Each metal has its own characteristic work function.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163713523834\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"31351_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-3-the-compton-effect\/\"><span class=\"os-number\">2.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">The Compton Effect<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1163709750002\" data-bullet-style=\"bullet\">\r\n \t<li>In the Compton effect, X-rays scattered off some materials have different wavelengths than the wavelength of the incident X-rays. This phenomenon does not have a classical explanation.<\/li>\r\n \t<li>The Compton effect is explained by assuming that radiation consists of photons that collide with weakly bound electrons in the target material. Both electron and photon are treated as relativistic particles. Conservation laws of the total energy and of momentum are obeyed in collisions.<\/li>\r\n \t<li>Treating the photon as a particle with momentum that can be transferred to an electron leads to a theoretical Compton shift that agrees with the wavelength shift measured in the experiment. This provides evidence that radiation consists of photons.<\/li>\r\n \t<li>Compton scattering is an inelastic scattering, in which scattered radiation has a longer wavelength than that of incident radiation.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163713328376\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"67977_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-4-bohrs-model-of-the-hydrogen-atom\/\"><span class=\"os-number\">2.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Bohr\u2019s Model of the Hydrogen Atom<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1163713328382\" data-bullet-style=\"bullet\">\r\n \t<li>Positions of absorption and emission lines in the spectrum of atomic hydrogen are given by the experimental Rydberg formula. Classical physics cannot explain the spectrum of atomic hydrogen.<\/li>\r\n \t<li>The Bohr model of hydrogen was the first model of atomic structure to correctly explain the radiation spectra of atomic hydrogen. It was preceded by the Rutherford nuclear model of the atom. In Rutherford\u2019s model, an atom consists of a positively charged point-like nucleus that contains almost the entire mass of the atom and of negative electrons that are located far away from the nucleus.<\/li>\r\n \t<li>Bohr\u2019s model of the hydrogen atom is based on three postulates: (1) an electron moves around the nucleus in a circular orbit, (2) an electron\u2019s angular momentum in the orbit is quantized, and (3) the change in an electron\u2019s energy as it makes a quantum jump from one orbit to another is always accompanied by the emission or absorption of a photon. Bohr\u2019s model is semi-classical because it combines the classical concept of electron orbit (postulate 1) with the new concept of quantization (postulates 2 and 3).<\/li>\r\n \t<li>Bohr\u2019s model of the hydrogen atom explains the emission and absorption spectra of atomic hydrogen and hydrogen-like ions with low atomic numbers. It was the first model to introduce the concept of a quantum number to describe atomic states and to postulate quantization of electron orbits in the atom. Bohr\u2019s model is an important step in the development of quantum mechanics, which deals with many-electron atoms.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163711943215\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"26515_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-5-de-broglies-matter-waves\/\"><span class=\"os-number\">2.5<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">De Broglie\u2019s Matter Waves<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1163712236546\" data-bullet-style=\"bullet\">\r\n \t<li>De Broglie\u2019s hypothesis of matter waves postulates that any particle of matter that has linear momentum is also a wave. The wavelength of a matter wave associated with a particle is inversely proportional to the magnitude of the particle\u2019s linear momentum. The speed of the matter wave is the speed of the particle.<\/li>\r\n \t<li>De Broglie\u2019s concept of the electron matter wave provides a rationale for the quantization of the electron\u2019s angular momentum in Bohr\u2019s model of the hydrogen atom.<\/li>\r\n \t<li>In the Davisson\u2013Germer experiment, electrons are scattered off a crystalline nickel surface. Diffraction patterns of electron matter waves are observed. They are the evidence for the existence of matter waves. Matter waves are observed in diffraction experiments with various particles.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163710885823\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"35633_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-6-wave-particle-duality\/\"><span class=\"os-number\">2.6<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Wave-Particle Duality<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1163712283956\" data-bullet-style=\"bullet\">\r\n \t<li>Wave-particle duality exists in nature: Under some experimental conditions, a particle acts as a particle; under other experimental conditions, a particle acts as a wave. Conversely, under some physical circumstances, electromagnetic radiation acts as a wave, and under other physical circumstances, radiation acts as a beam of photons.<\/li>\r\n \t<li>Modern-era double-slit experiments with electrons demonstrated conclusively that electron-diffraction images are formed because of the wave nature of electrons.<\/li>\r\n \t<li>The wave-particle dual nature of particles and of radiation has no classical explanation.<\/li>\r\n \t<li>Quantum theory takes the wave property to be the fundamental property of all particles. A particle is seen as a moving wave packet. The wave nature of particles imposes a limitation on the simultaneous measurement of the particle\u2019s position and momentum. Heisenberg\u2019s uncertainty principle sets the limits on precision in such simultaneous measurements.<\/li>\r\n \t<li>Wave-particle duality is exploited in many devices, such as charge-couple devices (used in digital cameras) or in the electron microscopy of the scanning electron microscope (SEM) and the transmission electron microscope (TEM).<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<\/div>\r\n<\/div>\r\n<div class=\"os-review-conceptual-questions-container\">\r\n<h3 data-type=\"title\"><span class=\"os-text\">Conceptual Questions<\/span><\/h3>\r\n<div class=\"os-review-conceptual-questions\">\r\n<div class=\"os-section-area\"><section id=\"fs-id1163709819728\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"88119_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-1-blackbody-radiation\/\"><span class=\"os-number\">2.1<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Blackbody Radiation<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709819734\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709819736\">\r\n\r\n1<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709819738\">Which surface has a higher temperature \u2013 the surface of a yellow star or that of a red star?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709819752\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709819754\">\r\n\r\n<span class=\"os-number\">2<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709819756\">Describe what you would see when looking at a body whose temperature is increased from 1000 K to 1,000,000 K.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709819769\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709819771\">\r\n\r\n3<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709819773\">Explain the color changes in a hot body as its temperature is increased.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709819785\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709819787\">\r\n\r\n<span class=\"os-number\">4<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709819789\">Speculate as to why UV light causes sunburn, whereas visible light does not.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709819801\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709819803\">\r\n\r\n5<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709819805\">Two cavity radiators are constructed with walls made of different metals. At the same temperature, how would their radiation spectra differ?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709819818\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709819820\">\r\n\r\n<span class=\"os-number\">6<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709819822\">Discuss why some bodies appear black, other bodies appear red, and still other bodies appear white.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709827902\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709827904\">\r\n\r\n7<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709827907\">If everything radiates electromagnetic energy, why can we not see objects at room temperature in a dark room?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709827919\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709827922\">\r\n\r\n<span class=\"os-number\">8<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709827924\">How much does the power radiated by a blackbody increase when its temperature (in K) is tripled?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163713203408\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"72890_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-2-photoelectric-effect\/\"><span class=\"os-number\">2.2<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Photoelectric Effect<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713204295\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713478150\">\r\n\r\n9<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713156825\">For the same monochromatic light source, would the photoelectric effect occur for all metals?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713254799\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713099944\">\r\n\r\n<span class=\"os-number\">10<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713187040\">In the interpretation of the photoelectric effect, how is it known that an electron does not absorb more than one photon?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713197187\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713514955\">\r\n\r\n11<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713012857\">Explain how you can determine the work function from a plot of the stopping potential versus the frequency of the incident radiation in a photoelectric effect experiment. Can you determine the value of Planck\u2019s constant from this plot?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713106682\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713124682\">\r\n\r\n<span class=\"os-number\">12<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713434458\">Suppose that in the photoelectric-effect experiment we make a plot of the detected current versus the applied potential difference. What information do we obtain from such a plot? Can we determine from it the value of Planck\u2019s constant? Can we determine the work function of the metal?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713249547\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713433113\">\r\n\r\n13<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709647064\">Speculate how increasing the temperature of a photoelectrode affects the outcomes of the photoelectric effect experiment.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709649099\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713263854\">\r\n\r\n<span class=\"os-number\">14<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713060000\">Which aspects of the photoelectric effect cannot be explained by classical physics?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709829775\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713244084\">\r\n\r\n15<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713195147\">Is the photoelectric effect a consequence of the wave character of radiation or is it a consequence of the particle character of radiation? Explain briefly.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713052738\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713128031\">\r\n\r\n<span class=\"os-number\">16<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713537655\">The metals sodium, iron, and molybdenum have work functions 2.5 eV, 3.9 eV, and 4.2 eV, respectively. Which of these metals will emit photoelectrons when illuminated with 400 nm light?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163709821272\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"31351_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-3-the-compton-effect\/\"><span class=\"os-number\">2.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">The Compton Effect<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713293360\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709749405\">\r\n\r\n17<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709749407\">Discuss any similarities and differences between the photoelectric and the Compton effects.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709829580\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709827936\">\r\n\r\n<span class=\"os-number\">18<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709827938\">Which has a greater momentum: an UV photon or an IR photon?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713271214\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713271216\">\r\n\r\n19<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713294182\">Does changing the intensity of a monochromatic light beam affect the momentum of the individual photons in the beam? Does such a change affect the net momentum of the beam?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713483610\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709653940\">\r\n\r\n<span class=\"os-number\">20<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709653942\">Can the Compton effect occur with visible light? If so, will it be detectable?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713431110\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713431112\">\r\n\r\n21<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709831568\">Is it possible in the Compton experiment to observe scattered X-rays that have a shorter wavelength than the incident X-ray radiation?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713146463\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713146466\">\r\n\r\n<span class=\"os-number\">22<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709678961\">Show that the Compton wavelength has the dimension of length.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713490619\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713490621\">\r\n\r\n23<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709827809\">At what scattering angle is the wavelength shift in the Compton effect equal to the Compton wavelength?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163711964260\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"67977_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-4-bohrs-model-of-the-hydrogen-atom\/\"><span class=\"os-number\">2.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Bohr\u2019s Model of the Hydrogen Atom<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713537489\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713537491\">\r\n\r\n<span class=\"os-number\">24<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709758434\">Explain why the patterns of bright emission spectral lines have an identical spectral position to the pattern of dark absorption spectral lines for a given gaseous element.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713268590\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713412975\">\r\n\r\n25<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713412977\">Do the various spectral lines of the hydrogen atom overlap?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713258490\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713258493\">\r\n\r\n<span class=\"os-number\">26<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713258495\">The Balmer series for hydrogen was discovered before either the Lyman or the Paschen series. Why?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713050499\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713050501\">\r\n\r\n27<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713050503\">When the absorption spectrum of hydrogen at room temperature is analyzed, absorption lines for the Lyman series are found, but none are found for the Balmer series. What does this tell us about the energy state of most hydrogen atoms at room temperature?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713253754\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713535568\">\r\n\r\n<span class=\"os-number\">28<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713535570\">Hydrogen accounts for about 75% by mass of the matter at the surfaces of most stars. However, the absorption lines of hydrogen are strongest (of highest intensity) in the spectra of stars with a surface temperature of about 9000 K. They are weaker in the sun spectrum and are essentially nonexistent in very hot (temperatures above 25,000 K) or rather cool (temperatures below 3500 K) stars. Speculate as to why surface temperature affects the hydrogen absorption lines that we observe.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713485376\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713485378\">\r\n\r\n29<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713485380\">Discuss the similarities and differences between Thomson\u2019s model of the hydrogen atom and Bohr\u2019s model of the hydrogen atom.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713243485\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713243487\">\r\n\r\n<span class=\"os-number\">30<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713243489\">Discuss the way in which Thomson\u2019s model is nonphysical. Support your argument with experimental evidence.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713163950\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713163953\">\r\n\r\n31<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713289669\">If, in a hydrogen atom, an electron moves to an orbit with a larger radius, does the energy of the hydrogen atom increase or decrease?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713289682\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713010187\">\r\n\r\n<span class=\"os-number\">32<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713010189\">How is the energy conserved when an atom makes a transition from a higher to a lower energy state?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713010201\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709832973\">\r\n\r\n33<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709832975\">Suppose an electron in a hydrogen atom makes a transition from the (<em data-effect=\"italics\">n+1<\/em>)th orbit to the<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th orbit. Is the wavelength of the emitted photon longer for larger values of<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>, or for smaller values of<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713556636\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713556638\">\r\n\r\n<span class=\"os-number\">34<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713556640\">Discuss why the allowed energies of the hydrogen atom are negative.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709648346\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709648348\">\r\n\r\n35<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709648350\">Can a hydrogen atom absorb a photon whose energy is greater than 13.6 eV?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713204150\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713204152\">\r\n\r\n<span class=\"os-number\">36<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713204155\">Why can you see through glass but not through wood?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709681324\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709681326\">\r\n\r\n37<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709681329\">Do gravitational forces have a significant effect on atomic energy levels?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709724857\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709724859\">\r\n\r\n<span class=\"os-number\">38<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709724861\">Show that Planck\u2019s constant has the dimensions of angular momentum.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163710834697\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"26515_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-5-de-broglies-matter-waves\/\"><span class=\"os-number\">2.5<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">De Broglie\u2019s Matter Waves<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712372433\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712372435\">\r\n\r\n39<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712317174\">Which type of radiation is most suitable for the observation of diffraction patterns on crystalline solids; radio waves, visible light, or X-rays? Explain.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163710839854\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163710839856\">\r\n\r\n<span class=\"os-number\">40<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712266047\">Speculate as to how the diffraction patterns of a typical crystal would be affected if<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-167-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3-rays<\/span><\/span><\/span><span>\u00a0<\/span>were used instead of X-rays.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712315666\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712315668\">\r\n\r\n41<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712176981\">If an electron and a proton are traveling at the same speed, which one has the shorter de Broglie wavelength?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712378474\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712378476\">\r\n\r\n<span class=\"os-number\">42<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712378478\">If a particle is accelerating, how does this affect its de Broglie wavelength?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712275347\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712315094\">\r\n\r\n43<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712315096\">Why is the wave-like nature of matter not observed every day for macroscopic objects?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163710834867\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163710834870\">\r\n\r\n<span class=\"os-number\">44<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710834872\">What is the wavelength of a neutron at rest? Explain.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710957721\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712249030\">\r\n\r\n45<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712249032\">Why does the setup of Davisson\u2013Germer experiment need to be enclosed in a vacuum chamber? Discuss what result you expect when the chamber is not evacuated.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163712354339\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"35633_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-6-wave-particle-duality\/\"><span class=\"os-number\">2.6<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Wave-Particle Duality<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712349462\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712349465\">\r\n\r\n<span class=\"os-number\">46<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712349467\">Give an example of an experiment in which light behaves as waves. Give an example of an experiment in which light behaves as a stream of photons.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712315786\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712315788\">\r\n\r\n47<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712353651\">Discuss: How does the interference of water waves differ from the interference of electrons? How are they analogous?