{"id":96,"date":"2019-04-01T17:45:32","date_gmt":"2019-04-01T21:45:32","guid":{"rendered":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/?post_type=chapter&#038;p=96"},"modified":"2019-04-12T18:44:57","modified_gmt":"2019-04-12T22:44:57","slug":"chapter-review","status":"publish","type":"chapter","link":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/chapter-review\/","title":{"raw":"Chapter 1 Review","rendered":"Chapter 1 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-id1167793938539\">\r\n \t<dt id=\"38518\">classical (Galilean) velocity addition<\/dt>\r\n \t<dd id=\"fs-id1167794142090\">method of adding velocities when<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1689-Frame\"><span class=\"MathJax_MathContainer\">v&lt;&lt;c;<\/span><\/span>\u00a0<\/span>velocities add like regular numbers in one-dimensional motion:<span> u=v+u\u2032,\u00a0<\/span>where<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is the velocity between two observers,<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>is the velocity of an object relative to one observer, and<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1691-Frame\"><span class=\"MathJax_MathContainer\">u\u2032<\/span><\/span>\u00a0<\/span>is the velocity relative to the other observer<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793561609\">\r\n \t<dt id=\"53287\">event<\/dt>\r\n \t<dd id=\"fs-id1167793561614\">occurrence in space and time specified by its position and time coordinates (<em data-effect=\"italics\">x<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">y<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">z<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">t<\/em>) measured relative to a frame of reference<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793984547\">\r\n \t<dt id=\"84790\">first postulate of special relativity<\/dt>\r\n \t<dd id=\"fs-id1167794139578\">laws of physics are the same in all inertial frames of reference<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793787576\">\r\n \t<dt id=\"62803\">Galilean relativity<\/dt>\r\n \t<dd id=\"fs-id1167793261076\">if an observer measures a velocity in one frame of reference, and that frame of reference is moving with a velocity past a second reference frame, an observer in the second frame measures the original velocity as the vector sum of these velocities<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793277651\">\r\n \t<dt id=\"96665\">Galilean transformation<\/dt>\r\n \t<dd id=\"fs-id1167793277656\">relation between position and time coordinates of the same events as seen in different reference frames, according to classical mechanics<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793363172\">\r\n \t<dt id=\"8441\">inertial frame of reference<\/dt>\r\n \t<dd id=\"fs-id1167794142311\">reference frame in which a body at rest remains at rest and a body in motion moves at a constant speed in a straight line unless acted on by an outside force<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167794058670\">\r\n \t<dt id=\"62399\">length contraction<\/dt>\r\n \t<dd id=\"fs-id1167793692944\">decrease in observed length of an object from its proper length<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1692-Frame\"><span class=\"MathJax_MathContainer\">L0<\/span><\/span>\u00a0<\/span>to length<span>\u00a0<\/span><em data-effect=\"italics\">L<\/em><span>\u00a0<\/span>when its length is observed in a reference frame where it is traveling at speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793277662\">\r\n \t<dt id=\"19632\">Lorentz transformation<\/dt>\r\n \t<dd id=\"fs-id1167793277667\">relation between position and time coordinates of the same events as seen in different reference frames, according to the special theory of relativity<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793514956\">\r\n \t<dt id=\"3267\">Michelson-Morley experiment<\/dt>\r\n \t<dd id=\"fs-id1167793556786\">investigation performed in 1887 that showed that the speed of light in a vacuum is the same in all frames of reference from which it is viewed<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793933707\">\r\n \t<dt id=\"65548\">proper length<\/dt>\r\n \t<dd id=\"fs-id1167793278452\">L0; the distance between two points measured by an observer who is at rest relative to both of the points; for example, earthbound observers measure proper length when measuring the distance between two points that are stationary relative to Earth<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793409768\">\r\n \t<dt id=\"10222\">proper time<\/dt>\r\n \t<dd id=\"fs-id1167793433561\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1694-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394\u03c4<\/span><\/span><\/span><span>\u00a0<\/span>is the time interval measured by an observer who sees the beginning and end of the process that the time interval measures occur at the same location<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167794215993\">\r\n \t<dt id=\"16\">relativistic kinetic energy<\/dt>\r\n \t<dd id=\"fs-id1167794215998\">kinetic energy of an object moving at relativistic speeds<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167794041889\">\r\n \t<dt id=\"35073\">relativistic momentum<\/dt>\r\n \t<dd id=\"fs-id1167793887875\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1695-Frame\"><span class=\"MathJax_MathContainer\"><span>p\u2192,<\/span><\/span><\/span><span>\u00a0<\/span>the momentum of an object moving at relativistic velocity;<span> p\u2192=\u03b3mu\u2192<\/span><\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793583897\">\r\n \t<dt id=\"6785\">relativistic velocity addition<\/dt>\r\n \t<dd id=\"fs-id1167794293139\">method of adding velocities of an object moving at a relativistic speeds<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167794216002\">\r\n \t<dt id=\"70859\">rest energy<\/dt>\r\n \t<dd id=\"fs-id1167794216008\">energy stored in an object at rest:<span> E0=mc2<\/span><\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167794137438\">\r\n \t<dt id=\"56141\">rest frame<\/dt>\r\n \t<dd id=\"fs-id1167793750803\">frame of reference in which the observer is at rest<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793881872\">\r\n \t<dt id=\"2055\">rest mass<\/dt>\r\n \t<dd id=\"fs-id1167793510596\">mass of an object as measured by an observer at rest relative to the object<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793241040\">\r\n \t<dt id=\"3561\">second postulate of special relativity<\/dt>\r\n \t<dd id=\"fs-id1167793383391\">light travels in a vacuum with the same speed<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>in any direction in all inertial frames<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167794207045\">\r\n \t<dt id=\"85691\">special theory of relativity<\/dt>\r\n \t<dd id=\"fs-id1167794188118\">theory that Albert Einstein proposed in 1905 that assumes all the laws of physics have the same form in every inertial frame of reference, and that the speed of light is the same within all inertial frames<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167794216029\">\r\n \t<dt id=\"86171\">speed of light<\/dt>\r\n \t<dd id=\"fs-id1167794216034\">ultimate speed limit for any particle having mass<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167794070887\">\r\n \t<dt id=\"48566\">time dilation<\/dt>\r\n \t<dd id=\"fs-id1167793924861\">lengthening of the time interval between two events when seen in a moving inertial frame rather than the rest frame of the events (in which the events occur at the same location)<\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167794127467\">\r\n \t<dt id=\"93135\">total energy<\/dt>\r\n \t<dd id=\"fs-id1167794127472\">sum of all energies for a particle, including rest energy and kinetic energy, given for a particle of mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>and speed<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>by<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1698-Frame\"><span class=\"MathJax_MathContainer\">E=\u03b3mc2,<\/span><\/span>\u00a0where\u00a0<span class=\"MathJax_MathML\" id=\"MathJax-Element-1699-Frame\"><span class=\"MathJax_MathContainer\">\u03b3=11\u2212u2c2<\/span><\/span><\/span><\/dd>\r\n<\/dl>\r\n<dl id=\"fs-id1167793777605\">\r\n \t<dt id=\"85530\">world line<\/dt>\r\n \t<dd id=\"fs-id1167793777610\">path through space-time<\/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-id1172100944609\" class=\"key-equations\" data-depth=\"1\">\r\n<div class=\"os-table\">\r\n<table id=\"fs-id1172098602739\" class=\"unnumbered unstyled\" style=\"width: 667px;height: 431px\" summary=\"Table 2.1 Refractive Indices Relevant to the Eye *This is an average value. The actual index of refraction varies throughout the lens and is greatest in center of the lens.\" data-label=\"\">\r\n<tbody>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Time dilation<\/td>\r\n<td style=\"width: 478px;height: 17px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1700-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394t=\u0394\u03c41\u2212v2c2=\u03b3\u03c4<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Lorentz factor<\/td>\r\n<td style=\"width: 478px;height: 17px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1701-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=11\u2212v2c2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Length contraction<\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1702-Frame\"><span class=\"MathJax_MathContainer\"><span>L=L01\u2212v2c2=L0\u03b3<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Galilean transformation<\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1703-Frame\"><span class=\"MathJax_MathContainer\"><span>x=x\u2032+vt,y=y\u2032,z=z\u2032,t=t\u2032<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Lorentz transformation<\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1704-Frame\"><span class=\"MathJax_MathContainer\"><span>t=t\u2032+vx\u2032\/c21\u2212v2\/c2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1705-Frame\"><span class=\"MathJax_MathContainer\"><span>x=x\u2032+vt\u20321\u2212v2\/c2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1706-Frame\"><span class=\"MathJax_MathContainer\"><span>y=y\u2032<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1707-Frame\"><span class=\"MathJax_MathContainer\"><span>z=z\u2032<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 35px\">\r\n<td style=\"width: 189px;height: 35px\" data-align=\"left\">Inverse Lorentz transformation<\/td>\r\n<td style=\"width: 478px;height: 35px\" data-align=\"left\">t\u2032=t\u2212vx\/c21\u2212v2\/c2<\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1709-Frame\"><span class=\"MathJax_MathContainer\"><span>x\u2032=x\u2212vt1\u2212v2\/c2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1710-Frame\"><span class=\"MathJax_MathContainer\"><span>y\u2032=y<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1711-Frame\"><span class=\"MathJax_MathContainer\"><span>z\u2032=z<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Space-time invariants<\/td>\r\n<td style=\"width: 478px;height: 17px\" data-align=\"left\">(\u0394s)2=(\u0394x)2+(\u0394y)2+(\u0394z)2\u2212c2(\u0394t)2<\/td>\r\n<\/tr>\r\n<tr style=\"height: 35px\">\r\n<td style=\"width: 189px;height: 35px\" data-align=\"left\"><\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1713-Frame\"><span class=\"MathJax_MathContainer\"><span>(\u0394\u03c4)2=\u2212(\u0394s)2\/c2=(\u0394t)2\u2212[(\u0394x)2+(\u0394y)2+(\u0394z)2]c2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 35px\">\r\n<td style=\"width: 189px;height: 35px\" data-align=\"left\">Relativistic velocity addition<\/td>\r\n<td style=\"width: 478px;height: 35px\" data-align=\"left\">ux=(ux\u2032+v1+vux\u2032\/c2),uy=(uy\u2032\/\u03b31+vux\u2032\/c2),uz=(uz\u2032\/\u03b31+vux\u2032\/c2)<\/td>\r\n<\/tr>\r\n<tr style=\"height: 35px\">\r\n<td style=\"width: 189px;height: 35px\" data-align=\"left\">Relativistic Doppler effect for wavelength<\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1715-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bbobs=\u03bbs1+vc1\u2212vc<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 35px\">\r\n<td style=\"width: 189px;height: 35px\" data-align=\"left\">Relativistic Doppler effect for frequency<\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1716-Frame\"><span class=\"MathJax_MathContainer\"><span>fobs=fs1\u2212vc1+vc<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 18px\">\r\n<td style=\"width: 189px;height: 18px\" data-align=\"left\">Relativistic momentum<\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1717-Frame\"><span class=\"MathJax_MathContainer\"><span>p\u2192=\u03b3mu\u2192=mu\u21921\u2212u2c<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Relativistic total energy<\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1718-Frame\"><span class=\"MathJax_MathContainer\"><span>E=\u03b3mc2,where\u03b3=11\u2212u2c2<\/span><\/span><\/span><\/td>\r\n<\/tr>\r\n<tr style=\"height: 17px\">\r\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Relativistic kinetic energy<\/td>\r\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1719-Frame\"><span class=\"MathJax_MathContainer\"><span>Krel=(\u03b3\u22121)mc2,where\u03b3=11\u2212u2c2<\/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-id1167793568935\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"28720_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-1-invariance-of-physical-laws\/\"><span class=\"os-number\">1.1<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Invariance of Physical Laws<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1167793912156\" data-bullet-style=\"bullet\">\r\n \t<li>Relativity is the study of how observers in different reference frames measure the same event.<\/li>\r\n \t<li>Modern relativity is divided into two parts. Special relativity deals with observers in uniform (unaccelerated) motion, whereas general relativity includes accelerated relative motion and gravity. Modern relativity is consistent with all empirical evidence thus far and, in the limit of low velocity and weak gravitation, gives close agreement with the predictions of classical (Galilean) relativity.<\/li>\r\n \t<li>An inertial frame of reference is a reference frame in which a body at rest remains at rest and a body in motion moves at a constant speed in a straight line unless acted upon by an outside force.<\/li>\r\n \t<li>Modern relativity is based on Einstein\u2019s two postulates. The first postulate of special relativity is that the laws of physics are the same in all inertial frames of reference. The second postulate of special relativity is that the speed of light<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>is the same in all inertial frames of reference, independent of the relative motion of the observer and the light source.<\/li>\r\n \t<li>The Michelson-Morley experiment demonstrated that the speed of light in a vacuum is independent of the motion of Earth about the sun.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1167794052056\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"41148_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-2-relativity-of-simultaneity\/\"><span class=\"os-number\">1.2<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativity of Simultaneity<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1167794071141\" data-bullet-style=\"bullet\">\r\n \t<li>Two events are defined to be simultaneous if an observer measures them as occurring at the same time (such as by receiving light from the events).<\/li>\r\n \t<li>Two events at locations a distance apart that are simultaneous for an observer at rest in one frame of reference are not necessarily simultaneous for an observer at rest in a different frame of reference.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1167794159499\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"16808_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-3-time-dilation\/\"><span class=\"os-number\">1.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Time Dilation<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1167793473277\" data-bullet-style=\"bullet\">\r\n \t<li>Two events are defined to be simultaneous if an observer measures them as occurring at the same time. They are not necessarily simultaneous to all observers\u2014simultaneity is not absolute.<\/li>\r\n \t<li>Time dilation is the lengthening of the time interval between two events when seen in a moving inertial frame rather than the rest frame of the events (in which the events occur at the same location).<\/li>\r\n \t<li>Observers moving at a relative velocity<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>do not measure the same elapsed time between two events. Proper time<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1720-Frame\"><span class=\"MathJax_MathContainer\">\u0394\u03c4<\/span><\/span>\u00a0<\/span>is the time measured in the reference frame where the start and end of the time interval occur at the same location. The time interval<span> \u0394t<\/span><span>\u00a0<\/span>measured by an observer who sees the frame of events moving at speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is related to the proper time interval<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1722-Frame\"><span class=\"MathJax_MathContainer\">\u0394\u03c4<\/span><\/span>\u00a0<\/span>of the events by the equation:<span data-type=\"newline\">\r\n<\/span>\r\n<div class=\"unnumbered\" data-label=\"\" data-type=\"equation\" id=\"fs-id1167794210772\">\r\n<div class=\"MathJax_Display\">\u0394t=\u0394\u03c41\u2212v2c2=\u03b3\u0394\u03c4,<\/div>\r\n<\/div>\r\nwhere<span data-type=\"newline\">\r\n<\/span>\r\n<div class=\"unnumbered\" data-label=\"\" data-type=\"equation\" id=\"fs-id1167794139375\">\r\n<div class=\"MathJax_Display\">\u03b3=11\u2212v2c2.<\/div>\r\n<\/div><\/li>\r\n \t<li>The premise of the twin paradox is faulty because the traveling twin is accelerating. The journey is not symmetrical for the two twins.<\/li>\r\n \t<li>Time dilation is usually negligible at low relative velocities, but it does occur, and it has been verified by experiment.<\/li>\r\n \t<li>The proper time is the shortest measure of any time interval. Any observer who is moving relative to the system being observed measures a time interval longer than the proper time.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1167793466427\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"55108_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-4-length-contraction\/\"><span class=\"os-number\">1.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Length Contraction<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1167793301194\" data-bullet-style=\"bullet\">\r\n \t<li>All observers agree upon relative speed.<\/li>\r\n \t<li>Distance depends on an observer\u2019s motion. Proper length<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1725-Frame\"><span class=\"MathJax_MathContainer\">L0<\/span><\/span>\u00a0<\/span>is the distance between two points measured by an observer who is at rest relative to both of the points.<\/li>\r\n \t<li>Length contraction is the decrease in observed length of an object from its proper length<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1725-Frame\"><span class=\"MathJax_MathContainer\">L0<\/span><\/span>\u00a0<\/span>to length<span>\u00a0<\/span><em data-effect=\"italics\">L<\/em><span>\u00a0<\/span>when its length is observed in a reference frame where it is traveling at speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em>.<\/li>\r\n \t<li>The proper length is the longest measurement of any length interval. Any observer who is moving relative to the system being observed measures a length shorter than the proper length.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1167793547990\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"1528_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-5-the-lorentz-transformation\/\"><span class=\"os-number\">1.5<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">The Lorentz Transformation<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1167793547997\" data-bullet-style=\"bullet\">\r\n \t<li>The Galilean transformation equations describe how, in classical nonrelativistic mechanics, the position, velocity, and accelerations measured in one frame appear in another. Lengths remain unchanged and a single universal time scale is assumed to apply to all inertial frames.<\/li>\r\n \t<li>Newton\u2019s laws of mechanics obey the principle of having the same form in all inertial frames under a Galilean transformation, given by<span data-type=\"newline\">\r\n<\/span>\r\n<div class=\"unnumbered\" data-label=\"\" data-type=\"equation\" id=\"fs-id1167793384555\">\r\n<div class=\"MathJax_Display\">x=x\u2032+vt,y=y\u2032,z=z\u2032,t=t\u2032.<\/div>\r\n<\/div>\r\nThe concept that times and distances are the same in all inertial frames in the Galilean transformation, however, is inconsistent with the postulates of special relativity.<\/li>\r\n<\/ul>\r\nThe relativistically correct Lorentz transformation equations are<span data-type=\"newline\">\r\n<\/span>\r\n<div class=\"unnumbered\" data-label=\"\" data-type=\"equation\" id=\"fs-id1167793831535\">\r\n<div class=\"MathJax_Display\">\r\n\r\nLorentz transformation\r\n<span data-type=\"newline\">t=t\u2032+vx\u2032\/c21\u2212v2\/c2\r\nx=x\u2032+vt\u20321\u2212v2\/c2\r\ny=y\u2032\r\nz=z\u2032<\/span>\r\n\r\nInverse Lorentz transformation\r\n<span style=\"font-size: 14pt\">t\u2032=t\u2212vx\/c21\u2212v2\/c2\r\n<\/span><span style=\"font-size: 14pt\">x\u2032=x\u2212vt1\u2212v2\/c2\r\n<span data-type=\"newline\">y\u2032=y\r\nz\u2032=z<\/span>\r\n<\/span>\r\n\r\n<\/div>\r\n<\/div>\r\n<span data-type=\"newline\">\r\n<\/span>We can obtain these equations by requiring an expanding spherical light signal to have the same shape and speed of growth,<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>, in both reference frames.\r\n<ul id=\"fs-id1167793547997\" data-bullet-style=\"bullet\">\r\n \t<li>Relativistic phenomena can be explained in terms of the geometrical properties of four-dimensional space-time, in which Lorentz transformations correspond to rotations of axes.<\/li>\r\n \t<li>The Lorentz transformation corresponds to a space-time axis rotation, similar in some ways to a rotation of space axes, but in which the invariant spatial separation is given by<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1729-Frame\"><span class=\"MathJax_MathContainer\">\u0394s<\/span><\/span>\u00a0<\/span>rather than distances<span> \u0394r,\u00a0<\/span>and that the Lorentz transformation involving the time axis does not preserve perpendicularity of axes or the scales along the axes.<\/li>\r\n \t<li>The analysis of relativistic phenomena in terms of space-time diagrams supports the conclusion that these phenomena result from properties of space and time itself, rather than from the laws of electromagnetism.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1167793499870\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"75851_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-6-relativistic-velocity-transformation\/\"><span class=\"os-number\">1.6<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Velocity Transformation<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1167794051357\" data-bullet-style=\"bullet\">\r\n \t<li>With classical velocity addition, velocities add like regular numbers in one-dimensional motion:<span> u=v+u\u2032,<\/span><span>\u00a0<\/span>where<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is the velocity between two observers,<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>is the velocity of an object relative to one observer, and<span> u\u2032<\/span><span>\u00a0<\/span>is the velocity relative to the other observer.