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163710848660\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711933421\">\r\n\r\n<span class=\"os-number\">48<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711933423\">Give at least one argument in support of the matter-wave hypothesis.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712153601\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163710999019\">\r\n\r\n49<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710999021\">Give at least one argument in support of the particle-nature of radiation.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711953520\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711937978\">\r\n\r\n<span class=\"os-number\">50<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711937981\">Explain the importance of the Young double-slit experiment.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712144470\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712272274\">\r\n\r\n51<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712272276\">Does the Heisenberg uncertainty principle allow a particle to be at rest in a designated region in space?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711969685\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712382995\">\r\n\r\n<span class=\"os-number\">52<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712382997\">Can the de Broglie wavelength of a particle be known exactly?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710834186\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163710848906\">\r\n\r\n53<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710848908\">Do the photons of red light produce better resolution in a microscope than blue light photons? Explain.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711042258\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712317349\">\r\n\r\n<span class=\"os-number\">54<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712317352\">Discuss the main difference between an SEM and a TEM.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<\/div>\r\n<\/div>\r\n<div class=\"os-review-problems-container\">\r\n<h3 data-type=\"title\"><span class=\"os-text\">Problems<\/span><\/h3>\r\n<div class=\"os-review-problems\">\r\n<div class=\"os-section-area\"><section id=\"fs-id11637098279360\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"88119_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-1-blackbody-radiation\/\"><span class=\"os-number\">2.1<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Blackbody Radiation<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709827943\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709827945\">\r\n\r\n55<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709827947\">A 200-W heater emits a 1.5-\u00b5m radiation. (a) What value of the energy quantum does it emit? (b) Assuming that the specific heat of a 4.0-kg body is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-168-Frame\"><span class=\"MathJax_MathContainer\"><span>0.83kcal\/kg\u00b7K,<\/span><\/span><\/span><span>\u00a0<\/span>how many of these photons must be absorbed by the body to increase its temperature by 2 K? (c) How long does the heating process in (b) take, assuming that all radiation emitted by the heater gets absorbed by the body?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709830086\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709830088\">\r\n\r\n<span class=\"os-number\">56<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709830090\">A 900-W microwave generator in an oven generates energy quanta of frequency 2560 MHz. (a) How many energy quanta does it emit per second? (b) How many energy quanta must be absorbed by a pasta dish placed in the radiation cavity to increase its temperature by 45.0 K? Assume that the dish has a mass of 0.5 kg and that its specific heat is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-169-Frame\"><span class=\"MathJax_MathContainer\"><span>0.9kcal\/kg\u00b7K.<\/span><\/span><\/span><span>\u00a0<\/span>(c) Assume that all energy quanta emitted by the generator are absorbed by the pasta dish. How long must we wait until the dish in (b) is ready?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709830155\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709830157\">\r\n\r\n57<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709830160\">(a) For what temperature is the peak of blackbody radiation spectrum at 400 nm? (b) If the temperature of a blackbody is 800 K, at what wavelength does it radiate the most energy?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709830177\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709830179\">\r\n\r\n<span class=\"os-number\">58<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709830181\">The tungsten elements of incandescent light bulbs operate at 3200 K. At what frequency does the filament radiate maximum energy?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713537702\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713537704\">\r\n\r\n59<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713537706\">Interstellar space is filled with radiation of wavelength<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-170-Frame\"><span class=\"MathJax_MathContainer\"><span>970\u03bcm.<\/span><\/span><\/span><span>\u00a0<\/span>This radiation is considered to be a remnant of the \u201cbig bang.\u201d What is the corresponding blackbody temperature of this radiation?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713537725\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713537727\">\r\n\r\n<span class=\"os-number\">60<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713537729\">The radiant energy from the sun reaches its maximum at a wavelength of about 500.0 nm. What is the approximate temperature of the sun\u2019s surface?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163713276435\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"72890_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-2-photoelectric-effect\/\"><span class=\"os-number\">2.2<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Photoelectric Effect<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713427953\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713099928\">\r\n\r\n61<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713286730\">A photon has energy 20 keV. What are its frequency and wavelength?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713203684\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713160552\">\r\n\r\n<span class=\"os-number\">62<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713418745\">The wavelengths of visible light range from approximately 400 to 750 nm. What is the corresponding range of photon energies for visible light?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713089403\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713515015\">\r\n\r\n63<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713195273\">What is the longest wavelength of radiation that can eject a photoelectron from silver? Is it in the visible range?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713102973\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713006714\">\r\n\r\n<span class=\"os-number\">64<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713161402\">What is the longest wavelength of radiation that can eject a photoelectron from potassium, given the work function of potassium 2.24 eV? Is it in the visible range?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713044256\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713253944\">\r\n\r\n65<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713135648\">Estimate the binding energy of electrons in magnesium, given that the wavelength of 337 nm is the longest wavelength that a photon may have to eject a photoelectron from magnesium photoelectrode.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713287703\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713181348\">\r\n\r\n<span class=\"os-number\">66<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713260358\">The work function for potassium is 2.26 eV. What is the cutoff frequency when this metal is used as photoelectrode? What is the stopping potential when for the emitted electrons when this photoelectrode is exposed to radiation of frequency 1200 THz?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713181808\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713136812\">\r\n\r\n67<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709757529\">Estimate the work function of aluminum, given that the wavelength of 304 nm is the longest wavelength that a photon may have to eject a photoelectron from aluminum photoelectrode.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709666665\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709655949\">\r\n\r\n<span class=\"os-number\">68<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713009596\">What is the maximum kinetic energy of photoelectrons ejected from sodium by the incident radiation of wavelength 450 nm?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709681103\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713277885\">\r\n\r\n69<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713275799\">A 120-nm UV radiation illuminates a gold-plated electrode. What is the maximum kinetic energy of the ejected photoelectrons?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713123904\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713084917\">\r\n\r\n<span class=\"os-number\">70<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713181082\">A 400-nm violet light ejects photoelectrons with a maximum kinetic energy of 0.860 eV from sodium photoelectrode. What is the work function of sodium?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713125354\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713163493\">\r\n\r\n71<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713254262\">A 600-nm light falls on a photoelectric surface and electrons with the maximum kinetic energy of 0.17 eV are emitted. Determine (a) the work function and (b) the cutoff frequency of the surface. (c) What is the stopping potential when the surface is illuminated with light of wavelength 400 nm?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713275669\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713033157\">\r\n\r\n<span class=\"os-number\">72<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713009823\">The cutoff wavelength for the emission of photoelectrons from a particular surface is 500 nm. Find the maximum kinetic energy of the ejected photoelectrons when the surface is illuminated with light of wavelength 600 nm.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709668794\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713120255\">\r\n\r\n73<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713099793\">Find the wavelength of radiation that can eject 2.00-eV electrons from calcium electrode. The work function for calcium is 2.71 eV. In what range is this radiation?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713259069\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713424949\">\r\n\r\n<span class=\"os-number\">74<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713033129\">Find the wavelength of radiation that can eject 0.10-eV electrons from potassium electrode. The work function for potassium is 2.24 eV. In what range is this radiation?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713297676\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713067016\">\r\n\r\n75<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709733170\">Find the maximum velocity of photoelectrons ejected by an 80-nm radiation, if the work function of photoelectrode is 4.73 eV.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163713479845\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"31351_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-3-the-compton-effect\/\"><span class=\"os-number\">2.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">The Compton Effect<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709653867\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713427852\">\r\n\r\n<span class=\"os-number\">76<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713427854\">What is the momentum of a 589-nm yellow photon?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709700682\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713143241\">\r\n\r\n77<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713143243\">What is the momentum of a 4-cm microwave photon?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713184542\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713269350\">\r\n\r\n<span class=\"os-number\">78<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713269352\">In a beam of white light (wavelengths from 400 to 750 nm), what range of momentum can the photons have?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713438566\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713438568\">\r\n\r\n79<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713042337\">What is the energy of a photon whose momentum is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-171-Frame\"><span class=\"MathJax_MathContainer\"><span>3.0\u00d710\u221224kg\u00b7m\/s<\/span><\/span><\/span><span>\u00a0<\/span>?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713484828\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709676784\">\r\n\r\n<span class=\"os-number\">80<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709676786\">What is the wavelength of (a) a 12-keV X-ray photon; (b) a 2.0-MeV<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-172-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span>-ray photon?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709645515\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713053247\">\r\n\r\n81<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713053249\">Find the momentum and energy of a 1.0-\u00c5 photon.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713262171\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713262174\">\r\n\r\n<span class=\"os-number\">82<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713041547\">Find the wavelength and energy of a photon with momentum<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-173-Frame\"><span class=\"MathJax_MathContainer\"><span>5.00\u00d710\u221229kg\u00b7m\/s.<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713353953\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713487418\">\r\n\r\n83<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713487420\">A<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-174-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span>-ray photon has a momentum of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-175-Frame\"><span class=\"MathJax_MathContainer\"><span>8.00\u00d710\u221221kg\u00b7m\/s.<\/span><\/span><\/span><span>\u00a0<\/span>Find its wavelength and energy.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709832998\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713269708\">\r\n\r\n<span class=\"os-number\">84<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713269710\">(a) Calculate the momentum of a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-176-Frame\"><span class=\"MathJax_MathContainer\"><span>2.5-\u00b5m<\/span><\/span><\/span><span>\u00a0<\/span>photon. (b) Find the velocity of an electron with the same momentum. (c) What is the kinetic energy of the electron, and how does it compare to that of the photon?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713196802\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713196804\">\r\n\r\n85<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713196806\">Show that<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-177-Frame\"><span class=\"MathJax_MathContainer\"><span>p=h\/\u03bb<\/span><\/span><\/span><span>\u00a0<\/span>and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-178-Frame\"><span class=\"MathJax_MathContainer\"><span>Ef=hf<\/span><\/span><\/span><span>\u00a0<\/span>are consistent with the relativistic formula<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-179-Frame\"><span class=\"MathJax_MathContainer\"><span>E2=p2c2+m02c2.<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713263574\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713263576\">\r\n\r\n<span class=\"os-number\">86<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713263578\">Show that the energy<span>\u00a0<\/span><em data-effect=\"italics\">E<\/em><span>\u00a0<\/span>in eV of a photon is given by<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-180-Frame\"><span class=\"MathJax_MathContainer\"><span>E=1.241\u00d710\u22126eV\u00b7m\/\u03bb,<\/span><\/span><\/span><span>\u00a0<\/span>where<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-181-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bb<\/span><\/span><\/span><span>\u00a0<\/span>is its wavelength in meters.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713128336\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713128338\">\r\n\r\n87<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713128340\">For collisions with free electrons, compare the Compton shift of a photon scattered as an angle of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-182-Frame\"><span class=\"MathJax_MathContainer\"><span>30\u00b0<\/span><\/span><\/span><span>\u00a0<\/span>to that of a photon scattered at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-183-Frame\"><span class=\"MathJax_MathContainer\"><span>45\u00b0.<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713458514\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713458516\">\r\n\r\n<span class=\"os-number\">88<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709831535\">X-rays of wavelength 12.5 pm are scattered from a block of carbon. What are the wavelengths of photons scattered at (a)<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-184-Frame\"><span class=\"MathJax_MathContainer\"><span>30\u00b0;<\/span><\/span><\/span><span>\u00a0<\/span>(b)<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-185-Frame\"><span class=\"MathJax_MathContainer\"><span>90\u00b0;<\/span><\/span><\/span><span>\u00a0<\/span>and, (c)<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-186-Frame\"><span class=\"MathJax_MathContainer\"><span>180\u00b0<\/span><\/span><\/span><span>\u00a0<\/span>?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163709724868\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"67977_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-4-bohrs-model-of-the-hydrogen-atom\/\"><span class=\"os-number\">2.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Bohr\u2019s Model of the Hydrogen Atom<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713163833\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713163835\">\r\n\r\n89<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713163837\">Calculate the wavelength of the first line in the Lyman series and show that this line lies in the ultraviolet part of the spectrum.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709831664\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709831666\">\r\n\r\n<span class=\"os-number\">90<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709831668\">Calculate the wavelength of the fifth line in the Lyman series and show that this line lies in the ultraviolet part of the spectrum.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709827766\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709827768\">\r\n\r\n91<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709827770\">Calculate the energy changes corresponding to the transitions of the hydrogen atom: (a) from<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-187-Frame\"><span class=\"MathJax_MathContainer\"><span>n=3<\/span><\/span><\/span><span>\u00a0<\/span>to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-188-Frame\"><span class=\"MathJax_MathContainer\"><span>n=4;<\/span><\/span><\/span><span>\u00a0<\/span>(b) from<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-189-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2<\/span><\/span><\/span><span>\u00a0<\/span>to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-190-Frame\"><span class=\"MathJax_MathContainer\"><span>n=1;<\/span><\/span><\/span><span>\u00a0<\/span>and (c) from<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-191-Frame\"><span class=\"MathJax_MathContainer\"><span>n=3<\/span><\/span><\/span><span>\u00a0<\/span>to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-192-Frame\"><span class=\"MathJax_MathContainer\"><span>n=\u221e.<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713450603\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713450605\">\r\n\r\n<span class=\"os-number\">92<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713450607\">Determine the wavelength of the third Balmer line (transition from<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-193-Frame\"><span class=\"MathJax_MathContainer\"><span>n=5<\/span><\/span><\/span><span>\u00a0<\/span>to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-194-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2<\/span><\/span><\/span>).<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713429628\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713429630\">\r\n\r\n93<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713429632\">What is the frequency of the photon absorbed when the hydrogen atom makes the transition from the ground state to the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-195-Frame\"><span class=\"MathJax_MathContainer\"><span>n=4<\/span><\/span><\/span><span>\u00a0<\/span>state?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709829701\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709829703\">\r\n\r\n<span class=\"os-number\">94<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709829705\">When a hydrogen atom is in its ground state, what are the shortest and longest wavelengths of the photons it can absorb without being ionized?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713432792\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713432794\">\r\n\r\n95<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713432796\">When a hydrogen atom is in its third excided state, what are the shortest and longest wavelengths of the photons it can emit?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713284382\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713284384\">\r\n\r\n<span class=\"os-number\">96<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713284386\">What is the longest wavelength that light can have if it is to be capable of ionizing the hydrogen atom in its ground state?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713050379\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713050381\">\r\n\r\n97<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713050383\">For an electron in a hydrogen atom in the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-196-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2<\/span><\/span><\/span><span>\u00a0<\/span>state, compute: (a) the angular momentum; (b) the kinetic energy; (c) the potential energy; and (d) the total energy.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713246684\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713246686\">\r\n\r\n<span class=\"os-number\">98<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713246688\">Find the ionization energy of a hydrogen atom in the fourth energy state.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713557498\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713557500\">\r\n\r\n99<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713557502\">It has been measured that it required 0.850 eV to remove an electron from the hydrogen atom. In what state was the atom before the ionization happened?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713276597\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713276599\">\r\n\r\n<span class=\"os-number\">100<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713276601\">What is the radius of a hydrogen atom when the electron is in the first excited state?