<\/li>\r\n \t<li>Velocities cannot add to be greater than the speed of light.<\/li>\r\n \t<li>Relativistic velocity addition describes the velocities of an object moving at a relativistic velocity.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1167794296163\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"36417_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-7-doppler-effect-for-light\/\"><span class=\"os-number\">1.7<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Doppler Effect for Light<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1167793960641\" data-bullet-style=\"bullet\">\r\n \t<li>An observer of electromagnetic radiation sees relativistic Doppler effects if the source of the radiation is moving relative to the observer. The wavelength of the radiation is longer (called a red shift) than that emitted by the source when the source moves away from the observer and shorter (called a blue shift) when the source moves toward the observer. The shifted wavelength is described by the equation:<span data-type=\"newline\">\r\n<\/span>\r\n<div class=\"unnumbered\" data-label=\"\" data-type=\"equation\" id=\"fs-id1167794330470\">\r\n<div class=\"MathJax_Display\">\u03bbobs=\u03bbs1+vc1\u2212vc.<\/div>\r\n<\/div>\r\nwhere<span> \u03bbobs\u00a0<\/span>is the observed wavelength,<span> \u03bbs<\/span><span>\u00a0<\/span>is the source wavelength, and<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is the relative velocity of the source to the observer.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1167794051790\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"68539_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-8-relativistic-momentum\/\"><span class=\"os-number\">1.8<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Momentum<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1167793976155\" data-bullet-style=\"bullet\">\r\n \t<li>The law of conservation of momentum is valid for relativistic momentum whenever the net external force is zero. The relativistic momentum is<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1736-Frame\"><span class=\"MathJax_MathContainer\">p=\u03b3mu,<\/span><\/span>\u00a0<\/span>where<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>is the rest mass of the object,<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>is its velocity relative to an observer, and the relativistic factor is<span> \u03b3=11\u2212u2c2.<\/span><\/li>\r\n \t<li>At low velocities, relativistic momentum is equivalent to classical momentum.<\/li>\r\n \t<li>Relativistic momentum approaches infinity as<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>approaches<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>. This implies that an object with mass cannot reach the speed of light.<\/li>\r\n<\/ul>\r\n<\/section><\/div>\r\n<div class=\"os-section-area\"><section id=\"fs-id1167794314613\" class=\"key-concepts\" data-depth=\"1\">\r\n<h4 id=\"57975_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-9-relativistic-energy\/\"><span class=\"os-number\">1.9<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Energy<\/span><\/a><\/h4>\r\n<ul id=\"fs-id1167794314620\" data-bullet-style=\"bullet\">\r\n \t<li>The relativistic work-energy theorem is<span> Wnet=E\u2212E0=\u03b3mc2\u2212mc2=(\u03b3\u22121)mc2.<\/span><\/li>\r\n \t<li>Relativistically,<span> Wnet=Krel\u00a0<\/span>where<span> Krel\u00a0<\/span>is the relativistic kinetic energy.<\/li>\r\n \t<li>An object of<span>\u00a0<\/span><em data-effect=\"italics\">mass<\/em><span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>at velocity<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>has kinetic energy<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1741-Frame\"><span class=\"MathJax_MathContainer\">Krel=(\u03b3\u22121)mc2,<\/span><\/span>\u00a0where\u00a0<span class=\"MathJax_MathML\" id=\"MathJax-Element-1742-Frame\"><span class=\"MathJax_MathContainer\">\u03b3=11\u2212u2c2.<\/span><\/span><\/span><\/li>\r\n \t<li>At low velocities, relativistic kinetic energy reduces to classical kinetic energy.<\/li>\r\n \t<li>No object with mass can attain the speed of light, because an infinite amount of work and an infinite amount of energy input is required to accelerate a mass to the speed of light.<\/li>\r\n \t<li>Relativistic energy is conserved as long as we define it to include the possibility of mass changing to energy.<\/li>\r\n \t<li>The total energy of a particle with mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>traveling at speed<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>is defined as<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1743-Frame\"><span class=\"MathJax_MathContainer\">E=\u03b3mc2,<\/span><\/span>\u00a0<\/span>where\u00a0<span class=\"MathJax_MathML\" id=\"MathJax-Element-1744-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=11\u2212u2c2<\/span><\/span><\/span><span>\u00a0a<\/span>nd<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>denotes the velocity of the particle.<\/li>\r\n \t<li>The rest energy of an object of mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>is<span> E0=mc2,\u00a0<\/span>meaning that mass is a form of energy. If energy is stored in an object, its mass increases. Mass can be destroyed to release energy.<\/li>\r\n \t<li>We do not ordinarily notice the increase or decrease in mass of an object because the change in mass is so small for a large increase in energy. The equation<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1746-Frame\"><span class=\"MathJax_MathContainer\">E2=(pc)2+(mc2)2<\/span><\/span>\u00a0<\/span><span>\u00a0<\/span>relates the relativistic total energy<span>\u00a0<\/span><em data-effect=\"italics\">E<\/em><span>\u00a0<\/span>and the relativistic momentum<span>\u00a0<\/span><em data-effect=\"italics\">p<\/em>. At extremely high velocities, the rest energy<span> mc2<\/span><span>\u00a0<\/span>becomes negligible, and<span> E=pc.<\/span><\/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-id1167793269073\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"28720_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-1-invariance-of-physical-laws\/\"><span class=\"os-number\">1.1<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Invariance of Physical Laws<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793869864\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793953460\">\r\n\r\n1<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793640552\">Which of Einstein\u2019s postulates of special relativity includes a concept that does not fit with the ideas of classical physics? Explain.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793499879\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794101041\">\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-id1167793927571\">Is Earth an inertial frame of reference? Is the sun? Justify your response.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794003397\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794334344\">\r\n\r\n3<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794023568\">When you are flying in a commercial jet, it may appear to you that the airplane is stationary and Earth is moving beneath you. Is this point of view valid? Discuss briefly.<\/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-id1167794175883\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"16808_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-3-time-dilation\/\"><span class=\"os-number\">1.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Time Dilation<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793376295\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793395185\">\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-id1167793887481\">(a) Does motion affect the rate of a clock as measured by an observer moving with it? (b) Does motion affect how an observer moving relative to a clock measures its rate?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794325147\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793945117\">\r\n\r\n5<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793558006\">To whom does the elapsed time for a process seem to be longer, an observer moving relative to the process or an observer moving with the process? Which observer measures the interval of proper time?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793262959\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793624997\">\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-id1167793220373\">(a) How could you travel far into the future of Earth without aging significantly? (b) Could this method also allow you to travel into the past?<\/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-id1167793299668\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"55108_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-4-length-contraction\/\"><span class=\"os-number\">1.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Length Contraction<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793362235\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793362237\">\r\n\r\n7<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793280699\">To whom does an object seem greater in length, an observer moving with the object or an observer moving relative to the object? Which observer measures the object\u2019s proper length?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794090542\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793926426\">\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-id1167793926428\">Relativistic effects such as time dilation and length contraction are present for cars and airplanes. Why do these effects seem strange to us?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793441636\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793441638\">\r\n\r\n9<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794296704\">Suppose an astronaut is moving relative to Earth at a significant fraction of the speed of light. (a) Does he observe the rate of his clocks to have slowed? (b) What change in the rate of earthbound clocks does he see? (c) Does his ship seem to him to shorten? (d) What about the distance between two stars that lie in the direction of his motion? (e) Do he and an earthbound observer agree on his velocity relative to Earth?<\/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-id1167793238016\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"36417_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-7-doppler-effect-for-light\/\"><span class=\"os-number\">1.7<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Doppler Effect for Light<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794329262\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793896608\">\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-id1167793989777\">Explain the meaning of the terms \u201cred shift\u201d and \u201cblue shift\u201d as they relate to the relativistic Doppler effect.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793787639\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794188024\">\r\n\r\n11<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793251224\">What happens to the relativistic Doppler effect when relative velocity is zero? Is this the expected result?