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713249475\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713249477\">\r\n\r\n101<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713249479\">Find the shortest wavelength in the Balmer series. In what part of the spectrum does this line lie?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713249491\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713517356\">\r\n\r\n<span class=\"os-number\">102<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713517358\">Show that the entire Paschen series lies in the infrared part of the spectrum.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713517363\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713517366\">\r\n\r\n103<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713517368\">Do the Balmer series and the Lyman series overlap? Why? Why not? (Hint: calculate the shortest Balmer line and the longest Lyman line.)<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713535613\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163713535615\">\r\n\r\n<span class=\"os-number\">104<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163713535617\">(a) Which line in the Balmer series is the first one in the UV part of the spectrum? (b) How many Balmer lines lie in the visible part of the spectrum? (c) How many Balmer lines lie in the UV?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709817720\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163709817722\">\r\n\r\n105<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163709817724\">A<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-197-Frame\"><span class=\"MathJax_MathContainer\"><span>4.653-\u03bcm<\/span><\/span><\/span><span>\u00a0<\/span>emission line of atomic hydrogen corresponds to transition between the states<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-198-Frame\"><span class=\"MathJax_MathContainer\"><span>nf=5<\/span><\/span><\/span><span>\u00a0<\/span>and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-199-Frame\"><span class=\"MathJax_MathContainer\"><span>ni.<\/span><\/span><\/span><span>\u00a0<\/span>Find<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-200-Frame\"><span class=\"MathJax_MathContainer\"><span>ni.<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163712190070\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"26515_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-5-de-broglies-matter-waves\/\"><span class=\"os-number\">2.5<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">De Broglie\u2019s Matter Waves<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712279890\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712084068\">\r\n\r\n<span class=\"os-number\">106<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712084071\">At what velocity will an electron have a wavelength of 1.00 m?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712315240\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712315242\">\r\n\r\n107<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712315244\">What is the de Broglie wavelength of an electron travelling at a speed of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-201-Frame\"><span class=\"MathJax_MathContainer\"><span>5.0\u00d7106m\/s<\/span><\/span><\/span><span>\u00a0<\/span>?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712098145\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712098147\">\r\n\r\n<span class=\"os-number\">108<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712098149\">What is the de Broglie wavelength of an electron that is accelerated from rest through a potential difference of 20 keV?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712314741\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711933634\">\r\n\r\n109<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711933636\">What is the de Broglie wavelength of a proton whose kinetic energy is 2.0 MeV? 10.0 MeV?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712413228\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712413230\">\r\n\r\n<span class=\"os-number\">110<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712090894\">What is the de Broglie wavelength of a 10-kg football player running at a speed of 8.0 m\/s?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712183285\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712183287\">\r\n\r\n111<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712183289\">(a) What is the energy of an electron whose de Broglie wavelength is that of a photon of yellow light with wavelength 590 nm? (b) What is the de Broglie wavelength of an electron whose energy is that of the photon of yellow light?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712079249\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712079251\">\r\n\r\n<span class=\"os-number\">112<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712079253\">The de Broglie wavelength of a neutron is 0.01 nm. What is the speed and energy of this neutron?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710974558\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163710974560\">\r\n\r\n113<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710974562\">What is the wavelength of an electron that is moving at a 3% of the speed of light?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712257074\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712257076\">\r\n\r\n<span class=\"os-number\">114<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712274557\">At what velocity does a proton have a 6.0-fm wavelength (about the size of a nucleus)? Give your answer in units of<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712094058\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712094060\">\r\n\r\n115<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710846624\">What is the velocity of a 0.400-kg billiard ball if its wavelength is 7.50 fm?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712374839\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712374841\">\r\n\r\n<span class=\"os-number\">116<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712374844\">Find the wavelength of a proton that is moving at 1.00% of the speed of light (when<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-202-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b2=0.01).<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1163710981804\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"35633_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-6-wave-particle-duality\/\"><span class=\"os-number\">2.6<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Wave-Particle Duality<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712311334\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712311336\">\r\n\r\n117<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712311338\">An AM radio transmitter radiates 500 kW at a frequency of 760 kHz. How many photons per second does the emitter emit?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711888093\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711939071\">\r\n\r\n<span class=\"os-number\">118<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711939073\">Find the Lorentz factor<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-203-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>and de Broglie\u2019s wavelength for a 50-GeV electron in a particle accelerator.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712316372\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712316374\">\r\n\r\n119<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712316376\">Find the Lorentz factor<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-204-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>and de Broglie\u2019s wavelength for a 1.0-TeV proton in a particle accelerator.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712284485\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712284487\">\r\n\r\n<span class=\"os-number\">120<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712284489\">What is the kinetic energy of a 0.01-nm electron in a TEM?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712090899\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163710770573\">\r\n\r\n121<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710770576\">If electron is to be diffracted significantly by a crystal, its wavelength must be about equal to the spacing,<span>\u00a0<\/span><em data-effect=\"italics\">d<\/em>, of crystalline planes. Assuming<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-205-Frame\"><span class=\"MathJax_MathContainer\"><span>d=0.250nm,<\/span><\/span><\/span><span>\u00a0<\/span>estimate the potential difference through which an electron must be accelerated from rest if it is to be diffracted by these planes.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163710892218\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163710892220\">\r\n\r\n<span class=\"os-number\">122<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712440493\">X-rays form ionizing radiation that is dangerous to living tissue and undetectable to the human eye. Suppose that a student researcher working in an X-ray diffraction laboratory is accidentally exposed to a fatal dose of radiation. Calculate the temperature increase of the researcher under the following conditions: the energy of X-ray photons is 200 keV and the researcher absorbs<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-206-Frame\"><span class=\"MathJax_MathContainer\"><span>4\u00d71013<\/span><\/span><\/span><span>\u00a0<\/span>photons per each kilogram of body weight during the exposure. Assume that the specific heat of the student\u2019s body is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-207-Frame\"><span class=\"MathJax_MathContainer\"><span>0.83kcal\/kg\u00b7K.<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710955242\"><section>\r\n<div data-type=\"problem\" id=\"fs-id11637123150940\">\r\n\r\n123<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id11637123150960\">Solar wind (radiation) that is incident on the top of Earth\u2019s atmosphere has an average intensity of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-208-Frame\"><span class=\"MathJax_MathContainer\"><span>1.3kW\/m2.<\/span><\/span><\/span><span>\u00a0<\/span>Suppose that you are building a solar sail that is to propel a small toy spaceship with a mass of 0.1 kg in the space between the International Space Station and the moon. The sail is made from a very light material, which perfectly reflects the incident radiation. To assess whether such a project is feasible, answer the following questions, assuming that radiation photons are incident only in normal direction to the sail reflecting surface. (a) What is the radiation pressure (force per<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-209-Frame\"><span class=\"MathJax_MathContainer\"><span>m2<\/span><\/span><\/span>) of the radiation falling on the mirror-like sail? (b) Given the radiation pressure computed in (a), what will be the acceleration of the spaceship when the sail has of an area of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-210-Frame\"><span class=\"MathJax_MathContainer\"><span>10.0m2<\/span><\/span><\/span><span>\u00a0<\/span>? (c) Given the acceleration estimate in (b), how fast will the spaceship be moving after 24 hours when it starts from rest?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711048465\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711048467\">\r\n\r\n<span class=\"os-number\">124<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711048469\">Treat the human body as a blackbody and determine the percentage increase in the total power of its radiation when its temperature increases from 98.6<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-211-Frame\"><span class=\"MathJax_MathContainer\"><span>\u00b0<\/span><\/span><\/span><span>\u00a0<\/span>F to 103<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-212-Frame\"><span class=\"MathJax_MathContainer\"><span>\u00b0<\/span><\/span><\/span><span>\u00a0<\/span>F.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711020632\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711020634\">\r\n\r\n125<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711020636\">Show that Wien\u2019s displacement law results from Planck\u2019s radiation law. (<em data-effect=\"italics\">Hint:<\/em><span>\u00a0<\/span>substitute<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-213-Frame\"><span class=\"MathJax_MathContainer\"><span>x=hc\/\u03bbkT<\/span><\/span><\/span><span>\u00a0<\/span>and write Planck\u2019s law in the form<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-214-Frame\"><span class=\"MathJax_MathContainer\"><span>I(x,T)=Ax5\/(ex\u22121),<\/span><\/span><\/span><span>\u00a0<\/span>where<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-215-Frame\"><span class=\"MathJax_MathContainer\"><span>A=2\u03c0(kT)5\/(h4c3).<\/span><\/span><\/span><span>\u00a0<\/span>Now, for fixed<span>\u00a0<\/span><em data-effect=\"italics\">T<\/em>, find the position of the maximum in<span>\u00a0<\/span><em data-effect=\"italics\">I<\/em>(<em data-effect=\"italics\">x<\/em>,<em data-effect=\"italics\">T<\/em>) by solving for<span>\u00a0<\/span><em data-effect=\"italics\">x<\/em>in the equation<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-216-Frame\"><span class=\"MathJax_MathContainer\"><span>dI(x,T)\/dx=0.<\/span><\/span><\/span>)<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711965492\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711965494\">\r\n\r\n<span class=\"os-number\">126<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712331421\">Show that Stefan\u2019s law results from Planck\u2019s radiation law.<span>\u00a0<\/span><em data-effect=\"italics\">Hint:<\/em><span>\u00a0<\/span>To compute the total power of blackbody radiation emitted across the entire spectrum of wavelengths at a given temperature, integrate Planck\u2019s law over the entire spectrum<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-217-Frame\"><span class=\"MathJax_MathContainer\"><span>P(T)=\u222b0\u221eI(\u03bb,T)d\u03bb.<\/span><\/span><\/span><span>\u00a0<\/span>Use the substitution<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-218-Frame\"><span class=\"MathJax_MathContainer\"><span>x=hc\/\u03bbkT<\/span><\/span><\/span><span>\u00a0<\/span>and the tabulated value of the integral<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-219-Frame\"><span class=\"MathJax_MathContainer\"><span>\u222b0\u221edxx3\/(ex\u22121)=\u03c04\/15.<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<\/div>\r\n<\/div>\r\n<div class=\"os-review-additional-problems-container\">\r\n<h3 data-type=\"title\"><span class=\"os-text\">Additional Problems<\/span><\/h3>\r\n<section id=\"fs-id1172101896308\" class=\"review-additional-problems\" data-depth=\"1\">\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712316432\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712316434\">\r\n\r\n127<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712224356\">Determine the power intensity of radiation per unit wavelength emitted at a wavelength of 500.0 nm by a blackbody at a temperature of 10,000 K.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163710983419\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163710983421\">\r\n\r\n<span class=\"os-number\">128<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710983423\">The HCl molecule oscillates at a frequency of 87.0 THz. What is the difference (in eV) between its adjacent energy levels?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711969237\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712320737\">\r\n\r\n129<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712320739\">A quantum mechanical oscillator vibrates at a frequency of 250.0 THz. What is the minimum energy of radiation it can emit?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711888302\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711888304\">\r\n\r\n<span class=\"os-number\">130<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712279583\">In about 5 billion years, the sun will evolve to a red giant. Assume that its surface temperature will decrease to about half its present value of 6000 K, while its present radius of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-220-Frame\"><span class=\"MathJax_MathContainer\"><span>7.0\u00d7108m<\/span><\/span><\/span><span>\u00a0<\/span>will increase to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-221-Frame\"><span class=\"MathJax_MathContainer\"><span>1.5\u00d71011m<\/span><\/span><\/span><span>\u00a0<\/span>(which is the current Earth-sun distance). Calculate the ratio of the total power emitted by the sun in its red giant stage to its present power.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712174458\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163710886364\">\r\n\r\n131<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710886366\">A sodium lamp emits 2.0 W of radiant energy, most of which has a wavelength of about 589 nm. Estimate the number of photons emitted per second by the lamp.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712182419\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711939088\">\r\n\r\n<span class=\"os-number\">132<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711939090\">Photoelectrons are ejected from a photoelectrode and are detected at a distance of 2.50 cm away from the photoelectrode. The work function of the photoelectrode is 2.71 eV and the incident radiation has a wavelength of 420 nm. How long does it take a photoelectron to travel to the detector?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710813976\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712430770\">\r\n\r\n133<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712430772\">If the work function of a metal is 3.2 eV, what is the maximum wavelength that a photon can have to eject a photoelectron from this metal surface?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712228772\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712228774\">\r\n\r\n<span class=\"os-number\">134<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712283826\">The work function of a photoelectric surface is 2.00 eV. What is the maximum speed of the photoelectrons emitted from this surface when a 450-nm light falls on it?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711941332\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711941334\">\r\n\r\n135<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710974559\">A 400-nm laser beam is projected onto a calcium electrode. The power of the laser beam is 2.00 mW and the work function of calcium is 2.31 eV. (a) How many photoelectrons per second are ejected? (b) What net power is carried away by photoelectrons?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712291539\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712291542\">\r\n\r\n<span class=\"os-number\">136<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712291544\">(a) Calculate the number of photoelectrons per second that are ejected from a 1.00-mm<sup>2<\/sup><span>\u00a0<\/span>area of sodium metal by a 500-nm radiation with intensity<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-222-Frame\"><span class=\"MathJax_MathContainer\"><span>1.30kW\/m2<\/span><\/span><\/span><span>\u00a0<\/span>(the intensity of sunlight above Earth\u2019s atmosphere). (b) Given the work function of the metal as 2.28 eV, what power is carried away by these photoelectrons?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712161001\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711990340\">\r\n\r\n137<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711990342\">A laser with a power output of 2.00 mW at a 400-nm wavelength is used to project a beam of light onto a calcium photoelectrode. (a) How many photoelectrons leave the calcium surface per second? (b) What power is carried away by ejected photoelectrons, given that the work function of calcium is 2.31 eV? (c) Calculate the photocurrent. (d) If the photoelectrode suddenly becomes electrically insulated and the setup of two electrodes in the circuit suddenly starts to act like a 2.00-pF capacitor, how long will current flow before the capacitor voltage stops it?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711987098\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711987100\">\r\n\r\n<span class=\"os-number\">138<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711976750\">The work function for barium is 2.48 eV. Find the maximum kinetic energy of the ejected photoelectrons when the barium surface is illuminated with: (a) radiation emitted by a 100-kW radio station broadcasting at 800 kHz; (b) a 633-nm laser light emitted from a powerful He-Ne laser; and (c) a 434-nm blue light emitted by a small hydrogen gas discharge tube.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712175615\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712175617\">\r\n\r\n139<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712282142\">(a) Calculate the wavelength of a photon that has the same momentum as a proton moving with 1% of the speed of light in a vacuum. (b) What is the energy of this photon in MeV? (c) What is the kinetic energy of the proton in MeV?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712131536\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712131538\">\r\n\r\n<span class=\"os-number\">140<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712131540\">(a) Find the momentum of a 100-keV X-ray photon. (b) Find the velocity of a neutron with the same momentum. (c) What is the neutron\u2019s kinetic energy in eV?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711983460\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712299629\">\r\n\r\n141<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712299631\">The momentum of light, as it is for particles, is exactly reversed when a photon is reflected straight back from a mirror, assuming negligible recoil of the mirror. The change in momentum is twice the photon\u2019s incident momentum, as it is for the particles. Suppose that a beam of light has an intensity<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-223-Frame\"><span class=\"MathJax_MathContainer\"><span>1.0kW\/m2<\/span><\/span><\/span><span>\u00a0<\/span>and falls on a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-224-Frame\"><span class=\"MathJax_MathContainer\"><span>\u22122.0-m2<\/span><\/span><\/span><span>\u00a0<\/span>area of a mirror and reflects from it. (a) Calculate the energy reflected in 1.00 s. (b) What is the momentum imparted to the mirror? (c) Use Newton\u2019s second law to find the force on the mirror. (d) Does the assumption of no-recoil for the mirror seem reasonable?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711918192\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712382607\">\r\n\r\n<span class=\"os-number\">142<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712382609\">A photon of energy 5.0 keV collides with a stationary electron and is scattered at an angle of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-225-Frame\"><span class=\"MathJax_MathContainer\"><span>60\u00b0.<\/span><\/span><\/span><span>\u00a0<\/span>What is the energy acquired by the electron in the collision?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712189962\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712189965\">\r\n\r\n143<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710887829\">A 0.75-nm photon is scattered by a stationary electron. The speed of the electron\u2019s recoil is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-226-Frame\"><span class=\"MathJax_MathContainer\"><span>1.5\u00d7106m\/s.<\/span><\/span><\/span><span>\u00a0<\/span>(a) Find the wavelength shift of the photon. (b) Find the scattering angle of the photon.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712090793\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712090795\">\r\n\r\n<span class=\"os-number\">144<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712090797\">Find the maximum change in X-ray wavelength that can occur due to Compton scattering. Does this change depend on the wavelength of the incident beam?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712404968\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712404970\">\r\n\r\n145<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711964258\">A photon of wavelength 700 nm is incident on a hydrogen atom. When this photon is absorbed, the atom becomes ionized. What is the lowest possible orbit that the electron could have occupied before being ionized?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712438121\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712438123\">\r\n\r\n<span class=\"os-number\">146<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712438125\">What is the maximum kinetic energy of an electron such that a collision between the electron and a stationary hydrogen atom in its ground state is definitely elastic?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710886894\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163710886896\">\r\n\r\n147<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163710886899\">Singly ionized atomic helium<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-227-Frame\"><span class=\"MathJax_MathContainer\"><span>He+1<\/span><\/span><\/span><span>\u00a0<\/span>is a hydrogen-like ion. (a) What is its ground-state radius? (b) Calculate the energies of its four lowest energy states. (c) Repeat the calculations for the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-228-Frame\"><span class=\"MathJax_MathContainer\"><span>Li2+<\/span><\/span><\/span><span>\u00a0<\/span>ion.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711954120\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711954122\">\r\n\r\n<span class=\"os-number\">148<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711954124\">A triply ionized atom of beryllium<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-229-Frame\"><span class=\"MathJax_MathContainer\"><span>Be3+<\/span><\/span><\/span><span>\u00a0<\/span>is a hydrogen-like ion. When<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-230-Frame\"><span class=\"MathJax_MathContainer\"><span>Be3+<\/span><\/span><\/span><span>\u00a0<\/span>is in one of its excited states, its radius in this<em data-effect=\"italics\">n<\/em>th state is exactly the same as the radius of the first Bohr orbit of hydrogen. Find<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em><span>\u00a0<\/span>and compute the ionization energy for this state of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-231-Frame\"><span class=\"MathJax_MathContainer\"><span>Be3+.<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712039267\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712081947\">\r\n\r\n149<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712081949\">In extreme-temperature environments, such as those existing in a solar corona, atoms may be ionized by undergoing collisions with other atoms. One example of such ionization in the solar corona is the presence of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-232-Frame\"><span class=\"MathJax_MathContainer\"><span>C5+<\/span><\/span><\/span><span>\u00a0<\/span>ions, detected in the Fraunhofer spectrum. (a) By what factor do the energies of the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-233-Frame\"><span class=\"MathJax_MathContainer\"><span>C5+<\/span><\/span><\/span><span>\u00a0<\/span>ion scale compare to the energy spectrum of a hydrogen atom? (b) What is the wavelength of the first line in the Paschen series of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-234-Frame\"><span class=\"MathJax_MathContainer\"><span>C5+<\/span><\/span><\/span><span>\u00a0<\/span>? (c) In what part of the spectrum are these lines located?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712236542\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712236544\">\r\n\r\n<span class=\"os-number\">150<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id11637122365460\">(a) Calculate the ionization energy for<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-235-Frame\"><span class=\"MathJax_MathContainer\"><span>He+.<\/span><\/span><\/span><span>\u00a0<\/span>(b) What is the minimum frequency of a photon capable of ionizing<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-236-Frame\"><span class=\"MathJax_MathContainer\"><span>He+<\/span><\/span><\/span><span>\u00a0<\/span>?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711964124\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711964126\">\r\n\r\n151<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711964128\">Experiments are performed with ultracold neutrons having velocities as small as 1.00 m\/s. Find the wavelength of such an ultracold neutron and its kinetic energy.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712274837\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712274839\">\r\n\r\n<span class=\"os-number\">152<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712274841\">Find the velocity and kinetic energy of a 6.0-fm neutron. (Rest mass energy of neutron is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-237-Frame\"><span class=\"MathJax_MathContainer\"><span>E0=940MeV.)<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712274363\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712274365\">\r\n\r\n153<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712278869\">The spacing between crystalline planes in the NaCl crystal is 0.281 nm, as determined by X-ray diffraction with X-rays of wavelength 0.170 nm. What is the energy of neutrons in the neutron beam that produces diffraction peaks at the same locations as the peaks obtained with the X-rays?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711937333\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711937335\">\r\n\r\n<span class=\"os-number\">154<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711964193\">What is the wavelength of an electron accelerated from rest in a 30.0-kV potential difference?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712316677\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712316680\">\r\n\r\n155<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712279283\">Calculate the velocity of a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-238-Frame\"><span class=\"MathJax_MathContainer\"><span>1.0-\u03bcm<\/span><\/span><\/span><span>\u00a0<\/span>electron and a potential difference used to accelerate it from rest to this velocity.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712274221\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712274223\">\r\n\r\n<span class=\"os-number\">156<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712274225\">In a supercollider at CERN, protons are accelerated to velocities of 0.25<em data-effect=\"italics\">c<\/em>. What are their wavelengths at this speed? What are their kinetic energies? If a beam of protons were to gain its kinetic energy in only one pass through a potential difference, how high would this potential difference have to be? (Rest mass energy of a proton is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-239-Frame\"><span class=\"MathJax_MathContainer\"><span>E0=938MeV).<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712317995\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712317998\">\r\n\r\n157<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712318000\">Find the de Broglie wavelength of an electron accelerated from rest in an X-ray tube in the potential difference of 100 keV. (Rest mass energy of an electron is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-240-Frame\"><span class=\"MathJax_MathContainer\"><span>E0=511keV.)<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712283645\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712283647\">\r\n\r\n<span class=\"os-number\">158<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712283650\">The cutoff wavelength for the emission of photoelectrons from a particular surface is 500 nm. Find the maximum kinetic energy of the ejected photoelectrons when the surface is illuminated with light of wavelength 450 nm.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712279098\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712279100\">\r\n\r\n159<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712279102\">Compare the wavelength shift of a photon scattered by a free electron to that of a photon scattered at the same angle by a free proton.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712236888\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712236890\">\r\n\r\n<span class=\"os-number\">160<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712236892\">The spectrometer used to measure the wavelengths of the scattered X-rays in the Compton experiment is accurate to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-241-Frame\"><span class=\"MathJax_MathContainer\"><span>5.0\u00d710\u22124nm.<\/span><\/span><\/span><span>\u00a0<\/span>What is the minimum scattering angle for which the X-rays interacting with the free electrons can be distinguished from those interacting with the atoms?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712240128\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712240130\">\r\n\r\n161<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712240132\">Consider a hydrogen-like ion where an electron is orbiting a nucleus that has charge<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-242-Frame\"><span class=\"MathJax_MathContainer\"><span>q=+Ze.<\/span><\/span><\/span><span>\u00a0<\/span>Derive the formulas for the energy<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-243-Frame\"><span class=\"MathJax_MathContainer\"><span>En<\/span><\/span><\/span><span>\u00a0<\/span>of the electron in<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th orbit and the orbital radius<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-244-Frame\"><span class=\"MathJax_MathContainer\"><span>rn.<\/span><\/span><\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712236459\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163712236461\">\r\n\r\n<span class=\"os-number\">162<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163712236463\">Assume that a hydrogen atom exists in the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-245-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2<\/span><\/span><\/span><span>\u00a0<\/span>excited state for<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-246-Frame\"><span class=\"MathJax_MathContainer\"><span>10\u22128s<\/span><\/span><\/span><span>\u00a0<\/span>before decaying to the ground state. How many times does the electron orbit the proton nucleus during this time? How long does it take Earth to orbit the sun this many times?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711991347\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1163711991350\">\r\n\r\n163<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1163711941154\">An atom can be formed when a negative muon is captured by a proton. The muon has the same charge as the electron and a mass 207 times that of the electron. Calculate the frequency of the photon emitted when this atom makes the transition from\u00a0<span class=\"MathJax_MathML\" id=\"MathJax-Element-247-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2\u00a0<\/span><\/span><\/span>to the<span class=\"MathJax_MathML\" id=\"MathJax-Element-248-Frame\"><span class=\"MathJax_MathContainer\"><span>n=1\u00a0<\/span><\/span><\/span>state. Assume that the muon is orbiting a stationary proton.<\/p>\r\n\r\n<\/div>\r\n&nbsp;\r\n<div class=\"textbox\"><em>Download for free at http:\/\/cnx.org\/contents\/af275420-6050-4707-995c-57b9cc13c358@11.1<\/em><\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>","rendered":"<div class=\"os-glossary-container\">\n<h3 data-type=\"title\"><span class=\"os-text\">Key Terms<\/span><\/h3>\n<dl id=\"fs-id1163709700583\">\n<dt id=\"38900\">absorber<\/dt>\n<dd id=\"fs-id1163713194408\">any object that absorbs radiation<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709818708\">\n<dt id=\"34524\">absorption spectrum<\/dt>\n<dd id=\"fs-id1163709818714\">wavelengths of absorbed radiation by atoms and molecules<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709837130\">\n<dt id=\"67087\">Balmer formula<\/dt>\n<dd id=\"fs-id1163709837136\">describes the emission spectrum of a hydrogen atom in the visible-light range<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709837140\">\n<dt id=\"70041\">Balmer series<\/dt>\n<dd id=\"fs-id1163709837145\">spectral lines corresponding to electron transitions to\/from the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-124-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2<\/span><\/span><\/span><span>\u00a0<\/span>state of the hydrogen atom, described by the Balmer formula<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713181127\">\n<dt id=\"74438\">blackbody<\/dt>\n<dd id=\"fs-id1163713162382\">perfect absorber\/emitter<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713260316\">\n<dt id=\"26227\">blackbody radiation<\/dt>\n<dd id=\"fs-id1163709827773\">radiation emitted by a blackbody<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709679234\">\n<dt id=\"70475\">Bohr radius of hydrogen<\/dt>\n<dd id=\"fs-id1163709679239\">radius of the first Bohr\u2019s orbit<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713535514\">\n<dt id=\"1201\">Bohr\u2019s model of the hydrogen atom<\/dt>\n<dd id=\"fs-id1163713535519\">first quantum model to explain emission spectra of hydrogen<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713535523\">\n<dt id=\"89547\">Brackett series<\/dt>\n<dd id=\"fs-id1163713535528\">spectral lines corresponding to electron transitions to\/from the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-125-Frame\"><span class=\"MathJax_MathContainer\"><span>n=4<\/span><\/span><\/span><span>\u00a0<\/span>state<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709829681\">\n<dt id=\"87316\">Compton effect<\/dt>\n<dd id=\"fs-id1163713439061\">the change in wavelength when an X-ray is scattered by its interaction with some materials<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713439065\">\n<dt id=\"97677\">Compton shift<\/dt>\n<dd id=\"fs-id1163713494397\">difference between the wavelengths of the incident X-ray and the scattered X-ray<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713277248\">\n<dt id=\"46976\">Compton wavelength<\/dt>\n<dd id=\"fs-id1163713256937\">physical constant with the value<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-126-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bbc=2.43pm<\/span><\/span><\/span><\/dd>\n<\/dl>\n<dl id=\"fs-id1163709827827\">\n<dt id=\"57397\">cut-off frequency<\/dt>\n<dd id=\"fs-id1163713294290\">frequency of incident light below which the photoelectric effect does not occur<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713259107\">\n<dt id=\"67259\">cut-off wavelength<\/dt>\n<dd id=\"fs-id1163713090752\">wavelength of incident light that corresponds to cut-off frequency<\/dd>\n<\/dl>\n<dl id=\"fs-id1163710830368\">\n<dt id=\"82213\">Davisson\u2013Germer experiment<\/dt>\n<dd id=\"fs-id1163710830374\">historically first electron-diffraction experiment that revealed electron waves<\/dd>\n<\/dl>\n<dl id=\"fs-id1163711969341\">\n<dt id=\"56615\">de Broglie wave<\/dt>\n<dd id=\"fs-id1163711969346\">matter wave associated with any object that has mass and momentum<\/dd>\n<\/dl>\n<dl id=\"fs-id1163712141867\">\n<dt id=\"1423\">de Broglie\u2019s hypothesis of matter waves<\/dt>\n<dd id=\"fs-id1163712189037\">particles of matter can behave like waves<\/dd>\n<\/dl>\n<dl id=\"fs-id1163711970261\">\n<dt id=\"8163\">double-slit interference experiment<\/dt>\n<dd id=\"fs-id1163711970266\">Young\u2019s double-slit experiment, which shows the interference of waves<\/dd>\n<\/dl>\n<dl id=\"fs-id1163712284810\">\n<dt id=\"64083\">electron microscopy<\/dt>\n<dd id=\"fs-id1163712272767\">microscopy that uses electron waves to \u201csee\u201d fine details of nano-size objects<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713513317\">\n<dt id=\"96405\">emission spectrum<\/dt>\n<dd id=\"fs-id1163713513322\">wavelengths of emitted radiation by atoms and molecules<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713244844\">\n<dt id=\"41670\">emitter<\/dt>\n<dd id=\"fs-id1163713254613\">any object that emits radiation<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713488861\">\n<dt id=\"35284\">energy of a photon<\/dt>\n<dd id=\"fs-id1163709786938\">quantum of radiant energy, depends only on a photon\u2019s frequency<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713513327\">\n<dt id=\"42254\">energy spectrum of hydrogen<\/dt>\n<dd id=\"fs-id1163713513332\">set of allowed discrete energies of an electron in a hydrogen atom<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713513336\">\n<dt id=\"84251\">excited energy states of the H atom<\/dt>\n<dd id=\"fs-id1163713195307\">energy state other than the ground state<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713195311\">\n<dt id=\"53944\">Fraunhofer lines<\/dt>\n<dd id=\"fs-id1163713195316\">dark absorption lines in the continuum solar emission spectrum<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713430117\">\n<dt id=\"69690\">ground state energy of the hydrogen atom<\/dt>\n<dd id=\"fs-id1163713430122\">energy of an electron in the first Bohr orbit of the hydrogen atom<\/dd>\n<\/dl>\n<dl id=\"fs-id1163711997462\">\n<dt id=\"41779\">group velocity<\/dt>\n<dd id=\"fs-id1163712272028\">velocity of a wave, energy travels with the group velocity<\/dd>\n<\/dl>\n<dl id=\"fs-id1163712272772\">\n<dt id=\"14467\">Heisenberg uncertainty principle<\/dt>\n<dd id=\"fs-id1163711057547\">sets the limits on precision in simultaneous measurements of momentum and position of a particle<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713430127\">\n<dt id=\"32158\">Humphreys series<\/dt>\n<dd id=\"fs-id1163713430132\">spectral lines corresponding to electron transitions to\/from the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-127-Frame\"><span class=\"MathJax_MathContainer\"><span>n=6<\/span><\/span><\/span><span>\u00a0<\/span>state<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709831628\">\n<dt id=\"75762\">hydrogen-like atom<\/dt>\n<dd id=\"fs-id1163709831633\">ionized atom with one electron remaining and nucleus with charge<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-128-Frame\"><span class=\"MathJax_MathContainer\"><span>+Ze<\/span><\/span><\/span><\/dd>\n<\/dl>\n<dl id=\"fs-id1163713424856\">\n<dt id=\"25461\">inelastic scattering<\/dt>\n<dd id=\"fs-id1163709820901\">scattering effect where kinetic energy is not conserved but the total energy is conserved<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709831646\">\n<dt id=\"23041\">ionization energy<\/dt>\n<dd id=\"fs-id1163709831651\">energy needed to remove an electron from an atom<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713557561\">\n<dt id=\"80790\">ionization limit of the hydrogen atom<\/dt>\n<dd id=\"fs-id1163713557566\">ionization energy needed to remove an electron from the first Bohr orbit<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713557570\">\n<dt id=\"99786\">Lyman series<\/dt>\n<dd id=\"fs-id1163713557576\">spectral lines corresponding to electron transitions to\/from the ground state<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713557580\">\n<dt id=\"72397\">nuclear model of the atom<\/dt>\n<dd id=\"fs-id1163713557585\">heavy positively charged nucleus at the center is surrounded by electrons, proposed by Rutherford<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709821220\">\n<dt id=\"76244\">Paschen series<\/dt>\n<dd id=\"fs-id1163709821226\">spectral lines corresponding to electron transitions to\/from the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-129-Frame\"><span class=\"MathJax_MathContainer\"><span>n=3<\/span><\/span><\/span><span>\u00a0<\/span>state<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709821239\">\n<dt id=\"96940\">Pfund series<\/dt>\n<dd id=\"fs-id1163713513434\">spectral lines corresponding to electron transitions to\/from the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-130-Frame\"><span class=\"MathJax_MathContainer\"><span>n=5<\/span><\/span><\/span><span>\u00a0<\/span>state<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713245842\">\n<dt id=\"79763\">photocurrent<\/dt>\n<dd id=\"fs-id1163709681087\">in a circuit, current that flows when a photoelectrode is illuminated<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713168168\">\n<dt id=\"54615\">photoelectric effect<\/dt>\n<dd id=\"fs-id1163713483006\">emission of electrons from a metal surface exposed to electromagnetic radiation of the proper frequency<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713425106\">\n<dt id=\"39602\">photoelectrode<\/dt>\n<dd id=\"fs-id1163713186641\">in a circuit, an electrode that emits photoelectrons<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713487413\">\n<dt id=\"78164\">photoelectron<\/dt>\n<dd id=\"fs-id1163713052088\">electron emitted from a metal surface in the presence of incident radiation<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713265704\">\n<dt id=\"54813\">photon<\/dt>\n<dd id=\"fs-id1163713157310\">particle of light<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713284371\">\n<dt id=\"57522\">Planck\u2019s hypothesis of energy quanta<\/dt>\n<dd id=\"fs-id1163709749887\">energy exchanges between the radiation and the walls take place only in the form of discrete energy quanta<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713513448\">\n<dt id=\"80262\">postulates of Bohr\u2019s model<\/dt>\n<dd id=\"fs-id1163713513454\">three assumptions that set a frame for Bohr\u2019s model<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713195295\">\n<dt id=\"80462\">power intensity<\/dt>\n<dd id=\"fs-id1163713087536\">energy that passes through a unit surface per unit time<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709820905\">\n<dt id=\"87582\">propagation vector<\/dt>\n<dd id=\"fs-id1163709749388\">vector with magnitude<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-131-Frame\"><span class=\"MathJax_MathContainer\"><span>2\u03c0\/\u03bb<\/span><\/span><\/span><span>\u00a0<\/span>that has the direction of the photon\u2019s linear momentum<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713071482\">\n<dt id=\"47059\">quantized energies<\/dt>\n<dd id=\"fs-id1163713310319\">discrete energies; not continuous<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713513459\">\n<dt id=\"997\">quantum number<\/dt>\n<dd id=\"fs-id1163713537359\">index that enumerates energy levels<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713033139\">\n<dt id=\"84074\">quantum phenomenon<\/dt>\n<dd id=\"fs-id1163713285340\">in interaction with matter, photon transfers either all its energy or nothing<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713275667\">\n<dt id=\"88162\">quantum state of a Planck\u2019s oscillator<\/dt>\n<dd id=\"fs-id1163713053248\">any mode of vibration of Planck\u2019s oscillator, enumerated by quantum number<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713282962\">\n<dt id=\"85834\">reduced Planck\u2019s constant<\/dt>\n<dd id=\"fs-id1163713443510\">Planck\u2019s constant divided by<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-132-Frame\"><span class=\"MathJax_MathContainer\"><span>2\u03c0<\/span><\/span><\/span><\/dd>\n<\/dl>\n<dl id=\"fs-id1163713537364\">\n<dt id=\"24660\">Rutherford\u2019s gold foil experiment<\/dt>\n<dd id=\"fs-id1163713537369\">first experiment to demonstrate the existence of the atomic nucleus<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713537373\">\n<dt id=\"91911\">Rydberg constant for hydrogen<\/dt>\n<dd id=\"fs-id1163713537379\">physical constant in the Balmer formula<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713537383\">\n<dt id=\"88424\">Rydberg formula<\/dt>\n<dd id=\"fs-id1163713537388\">experimentally found positions of spectral lines of hydrogen atom<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709826798\">\n<dt id=\"84253\">scattering angle<\/dt>\n<dd id=\"fs-id1163713525567\">angle between the direction of the scattered beam and the direction of the incident beam<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709682154\">\n<dt id=\"49732\">Stefan\u2013Boltzmann constant<\/dt>\n<dd id=\"fs-id1163709827755\">physical constant in Stefan\u2019s law<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709663034\">\n<dt id=\"91605\">stopping potential<\/dt>\n<dd id=\"fs-id1163713120926\">in a circuit, potential difference that stops photocurrent<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713427847\">\n<dt id=\"41511\">wave number<\/dt>\n<dd