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794100180\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793877466\">\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-id1167793895380\">Is the relativistic Doppler effect consistent with the classical Doppler effect in the respect that<span> \u03bbobs<\/span><span>\u00a0<\/span>is larger for motion away?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793591205\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794069449\">\r\n\r\n13<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794022158\">All galaxies farther away than about<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1750-Frame\"><span class=\"MathJax_MathContainer\">50\u00d7106ly<\/span><\/span>\u00a0<\/span>exhibit a red shift in their emitted light that is proportional to distance, with those farther and farther away having progressively greater red shifts. What does this imply, assuming that the only source of red shift is relative motion?<\/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-id1167793435694\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"68539_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-8-relativistic-momentum\/\"><span class=\"os-number\">1.8<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Momentum<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793629296\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793237831\">\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-id1167793938240\">How does modern relativity modify the law of conservation of momentum?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794326162\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793985685\">\r\n\r\n15<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794210766\">Is it possible for an external force to be acting on a system and relativistic momentum to be conserved? Explain.<\/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-id1167794032273\" class=\"review-conceptual-questions\" data-depth=\"1\">\r\n<h4 id=\"57975_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-9-relativistic-energy\/\"><span class=\"os-number\">1.9<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Energy<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794032281\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794032283\">\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-id1167794032285\">How are the classical laws of conservation of energy and conservation of mass modified by modern relativity?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793788572\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793788574\">\r\n\r\n17<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793788576\">What happens to the mass of water in a pot when it cools, assuming no molecules escape or are added? Is this observable in practice? Explain.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793495017\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793495020\">\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-id1167793495022\">Consider a thought experiment. You place an expanded balloon of air on weighing scales outside in the early morning. The balloon stays on the scales and you are able to measure changes in its mass. Does the mass of the balloon change as the day progresses? Discuss the difficulties in carrying out this 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-id1167793638889\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793638891\">\r\n\r\n19<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793638893\">The mass of the fuel in a nuclear reactor decreases by an observable amount as it puts out energy. Is the same true for the coal and oxygen combined in a conventional power plant? If so, is this observable in practice for the coal and oxygen? Explain.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794296573\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794296575\">\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-id1167794296577\">We know that the velocity of an object with mass has an upper limit of<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>. Is there an upper limit on its momentum? Its energy? 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-id1167793633482\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793633484\">\r\n\r\n21<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793633486\">Given the fact that light travels at<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>, can it have mass? Explain.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794097177\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794097180\">\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-id1167794097182\">If you use an Earth-based telescope to project a laser beam onto the moon, you can move the spot across the moon\u2019s surface at a velocity greater than the speed of light. Does this violate modern relativity? (Note that light is being sent from the Earth to the moon, not across the surface of the moon.)<\/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-id1167793603932\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"16808_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-3-time-dilation\/\"><span class=\"os-number\">1.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Time Dilation<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793862957\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794051776\">\r\n\r\n23<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793355328\">(a) <span>What is\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1751-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0if\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1752-Frame\"><span class=\"MathJax_MathContainer\"><span>v=0.250c?<\/span><\/span><\/span><span>\u00a0(b) If\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1753-Frame\"><span class=\"MathJax_MathContainer\"><span>v=0.500c?<\/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-id1167793379179\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794146271\">\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-id1167793928666\"><span>(a) What is\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1754-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0if\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1755-Frame\"><span class=\"MathJax_MathContainer\"><span>v=0.100c?<\/span><\/span><\/span><span>\u00a0(b) If\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1756-Frame\"><span class=\"MathJax_MathContainer\"><span>v=0.900c?<\/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-id1167793442208\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794327628\">\r\n\r\n25<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794327630\"><span>Particles called\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1757-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c0<\/span><\/span><\/span><span>-mesons are produced by accelerator beams. If these particles travel at\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1758-Frame\"><span class=\"MathJax_MathContainer\"><span>2.70\u00d7108m\/s<\/span><\/span><\/span><span>\u00a0and live\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1759-Frame\"><span class=\"MathJax_MathContainer\"><span>2.60\u00d710\u22128s\u00a0<\/span><\/span><\/span><span>when at rest relative to an observer, how long do they live as viewed in the laboratory?<\/span><\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793516837\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793516839\">\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-id1167794097955\"><span>Suppose a particle called a kaon is created by cosmic radiation striking the atmosphere. It moves by you at\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1760-Frame\"><span class=\"MathJax_MathContainer\"><span>0.980c,<\/span><\/span><\/span><span>\u00a0and it lives\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1761-Frame\"><span class=\"MathJax_MathContainer\"><span>1.24\u00d710\u22128s<\/span><\/span><\/span><span>\u00a0when at rest relative to an observer. How long does it live as you observe it?<\/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-id1167793401205\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793401207\">\r\n\r\n27<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793418092\">A neutral<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1762-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c0<\/span><\/span><\/span>-meson is a particle that can be created by accelerator beams. If one such particle lives<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1763-Frame\"><span class=\"MathJax_MathContainer\"><span>1.40\u00d710\u221216s<\/span><\/span><\/span><span>\u00a0<\/span>as measured in the laboratory, and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1764-Frame\"><span class=\"MathJax_MathContainer\"><span>0.840\u00d710\u221216s<\/span><\/span><\/span><span>\u00a0<\/span>when at rest relative to an observer, what is its velocity relative to the laboratory?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793261501\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793261503\">\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-id1167793248364\"><span>A neutron lives 900 s when at rest relative to an observer. How fast is the neutron moving relative to an observer who measures its life span to be 2065 s?<\/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-id1167793291690\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793291692\">\r\n\r\n29<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n\r\n<span class=\"os-divider\"><span>\u00a0<\/span><\/span><span style=\"font-size: 14pt\">If relativistic effects are to be less than 1%, then<\/span><span style=\"font-size: 14pt\">\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1765-Frame\" style=\"font-size: 14pt\"><span class=\"MathJax_MathContainer\">\u03b3<\/span><\/span><span style=\"font-size: 14pt\">\u00a0<\/span><span style=\"font-size: 14pt\">must be less than 1.01. At what relative velocity is<\/span><span style=\"font-size: 14pt\">\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1766-Frame\" style=\"font-size: 14pt\"><span class=\"MathJax_MathContainer\">\u03b3=1.01?<\/span><\/span>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793992264\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793992266\">\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-id1167793385868\"><span>If relativistic effects are to be less than 3%, then\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1767-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0must be less than 1.03. At what relative velocity is\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1768-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=1.03?<\/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-id1167794071932\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"55108_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-4-length-contraction\/\"><span class=\"os-number\">1.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Length Contraction<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793543353\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793268123\">\r\n\r\n31<span class=\"os-divider\">.<span><\/span><\/span>\r\n<div class=\"os-review-problems-container\">\r\n<div class=\"os-review-problems\">\r\n<div class=\"os-section-area\"><section id=\"fs-id1167794071932\" class=\"review-problems\" data-depth=\"1\">\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793543353\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793268123\"><span style=\"font-size: 14pt\">A spaceship, 200 m long as seen on board, moves by the Earth at 0.970<\/span><em style=\"font-size: 14pt\" data-effect=\"italics\">c<\/em><span style=\"font-size: 14pt\">. What is its length as measured by an earthbound observer?