id=\"fs-id1163713267196\">magnitude of the propagation vector<\/dd>\n<\/dl>\n<dl id=\"fs-id1163712082745\">\n<dt id=\"84498\">wave quantum mechanics<\/dt>\n<dd id=\"fs-id1163712082751\">theory that explains the physics of atoms and subatomic particles<\/dd>\n<\/dl>\n<dl id=\"fs-id1163711057551\">\n<dt id=\"47746\">wave-particle duality<\/dt>\n<dd id=\"fs-id1163712273108\">particles can behave as waves and radiation can behave as particles<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713432868\">\n<dt id=\"72630\">work function<\/dt>\n<dd id=\"fs-id1163713536679\">energy needed to detach photoelectron from the metal surface<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713120574\">\n<dt id=\"52612\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-133-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b1<\/span><\/span><\/span>-particle<\/dt>\n<dd id=\"fs-id1163713120583\">doubly ionized helium atom<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713120587\">\n<dt id=\"84734\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-134-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b1<\/span><\/span><\/span>-ray<\/dt>\n<dd id=\"fs-id1163713120595\">beam of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-135-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b1<\/span><\/span><\/span>-particles (alpha-particles)<\/dd>\n<\/dl>\n<dl id=\"fs-id1163709679224\">\n<dt id=\"70017\">\u03b2-ray<\/dt>\n<dd id=\"fs-id1163709679229\">beam of electrons<\/dd>\n<\/dl>\n<dl id=\"fs-id1163713195320\">\n<dt id=\"84006\">\u03b3-ray<\/dt>\n<dd id=\"fs-id1163713195326\">beam of highly energetic photons<\/dd>\n<\/dl>\n<\/div>\n<div class=\"os-key-equations-container\">\n<h3 data-type=\"title\"><span class=\"os-text\">Key Equations<\/span><\/h3>\n<section id=\"fs-id1163710783174\" class=\"key-equations\" data-depth=\"1\">\n<div class=\"os-table\">\n<table id=\"fs-id1172097547296\" class=\"unnumbered unstyled\" summary=\"Table 6.1\" data-label=\"\">\n<tbody>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Wien\u2019s displacement law<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-136-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bbmaxT=2.898\u00d710\u22123m\u22c5K<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Stefan\u2019s law<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-137-Frame\"><span class=\"MathJax_MathContainer\"><span>P(T)=\u03c3AT4<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Planck\u2019s constant<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-138-Frame\"><span class=\"MathJax_MathContainer\"><span>h=6.626\u00d710\u221234J\u22c5s=4.136\u00d710\u221215eV\u22c5s<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Energy quantum of radiation<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-139-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394E=hf<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Planck\u2019s blackbody radiation law<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-140-Frame\"><span class=\"MathJax_MathContainer\"><span>I(\u03bb,T)=2\u03c0hc2\u03bb51ehc\/\u03bbkBT\u22121<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Maximum kinetic energy<span data-type=\"newline\"><br \/>\n<\/span>of a photoelectron<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-141-Frame\"><span class=\"MathJax_MathContainer\"><span>Kmax=e\u0394Vs<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Energy of a photon<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-142-Frame\"><span class=\"MathJax_MathContainer\"><span>Ef=hf<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Energy balance for photoelectron<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-143-Frame\"><span class=\"MathJax_MathContainer\"><span>Kmax=hf\u2212\u03d5<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Cut-off frequency<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-144-Frame\"><span class=\"MathJax_MathContainer\"><span>fc=\u03d5h<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Relativistic invariant<span data-type=\"newline\"><br \/>\n<\/span>energy equation<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-145-Frame\"><span class=\"MathJax_MathContainer\"><span>E2=p2c2+m02c4<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Energy-momentum relation<span data-type=\"newline\"><br \/>\n<\/span>for photon<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-146-Frame\"><span class=\"MathJax_MathContainer\"><span>pf=Efc<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Energy of a photon<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-147-Frame\"><span class=\"MathJax_MathContainer\"><span>Ef=hf=hc\u03bb<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Magnitude of photon\u2019s momentum<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-148-Frame\"><span class=\"MathJax_MathContainer\"><span>pf=h\u03bb<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Photon\u2019s linear<span data-type=\"newline\"><br \/>\n<\/span>momentum vector<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-149-Frame\"><span class=\"MathJax_MathContainer\"><span>p\u2192f=\u210fk\u2192<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">The Compton wavelength<span data-type=\"newline\"><br \/>\n<\/span>of an electron<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-150-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bbc=hm0c=0.00243nm<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">The Compton shift<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-151-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394\u03bb=\u03bbc(1\u2212cos\u03b8)<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">The Balmer formula<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-152-Frame\"><span class=\"MathJax_MathContainer\"><span>1\u03bb=RH(122\u22121n2)<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">The Rydberg formula<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-153-Frame\"><span class=\"MathJax_MathContainer\"><span>1\u03bb=RH(1nf2\u22121ni2),ni=nf+1,nf+2,\u2026<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Bohr\u2019s first quantization condition<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-154-Frame\"><span class=\"MathJax_MathContainer\"><span>Ln=n\u210f,n=1,2,\u2026<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Bohr\u2019s second quantization condition<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-155-Frame\"><span class=\"MathJax_MathContainer\"><span>hf=|En\u2212Em|<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Bohr\u2019s radius of hydrogen<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-156-Frame\"><span class=\"MathJax_MathContainer\"><span>a0=4\u03c0\u03b50\u210f2mee2=0.529\u00c5<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Bohr\u2019s radius of the<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th orbit<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-157-Frame\"><span class=\"MathJax_MathContainer\"><span>rn=a0n2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Ground-state energy value,<span data-type=\"newline\"><br \/>\n<\/span>ionization limit<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-158-Frame\"><span class=\"MathJax_MathContainer\"><span>E0=18\u03b502mee4h2=13.6eV<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Electron\u2019s energy in<span data-type=\"newline\"><br \/>\n<\/span>the<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th orbit<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-159-Frame\"><span class=\"MathJax_MathContainer\"><span>En=\u2212E01n2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Ground state energy of<span data-type=\"newline\"><br \/>\n<\/span>hydrogen<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-160-Frame\"><span class=\"MathJax_MathContainer\"><span>E1=\u2212E0=\u221213.6eV<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">The<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th orbit of<span data-type=\"newline\"><br \/>\n<\/span>hydrogen-like ion<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-161-Frame\"><span class=\"MathJax_MathContainer\"><span>rn=a0Zn2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">The<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th energy<span data-type=\"newline\"><br \/>\n<\/span>of hydrogen-like ion<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-162-Frame\"><span class=\"MathJax_MathContainer\"><span>En=\u2212Z2E01n2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Energy of a matter wave<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-163-Frame\"><span class=\"MathJax_MathContainer\"><span>E=hf<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">The de Broglie wavelength<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-164-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bb=hp<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">The frequency-wavelength relation<span data-type=\"newline\"><br \/>\n<\/span>for matter waves<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-165-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bbf=c\u03b2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr valign=\"top\">\n<td data-align=\"left\" data-valign=\"top\">Heisenberg\u2019s uncertainty principle<\/td>\n<td data-align=\"left\" data-valign=\"top\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-166-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394x\u0394p\u226512\u210f<\/span><\/span><\/span><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-key-concepts-container\">\n<h3 data-type=\"title\"><span class=\"os-text\">Summary<\/span><\/h3>\n<div class=\"os-key-concepts\">\n<div class=\"os-section-area\">\n<section id=\"fs-id1163709676722\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"88119_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-1-blackbody-radiation\/\"><span class=\"os-number\">2.1<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Blackbody Radiation<\/span><\/a><\/h4>\n<ul id=\"fs-id1163709676729\" data-bullet-style=\"bullet\">\n<li>All bodies radiate energy. The amount of radiation a body emits depends on its temperature. The experimental Wien\u2019s displacement law states that the hotter the body, the shorter the wavelength corresponding to the emission peak in the radiation curve. The experimental Stefan\u2019s law states that the total power of radiation emitted across the entire spectrum of wavelengths at a given temperature is proportional to the fourth power of the Kelvin temperature of the radiating body.<\/li>\n<li>Absorption and emission of radiation are studied within the model of a blackbody. In the classical approach, the exchange of energy between radiation and cavity walls is continuous. The classical approach does not explain the blackbody radiation curve.<\/li>\n<li>To explain the blackbody radiation curve, Planck assumed that the exchange of energy between radiation and cavity walls takes place only in discrete quanta of energy. Planck\u2019s hypothesis of energy quanta led to the theoretical Planck\u2019s radiation law, which agrees with the experimental blackbody radiation curve; it also explains Wien\u2019s and Stefan\u2019s laws.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163713129978\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"72890_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-2-photoelectric-effect\/\"><span class=\"os-number\">2.2<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Photoelectric Effect<\/span><\/a><\/h4>\n<ul id=\"fs-id1163713120118\" data-bullet-style=\"bullet\">\n<li>The photoelectric effect occurs when photoelectrons are ejected from a metal surface in response to monochromatic radiation incident on the surface. It has three characteristics: (1) it is instantaneous, (2) it occurs only when the radiation is above a cut-off frequency, and (3) kinetic energies of photoelectrons at the surface do not depend of the intensity of radiation. The photoelectric effect cannot be explained by classical theory.<\/li>\n<li>We can explain the photoelectric effect by assuming that radiation consists of photons (particles of light). Each photon carries a quantum of energy. The energy of a photon depends only on its frequency, which is the frequency of the radiation. At the surface, the entire energy of a photon is transferred to one photoelectron.<\/li>\n<li>The maximum kinetic energy of a photoelectron at the metal surface is the difference between the energy of the incident photon and the work function of the metal. The work function is the binding energy of electrons to the metal surface. Each metal has its own characteristic work function.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163713523834\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"31351_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-3-the-compton-effect\/\"><span class=\"os-number\">2.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">The Compton Effect<\/span><\/a><\/h4>\n<ul id=\"fs-id1163709750002\" data-bullet-style=\"bullet\">\n<li>In the Compton effect, X-rays scattered off some materials have different wavelengths than the wavelength of the incident X-rays. This phenomenon does not have a classical explanation.<\/li>\n<li>The Compton effect is explained by assuming that radiation consists of photons that collide with weakly bound electrons in the target material. Both electron and photon are treated as relativistic particles. Conservation laws of the total energy and of momentum are obeyed in collisions.<\/li>\n<li>Treating the photon as a particle with momentum that can be transferred to an electron leads to a theoretical Compton shift that agrees with the wavelength shift measured in the experiment. This provides evidence that radiation consists of photons.<\/li>\n<li>Compton scattering is an inelastic scattering, in which scattered radiation has a longer wavelength than that of incident radiation.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163713328376\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"67977_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-4-bohrs-model-of-the-hydrogen-atom\/\"><span class=\"os-number\">2.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Bohr\u2019s Model of the Hydrogen Atom<\/span><\/a><\/h4>\n<ul id=\"fs-id1163713328382\" data-bullet-style=\"bullet\">\n<li>Positions of absorption and emission lines in the spectrum of atomic hydrogen are given by the experimental Rydberg formula. Classical physics cannot explain the spectrum of atomic hydrogen.<\/li>\n<li>The Bohr model of hydrogen was the first model of atomic structure to correctly explain the radiation spectra of atomic hydrogen. It was preceded by the Rutherford nuclear model of the atom. In Rutherford\u2019s model, an atom consists of a positively charged point-like nucleus that contains almost the entire mass of the atom and of negative electrons that are located far away from the nucleus.<\/li>\n<li>Bohr\u2019s model of the hydrogen atom is based on three postulates: (1) an electron moves around the nucleus in a circular orbit, (2) an electron\u2019s angular momentum in the orbit is quantized, and (3) the change in an electron\u2019s energy as it makes a quantum jump from one orbit to another is always accompanied by the emission or absorption of a photon. Bohr\u2019s model is semi-classical because it combines the classical concept of electron orbit (postulate 1) with the new concept of quantization (postulates 2 and 3).<\/li>\n<li>Bohr\u2019s model of the hydrogen atom explains the emission and absorption spectra of atomic hydrogen and hydrogen-like ions with low atomic numbers. It was the first model to introduce the concept of a quantum number to describe atomic states and to postulate quantization of electron orbits in the atom. Bohr\u2019s model is an important step in the development of quantum mechanics, which deals with many-electron atoms.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163711943215\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"26515_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-5-de-broglies-matter-waves\/\"><span class=\"os-number\">2.5<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">De Broglie\u2019s Matter Waves<\/span><\/a><\/h4>\n<ul id=\"fs-id1163712236546\" data-bullet-style=\"bullet\">\n<li>De Broglie\u2019s hypothesis of matter waves postulates that any particle of matter that has linear momentum is also a wave. The wavelength of a matter wave associated with a particle is inversely proportional to the magnitude of the particle\u2019s linear momentum. The speed of the matter wave is the speed of the particle.<\/li>\n<li>De Broglie\u2019s concept of the electron matter wave provides a rationale for the quantization of the electron\u2019s angular momentum in Bohr\u2019s model of the hydrogen atom.<\/li>\n<li>In the Davisson\u2013Germer experiment, electrons are scattered off a crystalline nickel surface. Diffraction patterns of electron matter waves are observed. They are the evidence for the existence of matter waves. Matter waves are observed in diffraction experiments with various particles.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163710885823\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"35633_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-6-wave-particle-duality\/\"><span class=\"os-number\">2.6<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Wave-Particle Duality<\/span><\/a><\/h4>\n<ul id=\"fs-id1163712283956\" data-bullet-style=\"bullet\">\n<li>Wave-particle duality exists in nature: Under some experimental conditions, a particle acts as a particle; under other experimental conditions, a particle acts as a wave. Conversely, under some physical circumstances, electromagnetic radiation acts as a wave, and under other physical circumstances, radiation acts as a beam of photons.<\/li>\n<li>Modern-era double-slit experiments with electrons demonstrated conclusively that electron-diffraction images are formed because of the wave nature of electrons.<\/li>\n<li>The wave-particle dual nature of particles and of radiation has no classical explanation.<\/li>\n<li>Quantum theory takes the wave property to be the fundamental property of all particles. A particle is seen as a moving wave packet. The wave nature of particles imposes a limitation on the simultaneous measurement of the particle\u2019s position and momentum. Heisenberg\u2019s uncertainty principle sets the limits on precision in such simultaneous measurements.<\/li>\n<li>Wave-particle duality is exploited in many devices, such as charge-couple devices (used in digital cameras) or in the electron microscopy of the scanning electron microscope (SEM) and the transmission electron microscope (TEM).<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"os-review-conceptual-questions-container\">\n<h3 data-type=\"title\"><span class=\"os-text\">Conceptual Questions<\/span><\/h3>\n<div class=\"os-review-conceptual-questions\">\n<div class=\"os-section-area\">\n<section id=\"fs-id1163709819728\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"88119_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-1-blackbody-radiation\/\"><span class=\"os-number\">2.1<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Blackbody Radiation<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709819734\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709819736\">\n<p>1<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709819738\">Which surface has a higher temperature \u2013 the surface of a yellow star or that of a red star?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709819752\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709819754\">\n<p><span class=\"os-number\">2<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709819756\">Describe what you would see when looking at a body whose temperature is increased from 1000 K to 1,000,000 K.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709819769\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709819771\">\n<p>3<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709819773\">Explain the color changes in a hot body as its temperature is increased.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709819785\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709819787\">\n<p><span class=\"os-number\">4<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709819789\">Speculate as to why UV light causes sunburn, whereas visible light does not.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709819801\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709819803\">\n<p>5<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709819805\">Two cavity radiators are constructed with walls made of different metals. At the same temperature, how would their radiation spectra differ?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709819818\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709819820\">\n<p><span class=\"os-number\">6<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709819822\">Discuss why some bodies appear black, other bodies appear red, and still other bodies appear white.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709827902\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709827904\">\n<p>7<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709827907\">If everything radiates electromagnetic energy, why can we not see objects at room temperature in a dark room?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709827919\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709827922\">\n<p><span class=\"os-number\">8<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709827924\">How much does the power radiated by a blackbody increase when its temperature (in K) is tripled?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163713203408\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"72890_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-2-photoelectric-effect\/\"><span class=\"os-number\">2.2<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Photoelectric Effect<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713204295\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713478150\">\n<p>9<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713156825\">For the same monochromatic light source, would the photoelectric effect occur for all metals?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713254799\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713099944\">\n<p><span class=\"os-number\">10<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713187040\">In the interpretation of the photoelectric effect, how is it known that an electron does not absorb more than one photon?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713197187\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713514955\">\n<p>11<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713012857\">Explain how you can determine the work function from a plot of the stopping potential versus the frequency of the incident radiation in a photoelectric effect experiment. Can you determine the value of Planck\u2019s constant from this plot?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713106682\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713124682\">\n<p><span class=\"os-number\">12<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713434458\">Suppose that in the photoelectric-effect experiment we make a plot of the detected current versus the applied potential difference. What information do we obtain from such a plot? Can we determine from it the value of Planck\u2019s constant? Can we determine the work function of the metal?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713249547\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713433113\">\n<p>13<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709647064\">Speculate how increasing the temperature of a photoelectrode affects the outcomes of the photoelectric effect experiment.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709649099\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713263854\">\n<p><span class=\"os-number\">14<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713060000\">Which aspects of the photoelectric effect cannot be explained by classical physics?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709829775\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713244084\">\n<p>15<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713195147\">Is the photoelectric effect a consequence of the wave character of radiation or is it a consequence of the particle character of radiation? Explain briefly.