<\/span><\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793638126\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793638128\">\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-id1167793638130\">How fast would a 6.0 m-long sports car have to be going past you in order for it to appear only 5.5 m long?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793377362\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793377364\">\r\n\r\n33<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793377366\">(a) How far does the muon in<span>\u00a0<\/span>Example 1.3<span>\u00a0<\/span>travel according to the earthbound observer? (b) How far does it travel as viewed by an observer moving with it? Base your calculation on its velocity relative to the Earth and the time it lives (proper time). (c) Verify that these two distances are related through length contraction<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1769-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=3.20.<\/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-id1167793432903\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793432905\">\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-id1167794095197\">(a) How long would the muon in<span>\u00a0<\/span>Example 1.3<span>\u00a0<\/span>have lived as observed on Earth if its velocity was<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1770-Frame\"><span class=\"MathJax_MathContainer\"><span>0.0500c?<\/span><\/span><\/span><span>\u00a0<\/span>(b) How far would it have traveled as observed on Earth? (c) What distance is this in the muon\u2019s frame?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793363299\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793363301\">\r\n\r\n35<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793960774\"><strong data-effect=\"bold\">Unreasonable Results<\/strong><span>\u00a0<\/span>A spaceship is heading directly toward Earth at a velocity of 0.800<em data-effect=\"italics\">c<\/em>. The astronaut on board claims that he can send a canister toward the Earth at 1.20<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>relative to Earth. (a) Calculate the velocity the canister must have relative to the spaceship. (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent?<\/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-id1167793362177\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"1528_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-5-the-lorentz-transformation\/\"><span class=\"os-number\">1.5<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">The Lorentz Transformation<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793362185\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793362187\">\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-id1167793362189\">Describe the following physical occurrences as events, that is, in the form (<em data-effect=\"italics\">x<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">y<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">z<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">t<\/em>): (a) A postman rings a doorbell of a house precisely at noon. (b) At the same time as the doorbell is rung, a slice of bread pops out of a toaster that is located 10 m from the door in the east direction from the door. (c) Ten seconds later, an airplane arrives at the airport, which is 10 km from the door in the east direction and 2 km to the south.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793506346\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793506348\">\r\n\r\n37<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793506351\">Describe what happens to the angle<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1771-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b1=tan(v\/c),<\/span><\/span><\/span><span>\u00a0<\/span>and therefore to the transformed axes in<span>\u00a0<\/span>Figure 1.17, as the relative velocity<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>of the S and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1772-Frame\"><span class=\"MathJax_MathContainer\"><span>S\u2032<\/span><\/span><\/span><span>\u00a0<\/span>frames of reference approaches<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=\"\" data-type=\"exercise\" id=\"fs-id1167794336770\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794336772\">\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-id1167794336774\">Describe the shape of the world line on a space-time diagram of (a) an object that remains at rest at a specific position along the<span>\u00a0<\/span><em data-effect=\"italics\">x-<\/em>axis; (b) an object that moves at constant velocity<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>in the<span>\u00a0<\/span><em data-effect=\"italics\">x-<\/em>direction; (c) an object that begins at rest and accelerates at a constant rate of in the positive<span>\u00a0<\/span><em data-effect=\"italics\">x-<\/em>direction.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793581706\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793581708\">\r\n\r\n39<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793581710\">A man standing still at a train station watches two boys throwing a baseball in a moving train. Suppose the train is moving east with a constant speed of 20 m\/s and one of the boys throws the ball with a speed of 5 m\/s with respect to himself toward the other boy, who is 5 m west from him. What is the velocity of the ball as observed by the man on the station?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794137014\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794137016\">\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-id1167794137018\">When observed from the sun at a particular instant, Earth and Mars appear to move in opposite directions with speeds 108,000 km\/h and 86,871 km\/h, respectively. What is the speed of Mars at this instant when observed from Earth?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793510460\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793510462\">\r\n\r\n41<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793510464\">A man is running on a straight road perpendicular to a train track and away from the track at a speed of 12 m\/s. The train is moving with a speed of 30 m\/s with respect to the track. What is the speed of the man with respect to a passenger sitting at rest in the train?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793510479\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793510481\">\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-id1167793510483\">A man is running on a straight road that makes<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1773-Frame\"><span class=\"MathJax_MathContainer\"><span>30\u00b0<\/span><\/span><\/span><span>\u00a0<\/span>with the train track. The man is running in the direction on the road that is away from the track at a speed of 12 m\/s. The train is moving with a speed of 30 m\/s with respect to the track. What is the speed of the man with respect to a passenger sitting at rest in the train?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793603752\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793603755\">\r\n\r\n43<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793603757\">In a frame at rest with respect to the billiard table, a billiard ball of mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>moving with speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>strikes another billiard ball of mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>at rest. The first ball comes to rest after the collision while the second ball takes off with speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>in the original direction of the motion of the first ball. This shows that momentum is conserved in this frame. (a) Now, describe the same collision from the perspective of a frame that is moving with speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>in the direction of the motion of the first ball. (b) Is the momentum conserved in this frame?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794163815\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794163817\">\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-id1167794163819\">In a frame at rest with respect to the billiard table, two billiard balls of same mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>are moving toward each other with the same speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em>. After the collision, the two balls come to rest. (a) Show that momentum is conserved in this frame. (b) Now, describe the same collision from the perspective of a frame that is moving with speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>in the direction of the motion of the first ball. (c) Is the momentum conserved in this frame?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794160228\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794160231\">\r\n\r\n45<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794160233\">In a frame S, two events are observed: event 1: a pion is created at rest at the origin and event 2: the pion disintegrates after time<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1774-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c4<\/span><\/span><\/span>. Another observer in a frame<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1775-Frame\"><span class=\"MathJax_MathContainer\"><span>S\u2032<\/span><\/span><\/span><span>\u00a0<\/span>is moving in the positive direction along the positive<span>\u00a0<\/span><em data-effect=\"italics\">x<\/em>-axis with a constant speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em>and observes the same two events in his frame. The origins of the two frames coincide at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1776-Frame\"><span class=\"MathJax_MathContainer\"><span>t=t\u2032=0.<\/span><\/span><\/span><span>\u00a0<\/span>(a) Find the positions and timings of these two events in the frame<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1777-Frame\"><span class=\"MathJax_MathContainer\"><span>S\u2032<\/span><\/span><\/span><span>\u00a0<\/span>(a) according to the Galilean transformation, and (b) according to the Lorentz transformation.<\/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-id1167793354906\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"75851_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-6-relativistic-velocity-transformation\/\"><span class=\"os-number\">1.6<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Velocity Transformation<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793593202\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794065574\">\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-id1167794065576\">If two spaceships are heading directly toward each other at 0.800<em data-effect=\"italics\">c<\/em>, at what speed must a canister be shot from the first ship to approach the other at 0.999<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>as seen by the second ship?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793618179\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793618181\">\r\n\r\n47<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793618183\">Two planets are on a collision course, heading directly toward each other at 0.250<em data-effect=\"italics\">c<\/em>. A spaceship sent from one planet approaches the second at 0.750<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>as seen by the second planet. What is the velocity of the ship relative to the first planet?