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713052738\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713128031\">\n<p><span class=\"os-number\">16<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713537655\">The metals sodium, iron, and molybdenum have work functions 2.5 eV, 3.9 eV, and 4.2 eV, respectively. Which of these metals will emit photoelectrons when illuminated with 400 nm light?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163709821272\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"31351_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-3-the-compton-effect\/\"><span class=\"os-number\">2.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">The Compton Effect<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713293360\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709749405\">\n<p>17<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709749407\">Discuss any similarities and differences between the photoelectric and the Compton effects.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709829580\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709827936\">\n<p><span class=\"os-number\">18<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709827938\">Which has a greater momentum: an UV photon or an IR photon?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713271214\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713271216\">\n<p>19<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713294182\">Does changing the intensity of a monochromatic light beam affect the momentum of the individual photons in the beam? Does such a change affect the net momentum of the beam?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713483610\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709653940\">\n<p><span class=\"os-number\">20<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709653942\">Can the Compton effect occur with visible light? If so, will it be detectable?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713431110\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713431112\">\n<p>21<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709831568\">Is it possible in the Compton experiment to observe scattered X-rays that have a shorter wavelength than the incident X-ray radiation?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713146463\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713146466\">\n<p><span class=\"os-number\">22<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709678961\">Show that the Compton wavelength has the dimension of length.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713490619\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713490621\">\n<p>23<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709827809\">At what scattering angle is the wavelength shift in the Compton effect equal to the Compton wavelength?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163711964260\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"67977_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-4-bohrs-model-of-the-hydrogen-atom\/\"><span class=\"os-number\">2.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Bohr\u2019s Model of the Hydrogen Atom<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713537489\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713537491\">\n<p><span class=\"os-number\">24<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709758434\">Explain why the patterns of bright emission spectral lines have an identical spectral position to the pattern of dark absorption spectral lines for a given gaseous element.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713268590\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713412975\">\n<p>25<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713412977\">Do the various spectral lines of the hydrogen atom overlap?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713258490\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713258493\">\n<p><span class=\"os-number\">26<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713258495\">The Balmer series for hydrogen was discovered before either the Lyman or the Paschen series. Why?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713050499\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713050501\">\n<p>27<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713050503\">When the absorption spectrum of hydrogen at room temperature is analyzed, absorption lines for the Lyman series are found, but none are found for the Balmer series. What does this tell us about the energy state of most hydrogen atoms at room temperature?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713253754\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713535568\">\n<p><span class=\"os-number\">28<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713535570\">Hydrogen accounts for about 75% by mass of the matter at the surfaces of most stars. However, the absorption lines of hydrogen are strongest (of highest intensity) in the spectra of stars with a surface temperature of about 9000 K. They are weaker in the sun spectrum and are essentially nonexistent in very hot (temperatures above 25,000 K) or rather cool (temperatures below 3500 K) stars. Speculate as to why surface temperature affects the hydrogen absorption lines that we observe.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713485376\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713485378\">\n<p>29<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713485380\">Discuss the similarities and differences between Thomson\u2019s model of the hydrogen atom and Bohr\u2019s model of the hydrogen atom.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713243485\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713243487\">\n<p><span class=\"os-number\">30<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713243489\">Discuss the way in which Thomson\u2019s model is nonphysical. Support your argument with experimental evidence.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713163950\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713163953\">\n<p>31<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713289669\">If, in a hydrogen atom, an electron moves to an orbit with a larger radius, does the energy of the hydrogen atom increase or decrease?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713289682\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713010187\">\n<p><span class=\"os-number\">32<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713010189\">How is the energy conserved when an atom makes a transition from a higher to a lower energy state?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713010201\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709832973\">\n<p>33<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709832975\">Suppose an electron in a hydrogen atom makes a transition from the (<em data-effect=\"italics\">n+1<\/em>)th orbit to the<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th orbit. Is the wavelength of the emitted photon longer for larger values of<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>, or for smaller values of<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713556636\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713556638\">\n<p><span class=\"os-number\">34<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713556640\">Discuss why the allowed energies of the hydrogen atom are negative.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709648346\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709648348\">\n<p>35<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709648350\">Can a hydrogen atom absorb a photon whose energy is greater than 13.6 eV?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713204150\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713204152\">\n<p><span class=\"os-number\">36<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713204155\">Why can you see through glass but not through wood?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709681324\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709681326\">\n<p>37<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709681329\">Do gravitational forces have a significant effect on atomic energy levels?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709724857\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709724859\">\n<p><span class=\"os-number\">38<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709724861\">Show that Planck\u2019s constant has the dimensions of angular momentum.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163710834697\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"26515_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-5-de-broglies-matter-waves\/\"><span class=\"os-number\">2.5<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">De Broglie\u2019s Matter Waves<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712372433\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712372435\">\n<p>39<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712317174\">Which type of radiation is most suitable for the observation of diffraction patterns on crystalline solids; radio waves, visible light, or X-rays? Explain.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163710839854\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163710839856\">\n<p><span class=\"os-number\">40<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712266047\">Speculate as to how the diffraction patterns of a typical crystal would be affected if<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-167-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3-rays<\/span><\/span><\/span><span>\u00a0<\/span>were used instead of X-rays.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712315666\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712315668\">\n<p>41<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712176981\">If an electron and a proton are traveling at the same speed, which one has the shorter de Broglie wavelength?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712378474\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712378476\">\n<p><span class=\"os-number\">42<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712378478\">If a particle is accelerating, how does this affect its de Broglie wavelength?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712275347\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712315094\">\n<p>43<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712315096\">Why is the wave-like nature of matter not observed every day for macroscopic objects?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163710834867\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163710834870\">\n<p><span class=\"os-number\">44<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710834872\">What is the wavelength of a neutron at rest? Explain.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710957721\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712249030\">\n<p>45<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712249032\">Why does the setup of Davisson\u2013Germer experiment need to be enclosed in a vacuum chamber? Discuss what result you expect when the chamber is not evacuated.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163712354339\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"35633_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-6-wave-particle-duality\/\"><span class=\"os-number\">2.6<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Wave-Particle Duality<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712349462\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712349465\">\n<p><span class=\"os-number\">46<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712349467\">Give an example of an experiment in which light behaves as waves. Give an example of an experiment in which light behaves as a stream of photons.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712315786\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712315788\">\n<p>47<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712353651\">Discuss: How does the interference of water waves differ from the interference of electrons? How are they analogous?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163710848660\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711933421\">\n<p><span class=\"os-number\">48<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711933423\">Give at least one argument in support of the matter-wave hypothesis.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712153601\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163710999019\">\n<p>49<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710999021\">Give at least one argument in support of the particle-nature of radiation.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711953520\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711937978\">\n<p><span class=\"os-number\">50<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711937981\">Explain the importance of the Young double-slit experiment.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712144470\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712272274\">\n<p>51<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712272276\">Does the Heisenberg uncertainty principle allow a particle to be at rest in a designated region in space?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711969685\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712382995\">\n<p><span class=\"os-number\">52<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712382997\">Can the de Broglie wavelength of a particle be known exactly?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710834186\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163710848906\">\n<p>53<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710848908\">Do the photons of red light produce better resolution in a microscope than blue light photons? Explain.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711042258\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712317349\">\n<p><span class=\"os-number\">54<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712317352\">Discuss the main difference between an SEM and a TEM.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"os-review-problems-container\">\n<h3 data-type=\"title\"><span class=\"os-text\">Problems<\/span><\/h3>\n<div class=\"os-review-problems\">\n<div class=\"os-section-area\">\n<section id=\"fs-id11637098279360\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"88119_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-1-blackbody-radiation\/\"><span class=\"os-number\">2.1<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Blackbody Radiation<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709827943\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709827945\">\n<p>55<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709827947\">A 200-W heater emits a 1.5-\u00b5m radiation. (a) What value of the energy quantum does it emit? (b) Assuming that the specific heat of a 4.0-kg body is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-168-Frame\"><span class=\"MathJax_MathContainer\"><span>0.83kcal\/kg\u00b7K,<\/span><\/span><\/span><span>\u00a0<\/span>how many of these photons must be absorbed by the body to increase its temperature by 2 K? (c) How long does the heating process in (b) take, assuming that all radiation emitted by the heater gets absorbed by the body?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709830086\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709830088\">\n<p><span class=\"os-number\">56<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709830090\">A 900-W microwave generator in an oven generates energy quanta of frequency 2560 MHz. (a) How many energy quanta does it emit per second? (b) How many energy quanta must be absorbed by a pasta dish placed in the radiation cavity to increase its temperature by 45.0 K? Assume that the dish has a mass of 0.5 kg and that its specific heat is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-169-Frame\"><span class=\"MathJax_MathContainer\"><span>0.9kcal\/kg\u00b7K.<\/span><\/span><\/span><span>\u00a0<\/span>(c) Assume that all energy quanta emitted by the generator are absorbed by the pasta dish. How long must we wait until the dish in (b) is ready?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709830155\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709830157\">\n<p>57<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709830160\">(a) For what temperature is the peak of blackbody radiation spectrum at 400 nm? (b) If the temperature of a blackbody is 800 K, at what wavelength does it radiate the most energy?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709830177\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709830179\">\n<p><span class=\"os-number\">58<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709830181\">The tungsten elements of incandescent light bulbs operate at 3200 K. At what frequency does the filament radiate maximum energy?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713537702\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713537704\">\n<p>59<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713537706\">Interstellar space is filled with radiation of wavelength<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-170-Frame\"><span class=\"MathJax_MathContainer\"><span>970\u03bcm.<\/span><\/span><\/span><span>\u00a0<\/span>This radiation is considered to be a remnant of the \u201cbig bang.\u201d What is the corresponding blackbody temperature of this radiation?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713537725\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713537727\">\n<p><span class=\"os-number\">60<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713537729\">The radiant energy from the sun reaches its maximum at a wavelength of about 500.0 nm. What is the approximate temperature of the sun\u2019s surface?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163713276435\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"72890_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-2-photoelectric-effect\/\"><span class=\"os-number\">2.2<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Photoelectric Effect<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713427953\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713099928\">\n<p>61<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713286730\">A photon has energy 20 keV. What are its frequency and wavelength?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713203684\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713160552\">\n<p><span class=\"os-number\">62<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713418745\">The wavelengths of visible light range from approximately 400 to 750 nm. What is the corresponding range of photon energies for visible light?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713089403\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713515015\">\n<p>63<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713195273\">What is the longest wavelength of radiation that can eject a photoelectron from silver? Is it in the visible range?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713102973\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713006714\">\n<p><span class=\"os-number\">64<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713161402\">What is the longest wavelength of radiation that can eject a photoelectron from potassium, given the work function of potassium 2.24 eV? Is it in the visible range?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713044256\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713253944\">\n<p>65<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713135648\">Estimate the binding energy of electrons in magnesium, given that the wavelength of 337 nm is the longest wavelength that a photon may have to eject a photoelectron from magnesium photoelectrode.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713287703\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713181348\">\n<p><span class=\"os-number\">66<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713260358\">The work function for potassium is 2.26 eV. What is the cutoff frequency when this metal is used as photoelectrode? What is the stopping potential when for the emitted electrons when this photoelectrode is exposed to radiation of frequency 1200 THz?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713181808\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713136812\">\n<p>67<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709757529\">Estimate the work function of aluminum, given that the wavelength of 304 nm is the longest wavelength that a photon may have to eject a photoelectron from aluminum photoelectrode.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709666665\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709655949\">\n<p><span class=\"os-number\">68<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713009596\">What is the maximum kinetic energy of photoelectrons ejected from sodium by the incident radiation of wavelength 450 nm?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709681103\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713277885\">\n<p>69<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713275799\">A 120-nm UV radiation illuminates a gold-plated electrode. What is the maximum kinetic energy of the ejected photoelectrons?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713123904\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713084917\">\n<p><span class=\"os-number\">70<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713181082\">A 400-nm violet light ejects photoelectrons with a maximum kinetic energy of 0.860 eV from sodium photoelectrode. What is the work function of sodium?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713125354\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713163493\">\n<p>71<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713254262\">A 600-nm light falls on a photoelectric surface and electrons with the maximum kinetic energy of 0.17 eV are emitted. Determine (a) the work function and (b) the cutoff frequency of the surface. (c) What is the stopping potential when the surface is illuminated with light of wavelength 400 nm?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713275669\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713033157\">\n<p><span class=\"os-number\">72<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713009823\">The cutoff wavelength for the emission of photoelectrons from a particular surface is 500 nm. Find the maximum kinetic energy of the ejected photoelectrons when the surface is illuminated with light of wavelength 600 nm.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709668794\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713120255\">\n<p>73<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713099793\">Find the wavelength of radiation that can eject 2.00-eV electrons from calcium electrode. The work function for calcium is 2.71 eV. In what range is this radiation?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713259069\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713424949\">\n<p><span class=\"os-number\">74<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713033129\">Find the wavelength of radiation that can eject 0.10-eV electrons from potassium electrode. The work function for potassium is 2.24 eV. In what range is this radiation?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713297676\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713067016\">\n<p>75<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709733170\">Find the maximum velocity of photoelectrons ejected by an 80-nm radiation, if the work function of photoelectrode is 4.73 eV.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163713479845\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"31351_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-3-the-compton-effect\/\"><span class=\"os-number\">2.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">The Compton Effect<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709653867\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713427852\">\n<p><span class=\"os-number\">76<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713427854\">What is the momentum of a 589-nm yellow photon?