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793462690\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793462692\">\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-id1167793503978\">When a missile is shot from one spaceship toward another, it leaves the first at 0.950<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>and approaches the other at 0.750<em data-effect=\"italics\">c<\/em>. What is the relative velocity of the two ships?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793450526\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793515300\">\r\n\r\n49<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793515302\">What is the relative velocity of two spaceships if one fires a missile at the other at 0.750<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>and the other observes it to approach at 0.950<em data-effect=\"italics\">c<\/em>?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793371632\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793371634\">\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-id1167793371636\">Prove that for any relative velocity<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>between two observers, a beam of light sent from one to the other will approach at speed<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>(provided that<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is less than<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>, of course).<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793372830\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793372832\">\r\n\r\n51<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794098950\">Show that for any relative velocity<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>between two observers, a beam of light projected by one directly away from the other will move away at the speed of light (provided that<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is less than<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>, of course).<\/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-id1167794125603\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"36417_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-7-doppler-effect-for-light\/\"><span class=\"os-number\">1.7<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Doppler Effect for Light<\/span><\/a><\/h4>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794028783\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794328906\">\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-id1167793662487\">A highway patrol officer uses a device that measures the speed of vehicles by bouncing radar off them and measuring the Doppler shift. The outgoing radar has a frequency of 100 GHz and the returning echo has a frequency 15.0 kHz higher. What is the velocity of the vehicle? Note that there are two Doppler shifts in echoes. Be certain not to round off until the end of the problem, because the effect is small.<\/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-id1167793999292\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"68539_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-8-relativistic-momentum\/\"><span class=\"os-number\">1.8<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Momentum<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794170660\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793290850\">\r\n\r\n53<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794027273\">Find the momentum of a helium nucleus having a mass of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1778-Frame\"><span class=\"MathJax_MathContainer\"><span>6.68\u00d710\u221227kg<\/span><\/span><\/span><span>\u00a0<\/span>that is moving at 0.200<em data-effect=\"italics\">c<\/em>.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793219303\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793442787\">\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-id1167794169326\">What is the momentum of an electron traveling at 0.980<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-id1167793931807\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794328891\">\r\n\r\n55<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794284915\">(a) Find the momentum of a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1779-Frame\"><span class=\"MathJax_MathContainer\"><span>1.00\u00d7109-kg<\/span><\/span><\/span><span>\u00a0<\/span>asteroid heading towards Earth at 30.0 km\/s. (b) Find the ratio of this momentum to the classical momentum. (Hint: Use the approximation that<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1780-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=1+(1\/2)v2\/c2<\/span><\/span><\/span><span>\u00a0<\/span>at low velocities.)<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794039506\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793376189\">\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-id1167793495147\">(a) What is the momentum of a 2000-kg satellite orbiting at 4.00 km\/s? (b) Find the ratio of this momentum to the classical momentum. (Hint: Use the approximation that<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1781-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=1+(1\/2)v2\/c2<\/span><\/span><\/span><span>\u00a0<\/span>at low velocities.)<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794026700\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794071266\">\r\n\r\n57<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793848355\">What is the velocity of an electron that has a momentum of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1782-Frame\"><span class=\"MathJax_MathContainer\"><span>3.04\u00d710\u221221kg\u00b7m\/s<\/span><\/span><\/span><span>\u00a0<\/span>? Note that you must calculate the velocity to at least four digits to see the difference from<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=\"\" data-type=\"exercise\" id=\"fs-id1167793933416\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794135652\">\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-id1167793637938\">Find the velocity of a proton that has a momentum of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1783-Frame\"><span class=\"MathJax_MathContainer\"><span>4.48\u00d710\u221219kg\u00b7m\/s.<\/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-id1167794181332\" class=\"review-problems\" data-depth=\"1\">\r\n<h4 id=\"57975_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-9-relativistic-energy\/\"><span class=\"os-number\">1.9<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Energy<\/span><\/a><\/h4>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794181339\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794181341\">\r\n\r\n59<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794181343\">What is the rest energy of an electron, given its mass is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1784-Frame\"><span class=\"MathJax_MathContainer\"><span>9.11\u00d710\u221231kg?<\/span><\/span><\/span><span>\u00a0<\/span>Give your answer in joules and MeV.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793554163\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793554165\">\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-id1167793554167\">Find the rest energy in joules and MeV of a proton, given its mass is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1785-Frame\"><span class=\"MathJax_MathContainer\"><span>1.67\u00d710\u221227kg.<\/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-id1167793547214\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793372797\">\r\n\r\n61<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793372799\">If the rest energies of a proton and a neutron (the two constituents of nuclei) are 938.3 and 939.6 MeV, respectively, what is the difference in their mass in kilograms?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793938876\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793938878\">\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-id1167793938880\">The Big Bang that began the universe is estimated to have released<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1786-Frame\"><span class=\"MathJax_MathContainer\"><span>1068J<\/span><\/span><\/span><span>\u00a0<\/span>of energy. How many stars could half this energy create, assuming the average star\u2019s mass is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1787-Frame\"><span class=\"MathJax_MathContainer\"><span>4.00\u00d71030kg<\/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-id1167793978530\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793978532\">\r\n\r\n63<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793978534\">A supernova explosion of a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1788-Frame\"><span class=\"MathJax_MathContainer\"><span>2.00\u00d71031kg<\/span><\/span><\/span><span>\u00a0<\/span>star produces<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1789-Frame\"><span class=\"MathJax_MathContainer\"><span>1.00\u00d71044J<\/span><\/span><\/span><span>\u00a0<\/span>of energy. (a) How many kilograms of mass are converted to energy in the explosion? (b) What is the ratio<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1790-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394m\/m<\/span><\/span><\/span><span>\u00a0<\/span>of mass destroyed to the original mass of the star?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793384967\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793384969\">\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-id1167793384971\">(a) Using data from<span>\u00a0<\/span><a href=\"https:\/\/cnx.org\/contents\/af275420-6050-4707-995c-57b9cc13c358@11.1:f36a3dfd-5697-445b-a5e6-c0642ed88f6d#fs-id1165036086155\" data-page=\"1\">Potential Energy of a System<\/a>, calculate the mass converted to energy by the fission of 1.00 kg of uranium. (b) What is the ratio of mass destroyed to the original mass,<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1791-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394m\/m?<\/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-id1167793928250\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793928252\">\r\n\r\n65<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793928254\">(a) Using data from<span>\u00a0<\/span><a href=\"https:\/\/cnx.org\/contents\/af275420-6050-4707-995c-57b9cc13c358@11.1:f36a3dfd-5697-445b-a5e6-c0642ed88f6d#fs-id1165036086155\" data-page=\"1\">Potential Energy of a System<\/a>, calculate the amount of mass converted to energy by the fusion of 1.00 kg of hydrogen. (b) What is the ratio of mass destroyed to the original mass,<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1792-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394m\/m<\/span><\/span><\/span><span>\u00a0<\/span>? (c) How does this compare with<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1793-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394m\/m\u00a0<\/span><\/span><\/span>for the fission of 1.00 kg of uranium?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794186600\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794186602\">\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-id1167794186604\">There is approximately<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1794-Frame\"><span class=\"MathJax_MathContainer\"><span>1034J<\/span><\/span><\/span><span>\u00a0<\/span>of energy available from fusion of hydrogen in the world\u2019s oceans. (a) If<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1795-Frame\"><span class=\"MathJax_MathContainer\"><span>1033J<\/span><\/span><\/span><span>\u00a0<\/span>of this energy were utilized, what would be the decrease in mass of the oceans? (b) How great a volume of water does this correspond to? (c) Comment on whether this is a significant fraction of the total mass of the oceans.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793371355\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793371357\">\r\n\r\n67<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793371359\">A muon has a rest mass energy of 105.7 MeV, and it decays into an electron and a massless particle. (a) If all the lost mass is converted into the electron\u2019s kinetic energy, find<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1796-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>for the electron. (b) What is the electron\u2019s velocity?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793371384\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793371386\">\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-id1167793641954\">A<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1797-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c0<\/span><\/span><\/span>-meson is a particle that decays into a muon and a massless particle. The<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1798-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c0<\/span><\/span><\/span>-meson has a rest mass energy of 139.6 MeV, and the muon has a rest mass energy of 105.7 MeV. Suppose the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1799-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c0<\/span><\/span><\/span>-meson is at rest and all of the missing mass goes into the muon\u2019s kinetic energy. How fast will the muon move?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793641984\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793641987\">\r\n\r\n69<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793641989\">(a) Calculate the relativistic kinetic energy of a 1000-kg car moving at 30.0 m\/s if the speed of light were only 45.0 m\/s. (b) Find the ratio of the relativistic kinetic energy to classical.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793626891\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793626893\">\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-id1167793626895\">Alpha decay is nuclear decay in which a helium nucleus is emitted. If the helium nucleus has a mass of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1800-Frame\"><span class=\"MathJax_MathContainer\"><span>6.80\u00d710\u221227kg<\/span><\/span><\/span><span>\u00a0<\/span>and is given 5.00 MeV of kinetic energy, what is its velocity?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793605318\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793605320\">\r\n\r\n71<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793605322\">(a) Beta decay is nuclear decay in which an electron is emitted. If the electron is given 0.750 MeV of kinetic energy, what is its velocity? (b) Comment on how the high velocity is consistent with the kinetic energy as it compares to the rest mass energy of the electron.<\/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-id1165039371212\" class=\"review-additional-problems\" data-depth=\"1\">\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793374981\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793374983\">\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-id1167793374986\">(a) At what relative velocity is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1801-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=1.50?<\/span><\/span><\/span><span>\u00a0<\/span>(b) At what relative velocity is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1802-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=100?<\/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-id1167793551988\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793551990\">\r\n\r\n73<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793551992\">(a) At what relative velocity is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1803-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=2.00?<\/span><\/span><\/span><span>\u00a0<\/span>(b) At what relative velocity is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1804-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=10.0?<\/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-id1167793384944\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793384946\">\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-id1167793384949\"><strong data-effect=\"bold\">Unreasonable Results<\/strong><span>\u00a0<\/span>(a) Find the value of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1805-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>required for the following situation. An earthbound observer measures 23.9 h to have passed while signals from a high-velocity space probe indicate that 24.0 h have passed on board. (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793376212\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793376214\">\r\n\r\n75<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793376216\">(a) How long does it take the astronaut in<span>\u00a0<\/span>Example 1.5<span>\u00a0<\/span>to travel 4.30 ly at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1806-Frame\"><span class=\"MathJax_MathContainer\"><span>0.99944c<\/span><\/span><\/span><span>\u00a0<\/span>(as measured by the earthbound observer)? (b) How long does it take according to the astronaut? (c) Verify that these two times are related through time dilation with<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1807-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=30.00<\/span><\/span><\/span><span>\u00a0<\/span>as given.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793599601\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793599603\">\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-id1167793599605\">(a) How fast would an athlete need to be running for a 100-<span class=\"MathJax_MathML\" id=\"MathJax-Element-1808-Frame\"><span class=\"MathJax_MathContainer\"><span>m<\/span><\/span><\/span><span>\u00a0<\/span>race to look 100 yd long? (b) Is the answer consistent with the fact that relativistic effects are difficult to observe in ordinary circumstances? 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-id1167793219328\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793219331\">\r\n\r\n77<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793219333\">(a) Find the value of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1809-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>for the following situation. An astronaut measures the length of his spaceship to be 100 m, while an earthbound observer measures it to be 25.0 m. (b) What is the speed of the spaceship relative to Earth?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793422000\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793422003\">\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-id1167793422005\">A clock in a spaceship runs one-tenth the rate at which an identical clock on Earth runs. What is the speed of the spaceship?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793422027\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794095442\">\r\n\r\n79<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794095444\">An astronaut has a heartbeat rate of 66 beats per minute as measured during his physical exam on Earth. The heartbeat rate of the astronaut is measured when he is in a spaceship traveling at 0.5<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>with respect to Earth by an observer (A) in the ship and by an observer (B) on Earth. (a) Describe an experimental method by which observer B on Earth will be able to determine the heartbeat rate of the astronaut when the astronaut is in the spaceship. (b) What will be the heartbeat rate(s) of the astronaut reported by observers A and B?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794326142\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794326144\">\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-id1167794326147\">A spaceship (A) is moving at speed<span>\u00a0<\/span><em data-effect=\"italics\">c\/<\/em>2 with respect to another spaceship (B). Observers in A and B set their clocks so that the event at (<em data-effect=\"italics\">x, y, z, t<\/em>) of turning on a laser in spaceship B has coordinates (0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0) in A and also (0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0) in B. An observer at the origin of B turns on the laser at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1810-Frame\"><span class=\"MathJax_MathContainer\"><span>t=0<\/span><\/span><\/span><span>\u00a0<\/span>and turns it off at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1811-Frame\"><span class=\"MathJax_MathContainer\"><span>t=\u03c4<\/span><\/span><\/span><span>\u00a0<\/span>in his time. What is the time duration between on and off as seen by an observer in A?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793245244\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793245246\">\r\n\r\n81<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793245248\">Same two observers as in the preceding exercise, but now we look at two events occurring in spaceship A. A photon arrives at the origin of A at its time<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1812-Frame\"><span class=\"MathJax_MathContainer\"><span>t=0<\/span><\/span><\/span><span>\u00a0<\/span>and another photon arrives at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1813-Frame\"><span class=\"MathJax_MathContainer\"><span>(x=1.00m,0,0)<\/span><\/span><\/span><span>\u00a0<\/span>at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1814-Frame\"><span class=\"MathJax_MathContainer\"><span>t=0<\/span><\/span><\/span><span>\u00a0<\/span>in the frame of ship A. (a) Find the coordinates and times of the two events as seen by an observer in frame B. (b) In which frame are the two events simultaneous and in which frame are they are not simultaneous?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793937391\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793937393\">\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-id1167793937395\">Same two observers as in the preceding exercises. A rod of length 1 m is laid out on the<span>\u00a0<\/span><em data-effect=\"italics\">x<\/em>-axis in the frame of B from origin to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1815-Frame\"><span class=\"MathJax_MathContainer\"><span>(x=1.00m,0,0).<\/span><\/span><\/span><span>\u00a0<\/span>What is the length of the rod observed by an observer in the frame of spaceship A?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793609489\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793609491\">\r\n\r\n83<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793609493\">An observer at origin of inertial frame S sees a flashbulb go off at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1816-Frame\"><span class=\"MathJax_MathContainer\"><span>x=150km,y=15.0km,<\/span><\/span><\/span><span>\u00a0<\/span>and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1817-Frame\"><span class=\"MathJax_MathContainer\"><span>z=1.00km<\/span><\/span><\/span><span>\u00a0<\/span>at time<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1818-Frame\"><span class=\"MathJax_MathContainer\"><span>t=4.5\u00d710\u22124s.<\/span><\/span><\/span>At what time and position in the S<span class=\"MathJax_MathML\" id=\"MathJax-Element-1819-Frame\"><span class=\"MathJax_MathContainer\"><span>\u2032<\/span><\/span><\/span><span>\u00a0<\/span>system did the flash occur, if S<span class=\"MathJax_MathML\" id=\"MathJax-Element-1820-Frame\"><span class=\"MathJax_MathContainer\"><span>\u2032<\/span><\/span><\/span><span>\u00a0<\/span>is moving along shared<span>\u00a0<\/span><em data-effect=\"italics\">x<\/em>-direction with S at a velocity<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1821-Frame\"><span class=\"MathJax_MathContainer\"><span>v=0.6c?