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709700682\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713143241\">\n<p>77<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713143243\">What is the momentum of a 4-cm microwave photon?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713184542\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713269350\">\n<p><span class=\"os-number\">78<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713269352\">In a beam of white light (wavelengths from 400 to 750 nm), what range of momentum can the photons have?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713438566\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713438568\">\n<p>79<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713042337\">What is the energy of a photon whose momentum is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-171-Frame\"><span class=\"MathJax_MathContainer\"><span>3.0\u00d710\u221224kg\u00b7m\/s<\/span><\/span><\/span><span>\u00a0<\/span>?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713484828\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709676784\">\n<p><span class=\"os-number\">80<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709676786\">What is the wavelength of (a) a 12-keV X-ray photon; (b) a 2.0-MeV<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-172-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span>-ray photon?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709645515\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713053247\">\n<p>81<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713053249\">Find the momentum and energy of a 1.0-\u00c5 photon.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713262171\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713262174\">\n<p><span class=\"os-number\">82<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713041547\">Find the wavelength and energy of a photon with momentum<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-173-Frame\"><span class=\"MathJax_MathContainer\"><span>5.00\u00d710\u221229kg\u00b7m\/s.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713353953\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713487418\">\n<p>83<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713487420\">A<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-174-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span>-ray photon has a momentum of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-175-Frame\"><span class=\"MathJax_MathContainer\"><span>8.00\u00d710\u221221kg\u00b7m\/s.<\/span><\/span><\/span><span>\u00a0<\/span>Find its wavelength and energy.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709832998\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713269708\">\n<p><span class=\"os-number\">84<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713269710\">(a) Calculate the momentum of a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-176-Frame\"><span class=\"MathJax_MathContainer\"><span>2.5-\u00b5m<\/span><\/span><\/span><span>\u00a0<\/span>photon. (b) Find the velocity of an electron with the same momentum. (c) What is the kinetic energy of the electron, and how does it compare to that of the photon?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713196802\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713196804\">\n<p>85<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713196806\">Show that<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-177-Frame\"><span class=\"MathJax_MathContainer\"><span>p=h\/\u03bb<\/span><\/span><\/span><span>\u00a0<\/span>and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-178-Frame\"><span class=\"MathJax_MathContainer\"><span>Ef=hf<\/span><\/span><\/span><span>\u00a0<\/span>are consistent with the relativistic formula<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-179-Frame\"><span class=\"MathJax_MathContainer\"><span>E2=p2c2+m02c2.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713263574\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713263576\">\n<p><span class=\"os-number\">86<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713263578\">Show that the energy<span>\u00a0<\/span><em data-effect=\"italics\">E<\/em><span>\u00a0<\/span>in eV of a photon is given by<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-180-Frame\"><span class=\"MathJax_MathContainer\"><span>E=1.241\u00d710\u22126eV\u00b7m\/\u03bb,<\/span><\/span><\/span><span>\u00a0<\/span>where<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-181-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bb<\/span><\/span><\/span><span>\u00a0<\/span>is its wavelength in meters.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713128336\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713128338\">\n<p>87<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713128340\">For collisions with free electrons, compare the Compton shift of a photon scattered as an angle of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-182-Frame\"><span class=\"MathJax_MathContainer\"><span>30\u00b0<\/span><\/span><\/span><span>\u00a0<\/span>to that of a photon scattered at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-183-Frame\"><span class=\"MathJax_MathContainer\"><span>45\u00b0.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713458514\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713458516\">\n<p><span class=\"os-number\">88<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709831535\">X-rays of wavelength 12.5 pm are scattered from a block of carbon. What are the wavelengths of photons scattered at (a)<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-184-Frame\"><span class=\"MathJax_MathContainer\"><span>30\u00b0;<\/span><\/span><\/span><span>\u00a0<\/span>(b)<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-185-Frame\"><span class=\"MathJax_MathContainer\"><span>90\u00b0;<\/span><\/span><\/span><span>\u00a0<\/span>and, (c)<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-186-Frame\"><span class=\"MathJax_MathContainer\"><span>180\u00b0<\/span><\/span><\/span><span>\u00a0<\/span>?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163709724868\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"67977_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-4-bohrs-model-of-the-hydrogen-atom\/\"><span class=\"os-number\">2.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Bohr\u2019s Model of the Hydrogen Atom<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713163833\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713163835\">\n<p>89<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713163837\">Calculate the wavelength of the first line in the Lyman series and show that this line lies in the ultraviolet part of the spectrum.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709831664\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709831666\">\n<p><span class=\"os-number\">90<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709831668\">Calculate the wavelength of the fifth line in the Lyman series and show that this line lies in the ultraviolet part of the spectrum.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709827766\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709827768\">\n<p>91<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709827770\">Calculate the energy changes corresponding to the transitions of the hydrogen atom: (a) from<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-187-Frame\"><span class=\"MathJax_MathContainer\"><span>n=3<\/span><\/span><\/span><span>\u00a0<\/span>to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-188-Frame\"><span class=\"MathJax_MathContainer\"><span>n=4;<\/span><\/span><\/span><span>\u00a0<\/span>(b) from<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-189-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2<\/span><\/span><\/span><span>\u00a0<\/span>to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-190-Frame\"><span class=\"MathJax_MathContainer\"><span>n=1;<\/span><\/span><\/span><span>\u00a0<\/span>and (c) from<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-191-Frame\"><span class=\"MathJax_MathContainer\"><span>n=3<\/span><\/span><\/span><span>\u00a0<\/span>to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-192-Frame\"><span class=\"MathJax_MathContainer\"><span>n=\u221e.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713450603\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713450605\">\n<p><span class=\"os-number\">92<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713450607\">Determine the wavelength of the third Balmer line (transition from<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-193-Frame\"><span class=\"MathJax_MathContainer\"><span>n=5<\/span><\/span><\/span><span>\u00a0<\/span>to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-194-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2<\/span><\/span><\/span>).<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713429628\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713429630\">\n<p>93<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713429632\">What is the frequency of the photon absorbed when the hydrogen atom makes the transition from the ground state to the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-195-Frame\"><span class=\"MathJax_MathContainer\"><span>n=4<\/span><\/span><\/span><span>\u00a0<\/span>state?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163709829701\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709829703\">\n<p><span class=\"os-number\">94<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709829705\">When a hydrogen atom is in its ground state, what are the shortest and longest wavelengths of the photons it can absorb without being ionized?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713432792\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713432794\">\n<p>95<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713432796\">When a hydrogen atom is in its third excided state, what are the shortest and longest wavelengths of the photons it can emit?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713284382\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713284384\">\n<p><span class=\"os-number\">96<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713284386\">What is the longest wavelength that light can have if it is to be capable of ionizing the hydrogen atom in its ground state?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713050379\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713050381\">\n<p>97<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713050383\">For an electron in a hydrogen atom in the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-196-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2<\/span><\/span><\/span><span>\u00a0<\/span>state, compute: (a) the angular momentum; (b) the kinetic energy; (c) the potential energy; and (d) the total energy.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713246684\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713246686\">\n<p><span class=\"os-number\">98<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713246688\">Find the ionization energy of a hydrogen atom in the fourth energy state.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713557498\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713557500\">\n<p>99<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713557502\">It has been measured that it required 0.850 eV to remove an electron from the hydrogen atom. In what state was the atom before the ionization happened?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713276597\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713276599\">\n<p><span class=\"os-number\">100<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713276601\">What is the radius of a hydrogen atom when the electron is in the first excited state?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713249475\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713249477\">\n<p>101<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713249479\">Find the shortest wavelength in the Balmer series. In what part of the spectrum does this line lie?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713249491\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713517356\">\n<p><span class=\"os-number\">102<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713517358\">Show that the entire Paschen series lies in the infrared part of the spectrum.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163713517363\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713517366\">\n<p>103<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713517368\">Do the Balmer series and the Lyman series overlap? Why? Why not? (Hint: calculate the shortest Balmer line and the longest Lyman line.)<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163713535613\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163713535615\">\n<p><span class=\"os-number\">104<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163713535617\">(a) Which line in the Balmer series is the first one in the UV part of the spectrum? (b) How many Balmer lines lie in the visible part of the spectrum? (c) How many Balmer lines lie in the UV?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163709817720\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163709817722\">\n<p>105<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163709817724\">A<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-197-Frame\"><span class=\"MathJax_MathContainer\"><span>4.653-\u03bcm<\/span><\/span><\/span><span>\u00a0<\/span>emission line of atomic hydrogen corresponds to transition between the states<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-198-Frame\"><span class=\"MathJax_MathContainer\"><span>nf=5<\/span><\/span><\/span><span>\u00a0<\/span>and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-199-Frame\"><span class=\"MathJax_MathContainer\"><span>ni.<\/span><\/span><\/span><span>\u00a0<\/span>Find<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-200-Frame\"><span class=\"MathJax_MathContainer\"><span>ni.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163712190070\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"26515_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-5-de-broglies-matter-waves\/\"><span class=\"os-number\">2.5<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">De Broglie\u2019s Matter Waves<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712279890\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712084068\">\n<p><span class=\"os-number\">106<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712084071\">At what velocity will an electron have a wavelength of 1.00 m?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712315240\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712315242\">\n<p>107<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712315244\">What is the de Broglie wavelength of an electron travelling at a speed of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-201-Frame\"><span class=\"MathJax_MathContainer\"><span>5.0\u00d7106m\/s<\/span><\/span><\/span><span>\u00a0<\/span>?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712098145\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712098147\">\n<p><span class=\"os-number\">108<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712098149\">What is the de Broglie wavelength of an electron that is accelerated from rest through a potential difference of 20 keV?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712314741\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711933634\">\n<p>109<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711933636\">What is the de Broglie wavelength of a proton whose kinetic energy is 2.0 MeV? 10.0 MeV?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712413228\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712413230\">\n<p><span class=\"os-number\">110<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712090894\">What is the de Broglie wavelength of a 10-kg football player running at a speed of 8.0 m\/s?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712183285\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712183287\">\n<p>111<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712183289\">(a) What is the energy of an electron whose de Broglie wavelength is that of a photon of yellow light with wavelength 590 nm? (b) What is the de Broglie wavelength of an electron whose energy is that of the photon of yellow light?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712079249\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712079251\">\n<p><span class=\"os-number\">112<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712079253\">The de Broglie wavelength of a neutron is 0.01 nm. What is the speed and energy of this neutron?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710974558\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163710974560\">\n<p>113<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710974562\">What is the wavelength of an electron that is moving at a 3% of the speed of light?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712257074\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712257076\">\n<p><span class=\"os-number\">114<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712274557\">At what velocity does a proton have a 6.0-fm wavelength (about the size of a nucleus)? Give your answer in units of<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712094058\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712094060\">\n<p>115<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710846624\">What is the velocity of a 0.400-kg billiard ball if its wavelength is 7.50 fm?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712374839\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712374841\">\n<p><span class=\"os-number\">116<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712374844\">Find the wavelength of a proton that is moving at 1.00% of the speed of light (when<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-202-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b2=0.01).<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1163710981804\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"35633_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/2-6-wave-particle-duality\/\"><span class=\"os-number\">2.6<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Wave-Particle Duality<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712311334\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712311336\">\n<p>117<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712311338\">An AM radio transmitter radiates 500 kW at a frequency of 760 kHz. How many photons per second does the emitter emit?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711888093\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711939071\">\n<p><span class=\"os-number\">118<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711939073\">Find the Lorentz factor<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-203-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>and de Broglie\u2019s wavelength for a 50-GeV electron in a particle accelerator.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712316372\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712316374\">\n<p>119<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712316376\">Find the Lorentz factor<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-204-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>and de Broglie\u2019s wavelength for a 1.0-TeV proton in a particle accelerator.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712284485\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712284487\">\n<p><span class=\"os-number\">120<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712284489\">What is the kinetic energy of a 0.01-nm electron in a TEM?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712090899\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163710770573\">\n<p>121<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710770576\">If electron is to be diffracted significantly by a crystal, its wavelength must be about equal to the spacing,<span>\u00a0<\/span><em data-effect=\"italics\">d<\/em>, of crystalline planes. Assuming<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-205-Frame\"><span class=\"MathJax_MathContainer\"><span>d=0.250nm,<\/span><\/span><\/span><span>\u00a0<\/span>estimate the potential difference through which an electron must be accelerated from rest if it is to be diffracted by these planes.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163710892218\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163710892220\">\n<p><span class=\"os-number\">122<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712440493\">X-rays form ionizing radiation that is dangerous to living tissue and undetectable to the human eye. Suppose that a student researcher working in an X-ray diffraction laboratory is accidentally exposed to a fatal dose of radiation. Calculate the temperature increase of the researcher under the following conditions: the energy of X-ray photons is 200 keV and the researcher absorbs<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-206-Frame\"><span class=\"MathJax_MathContainer\"><span>4\u00d71013<\/span><\/span><\/span><span>\u00a0<\/span>photons per each kilogram of body weight during the exposure. Assume that the specific heat of the student\u2019s body is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-207-Frame\"><span class=\"MathJax_MathContainer\"><span>0.83kcal\/kg\u00b7K.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710955242\">\n<section>\n<div data-type=\"problem\" id=\"fs-id11637123150940\">\n<p>123<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id11637123150960\">Solar wind (radiation) that is incident on the top of Earth\u2019s atmosphere has an average intensity of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-208-Frame\"><span class=\"MathJax_MathContainer\"><span>1.3kW\/m2.<\/span><\/span><\/span><span>\u00a0<\/span>Suppose that you are building a solar sail that is to propel a small toy spaceship with a mass of 0.1 kg in the space between the International Space Station and the moon. The sail is made from a very light material, which perfectly reflects the incident radiation. To assess whether such a project is feasible, answer the following questions, assuming that radiation photons are incident only in normal direction to the sail reflecting surface. (a) What is the radiation pressure (force per<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-209-Frame\"><span class=\"MathJax_MathContainer\"><span>m2<\/span><\/span><\/span>) of the radiation falling on the mirror-like sail? (b) Given the radiation pressure computed in (a), what will be the acceleration of the spaceship when the sail has of an area of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-210-Frame\"><span class=\"MathJax_MathContainer\"><span>10.0m2<\/span><\/span><\/span><span>\u00a0<\/span>? (c) Given the acceleration estimate in (b), how fast will the spaceship be moving after 24 hours when it starts from rest?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711048465\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711048467\">\n<p><span class=\"os-number\">124<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711048469\">Treat the human body as a blackbody and determine the percentage increase in the total power of its radiation when its temperature increases from 98.6<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-211-Frame\"><span class=\"MathJax_MathContainer\"><span>\u00b0<\/span><\/span><\/span><span>\u00a0<\/span>F to 103<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-212-Frame\"><span class=\"MathJax_MathContainer\"><span>\u00b0<\/span><\/span><\/span><span>\u00a0<\/span>F.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711020632\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711020634\">\n<p>125<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711020636\">Show that Wien\u2019s displacement law results from Planck\u2019s radiation law. (<em data-effect=\"italics\">Hint:<\/em><span>\u00a0<\/span>substitute<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-213-Frame\"><span class=\"MathJax_MathContainer\"><span>x=hc\/\u03bbkT<\/span><\/span><\/span><span>\u00a0<\/span>and write Planck\u2019s law in the form<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-214-Frame\"><span class=\"MathJax_MathContainer\"><span>I(x,T)=Ax5\/(ex\u22121),<\/span><\/span><\/span><span>\u00a0<\/span>where<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-215-Frame\"><span class=\"MathJax_MathContainer\"><span>A=2\u03c0(kT)5\/(h4c3).<\/span><\/span><\/span><span>\u00a0<\/span>Now, for fixed<span>\u00a0<\/span><em data-effect=\"italics\">T<\/em>, find the position of the maximum in<span>\u00a0<\/span><em data-effect=\"italics\">I<\/em>(<em data-effect=\"italics\">x<\/em>,<em data-effect=\"italics\">T<\/em>) by solving for<span>\u00a0<\/span><em data-effect=\"italics\">x<\/em>in the equation<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-216-Frame\"><span class=\"MathJax_MathContainer\"><span>dI(x,T)\/dx=0.<\/span><\/span><\/span>)<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711965492\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711965494\">\n<p><span class=\"os-number\">126<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712331421\">Show that Stefan\u2019s law results from Planck\u2019s radiation law.<span>\u00a0<\/span><em data-effect=\"italics\">Hint:<\/em><span>\u00a0<\/span>To compute the total power of blackbody radiation emitted across the entire spectrum of wavelengths at a given temperature, integrate Planck\u2019s law over the entire spectrum<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-217-Frame\"><span class=\"MathJax_MathContainer\"><span>P(T)=\u222b0\u221eI(\u03bb,T)d\u03bb.<\/span><\/span><\/span><span>\u00a0<\/span>Use the substitution<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-218-Frame\"><span class=\"MathJax_MathContainer\"><span>x=hc\/\u03bbkT<\/span><\/span><\/span><span>\u00a0<\/span>and the tabulated value of the integral<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-219-Frame\"><span class=\"MathJax_MathContainer\"><span>\u222b0\u221edxx3\/(ex\u22121)=\u03c04\/15.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"os-review-additional-problems-container\">\n<h3 data-type=\"title\"><span class=\"os-text\">Additional Problems<\/span><\/h3>\n<section id=\"fs-id1172101896308\" class=\"review-additional-problems\" data-depth=\"1\">\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712316432\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712316434\">\n<p>127<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712224356\">Determine the power intensity of radiation per unit wavelength emitted at a wavelength of 500.0 nm by a blackbody at a temperature of 10,000 K.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163710983419\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163710983421\">\n<p><span class=\"os-number\">128<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710983423\">The HCl molecule oscillates at a frequency of 87.0 THz. What is the difference (in eV) between its adjacent energy levels?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711969237\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712320737\">\n<p>129<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712320739\">A quantum mechanical oscillator vibrates at a frequency of 250.0 THz. What is the minimum energy of radiation it can emit?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711888302\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711888304\">\n<p><span class=\"os-number\">130<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712279583\">In about 5 billion years, the sun will evolve to a red giant. Assume that its surface temperature will decrease to about half its present value of 6000 K, while its present radius of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-220-Frame\"><span class=\"MathJax_MathContainer\"><span>7.0\u00d7108m<\/span><\/span><\/span><span>\u00a0<\/span>will increase to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-221-Frame\"><span class=\"MathJax_MathContainer\"><span>1.5\u00d71011m<\/span><\/span><\/span><span>\u00a0<\/span>(which is the current Earth-sun distance). Calculate the ratio of the total power emitted by the sun in its red giant stage to its present power.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712174458\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163710886364\">\n<p>131<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710886366\">A sodium lamp emits 2.0 W of radiant energy, most of which has a wavelength of about 589 nm. Estimate the number of photons emitted per second by the lamp.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712182419\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711939088\">\n<p><span class=\"os-number\">132<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711939090\">Photoelectrons are ejected from a photoelectrode and are detected at a distance of 2.50 cm away from the photoelectrode. The work function of the photoelectrode is 2.71 eV and the incident radiation has a wavelength of 420 nm. How long does it take a photoelectron to travel to the detector?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710813976\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712430770\">\n<p>133<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712430772\">If the work function of a metal is 3.2 eV, what is the maximum wavelength that a photon can have to eject a photoelectron from this metal surface?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712228772\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712228774\">\n<p><span class=\"os-number\">134<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712283826\">The work function of a photoelectric surface is 2.00 eV. What is the maximum speed of the photoelectrons emitted from this surface when a 450-nm light falls on it?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711941332\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711941334\">\n<p>135<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710974559\">A 400-nm laser beam is projected onto a calcium electrode. The power of the laser beam is 2.00 mW and the work function of calcium is 2.31 eV. (a) How many photoelectrons per second are ejected? (b) What net power is carried away by photoelectrons?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712291539\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712291542\">\n<p><span class=\"os-number\">136<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712291544\">(a) Calculate the number of photoelectrons per second that are ejected from a 1.00-mm<sup>2<\/sup><span>\u00a0<\/span>area of sodium metal by a 500-nm radiation with intensity<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-222-Frame\"><span class=\"MathJax_MathContainer\"><span>1.30kW\/m2<\/span><\/span><\/span><span>\u00a0<\/span>(the intensity of sunlight above Earth\u2019s atmosphere). (b) Given the work function of the metal as 2.28 eV, what power is carried away by these photoelectrons?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712161001\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711990340\">\n<p>137<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711990342\">A laser with a power output of 2.00 mW at a 400-nm wavelength is used to project a beam of light onto a calcium photoelectrode. (a) How many photoelectrons leave the calcium surface per second? (b) What power is carried away by ejected photoelectrons, given that the work function of calcium is 2.31 eV? (c) Calculate the photocurrent. (d) If the photoelectrode suddenly becomes electrically insulated and the setup of two electrodes in the circuit suddenly starts to act like a 2.00-pF capacitor, how long will current flow before the capacitor voltage stops it?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711987098\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711987100\">\n<p><span class=\"os-number\">138<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711976750\">The work function for barium is 2.48 eV. Find the maximum kinetic energy of the ejected photoelectrons when the barium surface is illuminated with: (a) radiation emitted by a 100-kW radio station broadcasting at 800 kHz; (b) a 633-nm laser light emitted from a powerful He-Ne laser; and (c) a 434-nm blue light emitted by a small hydrogen gas discharge tube.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712175615\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712175617\">\n<p>139<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712282142\">(a) Calculate the wavelength of a photon that has the same momentum as a proton moving with 1% of the speed of light in a vacuum. (b) What is the energy of this photon in MeV? (c) What is the kinetic energy of the proton in MeV?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712131536\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712131538\">\n<p><span class=\"os-number\">140<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712131540\">(a) Find the momentum of a 100-keV X-ray photon. (b) Find the velocity of a neutron with the same momentum. (c) What is the neutron\u2019s kinetic energy in eV?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711983460\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712299629\">\n<p>141<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712299631\">The momentum of light, as it is for particles, is exactly reversed when a photon is reflected straight back from a mirror, assuming negligible recoil of the mirror. The change in momentum is twice the photon\u2019s incident momentum, as it is for the particles. Suppose that a beam of light has an intensity<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-223-Frame\"><span class=\"MathJax_MathContainer\"><span>1.0kW\/m2<\/span><\/span><\/span><span>\u00a0<\/span>and falls on a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-224-Frame\"><span class=\"MathJax_MathContainer\"><span>\u22122.0-m2<\/span><\/span><\/span><span>\u00a0<\/span>area of a mirror and reflects from it. (a) Calculate the energy reflected in 1.00 s. (b) What is the momentum imparted to the mirror? (c) Use Newton\u2019s second law to find the force on the mirror. (d) Does the assumption of no-recoil for the mirror seem reasonable?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711918192\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712382607\">\n<p><span class=\"os-number\">142<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712382609\">A photon of energy 5.0 keV collides with a stationary electron and is scattered at an angle of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-225-Frame\"><span class=\"MathJax_MathContainer\"><span>60\u00b0.<\/span><\/span><\/span><span>\u00a0<\/span>What is the energy acquired by the electron in the collision?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712189962\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712189965\">\n<p>143<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710887829\">A 0.75-nm photon is scattered by a stationary electron. The speed of the electron\u2019s recoil is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-226-Frame\"><span class=\"MathJax_MathContainer\"><span>1.5\u00d7106m\/s.<\/span><\/span><\/span><span>\u00a0<\/span>(a) Find the wavelength shift of the photon. (b) Find the scattering angle of the photon.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712090793\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712090795\">\n<p><span class=\"os-number\">144<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712090797\">Find the maximum change in X-ray wavelength that can occur due to Compton scattering. Does this change depend on the wavelength of the incident beam?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712404968\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712404970\">\n<p>145<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711964258\">A photon of wavelength 700 nm is incident on a hydrogen atom. When this photon is absorbed, the atom becomes ionized. What is the lowest possible orbit that the electron could have occupied before being ionized?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712438121\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712438123\">\n<p><span class=\"os-number\">146<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712438125\">What is the maximum kinetic energy of an electron such that a collision between the electron and a stationary hydrogen atom in its ground state is definitely elastic?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163710886894\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163710886896\">\n<p>147<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163710886899\">Singly ionized atomic helium<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-227-Frame\"><span class=\"MathJax_MathContainer\"><span>He+1<\/span><\/span><\/span><span>\u00a0<\/span>is a hydrogen-like ion. (a) What is its ground-state radius? (b) Calculate the energies of its four lowest energy states. (c) Repeat the calculations for the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-228-Frame\"><span class=\"MathJax_MathContainer\"><span>Li2+<\/span><\/span><\/span><span>\u00a0<\/span>ion.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711954120\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711954122\">\n<p><span class=\"os-number\">148<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711954124\">A triply ionized atom of beryllium<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-229-Frame\"><span class=\"MathJax_MathContainer\"><span>Be3+<\/span><\/span><\/span><span>\u00a0<\/span>is a hydrogen-like ion. When<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-230-Frame\"><span class=\"MathJax_MathContainer\"><span>Be3+<\/span><\/span><\/span><span>\u00a0<\/span>is in one of its excited states, its radius in this<em data-effect=\"italics\">n<\/em>th state is exactly the same as the radius of the first Bohr orbit of hydrogen. Find<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em><span>\u00a0<\/span>and compute the ionization energy for this state of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-231-Frame\"><span class=\"MathJax_MathContainer\"><span>Be3+.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712039267\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712081947\">\n<p>149<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712081949\">In extreme-temperature environments, such as those existing in a solar corona, atoms may be ionized by undergoing collisions with other atoms. One example of such ionization in the solar corona is the presence of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-232-Frame\"><span class=\"MathJax_MathContainer\"><span>C5+<\/span><\/span><\/span><span>\u00a0<\/span>ions, detected in the Fraunhofer spectrum. (a) By what factor do the energies of the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-233-Frame\"><span class=\"MathJax_MathContainer\"><span>C5+<\/span><\/span><\/span><span>\u00a0<\/span>ion scale compare to the energy spectrum of a hydrogen atom? (b) What is the wavelength of the first line in the Paschen series of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-234-Frame\"><span class=\"MathJax_MathContainer\"><span>C5+<\/span><\/span><\/span><span>\u00a0<\/span>? (c) In what part of the spectrum are these lines located?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712236542\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712236544\">\n<p><span class=\"os-number\">150<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id11637122365460\">(a) Calculate the ionization energy for<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-235-Frame\"><span class=\"MathJax_MathContainer\"><span>He+.<\/span><\/span><\/span><span>\u00a0<\/span>(b) What is the minimum frequency of a photon capable of ionizing<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-236-Frame\"><span class=\"MathJax_MathContainer\"><span>He+<\/span><\/span><\/span><span>\u00a0<\/span>?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711964124\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711964126\">\n<p>151<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711964128\">Experiments are performed with ultracold neutrons having velocities as small as 1.00 m\/s. Find the wavelength of such an ultracold neutron and its kinetic energy.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712274837\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712274839\">\n<p><span class=\"os-number\">152<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712274841\">Find the velocity and kinetic energy of a 6.0-fm neutron. (Rest mass energy of neutron is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-237-Frame\"><span class=\"MathJax_MathContainer\"><span>E0=940MeV.)<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712274363\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712274365\">\n<p>153<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712278869\">The spacing between crystalline planes in the NaCl crystal is 0.281 nm, as determined by X-ray diffraction with X-rays of wavelength 0.170 nm. What is the energy of neutrons in the neutron beam that produces diffraction peaks at the same locations as the peaks obtained with the X-rays?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163711937333\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711937335\">\n<p><span class=\"os-number\">154<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711964193\">What is the wavelength of an electron accelerated from rest in a 30.0-kV potential difference?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712316677\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712316680\">\n<p>155<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712279283\">Calculate the velocity of a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-238-Frame\"><span class=\"MathJax_MathContainer\"><span>1.0-\u03bcm<\/span><\/span><\/span><span>\u00a0<\/span>electron and a potential difference used to accelerate it from rest to this velocity.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712274221\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712274223\">\n<p><span class=\"os-number\">156<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712274225\">In a supercollider at CERN, protons are accelerated to velocities of 0.25<em data-effect=\"italics\">c<\/em>. What are their wavelengths at this speed? What are their kinetic energies? If a beam of protons were to gain its kinetic energy in only one pass through a potential difference, how high would this potential difference have to be? (Rest mass energy of a proton is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-239-Frame\"><span class=\"MathJax_MathContainer\"><span>E0=938MeV).<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712317995\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712317998\">\n<p>157<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712318000\">Find the de Broglie wavelength of an electron accelerated from rest in an X-ray tube in the potential difference of 100 keV. (Rest mass energy of an electron is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-240-Frame\"><span class=\"MathJax_MathContainer\"><span>E0=511keV.)<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712283645\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712283647\">\n<p><span class=\"os-number\">158<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712283650\">The cutoff wavelength for the emission of photoelectrons from a particular surface is 500 nm. Find the maximum kinetic energy of the ejected photoelectrons when the surface is illuminated with light of wavelength 450 nm.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712279098\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712279100\">\n<p>159<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712279102\">Compare the wavelength shift of a photon scattered by a free electron to that of a photon scattered at the same angle by a free proton.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712236888\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712236890\">\n<p><span class=\"os-number\">160<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712236892\">The spectrometer used to measure the wavelengths of the scattered X-rays in the Compton experiment is accurate to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-241-Frame\"><span class=\"MathJax_MathContainer\"><span>5.0\u00d710\u22124nm.<\/span><\/span><\/span><span>\u00a0<\/span>What is the minimum scattering angle for which the X-rays interacting with the free electrons can be distinguished from those interacting with the atoms?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163712240128\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712240130\">\n<p>161<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712240132\">Consider a hydrogen-like ion where an electron is orbiting a nucleus that has charge<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-242-Frame\"><span class=\"MathJax_MathContainer\"><span>q=+Ze.<\/span><\/span><\/span><span>\u00a0<\/span>Derive the formulas for the energy<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-243-Frame\"><span class=\"MathJax_MathContainer\"><span>En<\/span><\/span><\/span><span>\u00a0<\/span>of the electron in<span>\u00a0<\/span><em data-effect=\"italics\">n<\/em>th orbit and the orbital radius<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-244-Frame\"><span class=\"MathJax_MathContainer\"><span>rn.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1163712236459\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163712236461\">\n<p><span class=\"os-number\">162<\/span><span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163712236463\">Assume that a hydrogen atom exists in the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-245-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2<\/span><\/span><\/span><span>\u00a0<\/span>excited state for<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-246-Frame\"><span class=\"MathJax_MathContainer\"><span>10\u22128s<\/span><\/span><\/span><span>\u00a0<\/span>before decaying to the ground state. How many times does the electron orbit the proton nucleus during this time? How long does it take Earth to orbit the sun this many times?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1163711991347\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1163711991350\">\n<p>163<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1163711941154\">An atom can be formed when a negative muon is captured by a proton. The muon has the same charge as the electron and a mass 207 times that of the electron. Calculate the frequency of the photon emitted when this atom makes the transition from\u00a0<span class=\"MathJax_MathML\" id=\"MathJax-Element-247-Frame\"><span class=\"MathJax_MathContainer\"><span>n=2\u00a0<\/span><\/span><\/span>to the<span class=\"MathJax_MathML\" id=\"MathJax-Element-248-Frame\"><span class=\"MathJax_MathContainer\"><span>n=1\u00a0<\/span><\/span><\/span>state. Assume that the muon is orbiting a stationary proton.<\/p>\n<\/div>\n<p>&nbsp;<\/p>\n<div class=\"textbox\"><em>Download for free at http:\/\/cnx.org\/contents\/af275420-6050-4707-995c-57b9cc13c358@11.1<\/em><\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n","protected":false},"author":615,"menu_order":8,"template":"","meta":{"pb_show_title":"on","pb_short_title":"2. Photons and Matter Waves","pb_subtitle":"Chapter 2 Review","pb_authors":[],"pb_section_license":""},"chapter-type":[],"contributor":[],"license":[],"class_list":["post-174","chapter","type-chapter","status-publish","hentry"],"part":36,"_links":{"self":[{"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapters\/174","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/wp\/v2\/users\/615"}],"version-history":[{"count":5,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapters\/174\/revisions"}],"predecessor-version":[{"id":405,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapters\/174\/revisions\/405"}],"part":[{"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/parts\/36"}],"metadata":[{"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapters\/174\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/wp\/v2\/media?parent=174"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapter-type?post=174"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/wp\/v2\/contributor?post=174"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/wp\/v2\/license?post=174"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}