<\/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-id1167793562268\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793562270\">\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-id1167793562272\">An observer sees two events<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1822-Frame\"><span class=\"MathJax_MathContainer\"><span>1.5\u00d710\u22128s<\/span><\/span><\/span><span>\u00a0<\/span>apart at a separation of 800 m. How fast must a second observer be moving relative to the first to see the two events occur simultaneously?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793770701\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793770704\">\r\n\r\n85<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793770706\">An observer standing by the railroad tracks sees two bolts of lightning strike the ends of a 500-m-long train simultaneously at the instant the middle of the train passes him at 50 m\/s. Use the Lorentz transformation to find the time between the lightning strikes as measured by a passenger seated in the middle of the train.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793282608\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793282610\">\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-id1167793282612\">Two astronomical events are observed from Earth to occur at a time of 1 s apart and a distance separation of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1823-Frame\"><span class=\"MathJax_MathContainer\"><span>1.5\u00d7109m\u00a0<\/span><\/span><\/span>from each other. (a) Determine whether separation of the two events is space like or time like. (b) State what this implies about whether it is consistent with special relativity for one event to have caused the other?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793570072\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793570074\">\r\n\r\n87<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793570076\">Two astronomical events are observed from Earth to occur at a time of 0.30 s apart and a distance separation of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1824-Frame\"><span class=\"MathJax_MathContainer\"><span>2.0\u00d7109m\u00a0<\/span><\/span><\/span>from each other. How fast must a spacecraft travel from the site of one event toward the other to make the events occur at the same time when measured in the frame of reference of the spacecraft?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793541239\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793541241\">\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-id1167793541243\">A spacecraft starts from being at rest at the origin and accelerates at a constant rate<span>\u00a0<\/span><em data-effect=\"italics\">g<\/em>, as seen from Earth, taken to be an inertial frame, until it reaches a speed of<span>\u00a0<\/span><em data-effect=\"italics\">c\/<\/em>2. (a) Show that the increment of proper time is related to the elapsed time in Earth\u2019s frame by:<\/p>\r\n\r\n<div class=\"unnumbered\" data-type=\"equation\" id=\"fs-id1167793541259\">\r\n<div class=\"MathJax_MathML\" id=\"MathJax-Element-1825-Frame\"><span class=\"MathJax_MathContainer\"><span>d\u03c4=1\u2212v2\/c2dt.<\/span><\/span><\/div>\r\n<\/div>\r\n<p id=\"fs-id1167793542713\">(b) Find an expression for the elapsed time to reach speed<span>\u00a0<\/span><em data-effect=\"italics\">c\/<\/em>2 as seen in Earth\u2019s frame. (c) Use the relationship in (a) to obtain a similar expression for the elapsed proper time to reach<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>\/2 as seen in the spacecraft, and determine the ratio of the time seen from Earth with that on the spacecraft to reach the final speed.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793377862\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793377865\">\r\n\r\n89<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793355655\">(a) All but the closest galaxies are receding from our own Milky Way Galaxy. If a galaxy<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1826-Frame\"><span class=\"MathJax_MathContainer\"><span>12.0\u00d7109ly<\/span><\/span><\/span><span>\u00a0<\/span>away is receding from us at 0.900<em data-effect=\"italics\">c<\/em>, at what velocity relative to us must we send an exploratory probe to approach the other galaxy at 0.990<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>as measured from that galaxy? (b) How long will it take the probe to reach the other galaxy as measured from Earth? You may assume that the velocity of the other galaxy remains constant. (c) How long will it then take for a radio signal to be beamed back? (All of this is possible in principle, but not practical.)<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794170763\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794170765\">\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-id1167794170767\">Suppose a spaceship heading straight toward the Earth at 0.750<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>can shoot a canister at 0.500<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>relative to the ship. (a) What is the velocity of the canister relative to Earth, if it is shot directly at Earth? (b) If it is shot directly away from Earth?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794170800\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793466382\">\r\n\r\n91<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793466384\">Repeat the preceding problem with the ship heading directly away from Earth.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793466404\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793466406\">\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-id1167793466408\">If a spaceship is approaching the Earth at 0.100<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>and a message capsule is sent toward it at 0.100<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>relative to Earth, what is the speed of the capsule relative to the ship?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793397968\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793397970\">\r\n\r\n93<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793397972\">(a) Suppose the speed of light were only 3000 m\/s. A jet fighter moving toward a target on the ground at 800 m\/s shoots bullets, each having a muzzle velocity of 1000 m\/s. What are the bullets\u2019 velocity relative to the target? (b) If the speed of light was this small, would you observe relativistic effects in everyday life? Discuss.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793397989\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793397991\">\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-id1167793397994\">If a galaxy moving away from the Earth has a speed of 1000 km\/s and emits 656 nm light characteristic of hydrogen (the most common element in the universe). (a) What wavelength would we observe on Earth? (b) What type of electromagnetic radiation is this? (c) Why is the speed of Earth in its orbit negligible here?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793887713\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793887715\">\r\n\r\n95<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793887717\">A space probe speeding towards the nearest star moves at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1827-Frame\"><span class=\"MathJax_MathContainer\"><span>0.250c<\/span><\/span><\/span><span>\u00a0<\/span>and sends radio information at a broadcast frequency of 1.00 GHz. What frequency is received on Earth?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793887738\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793887740\">\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-id1167793887742\">Near the center of our galaxy, hydrogen gas is moving directly away from us in its orbit about a black hole. We receive 1900 nm electromagnetic radiation and know that it was 1875 nm when emitted by the hydrogen gas. What is the speed of the gas?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793522406\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793522408\">\r\n\r\n97<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793522410\">(a) Calculate the speed of a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1828-Frame\"><span class=\"MathJax_MathContainer\"><span>1.00-\u03bcg<\/span><\/span><\/span><span>\u00a0<\/span>particle of dust that has the same momentum as a proton moving at 0.999<em data-effect=\"italics\">c<\/em>. (b) What does the small speed tell us about the mass of a proton compared to even a tiny amount of macroscopic matter?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793607675\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793607677\">\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-id1167793607679\">(a) Calculate<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1829-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>for a proton that has a momentum of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1830-Frame\"><span class=\"MathJax_MathContainer\"><span>1.00kg\u00b7m\/s.<\/span><\/span><\/span><span>\u00a0<\/span>(b) What is its speed? Such protons form a rare component of cosmic radiation with uncertain origins.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793619921\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793619923\">\r\n\r\n99<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793619925\">Show that the relativistic form of Newton\u2019s second law is (a)<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1831-Frame\"><span class=\"MathJax_MathContainer\"><span>F=mdudt1(1\u2212u2\/c2)3\/2;<\/span><\/span><\/span><span>\u00a0<\/span>(b) Find the force needed to accelerate a mass of 1 kg by 1<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1832-Frame\"><span class=\"MathJax_MathContainer\"><span>m\/s2<\/span><\/span><\/span><span>\u00a0<\/span>when it is traveling at a velocity of<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>\/2.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793316092\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793316094\">\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-id1167793316096\">A positron is an antimatter version of the electron, having exactly the same mass. When a positron and an electron meet, they annihilate, converting all of their mass into energy. (a) Find the energy released, assuming negligible kinetic energy before the annihilation. (b) If this energy is given to a proton in the form of kinetic energy, what is its velocity? (c) If this energy is given to another electron in the form of kinetic energy, what is its velocity?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793637706\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793637708\">\r\n\r\n101<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793637711\">What is the kinetic energy in MeV of a \u03c0-meson that lives<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1833-Frame\"><span class=\"MathJax_MathContainer\"><span>1.40\u00d710\u221216s<\/span><\/span><\/span><span>\u00a0<\/span>as measured in the laboratory, and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1834-Frame\"><span class=\"MathJax_MathContainer\"><span>0.840\u00d710\u221216s\u00a0<\/span><\/span><\/span>when at rest relative to an observer, given that its rest energy is 135 MeV?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793246023\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793246025\">\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-id1167793246027\">Find the kinetic energy in MeV of a neutron with a measured life span of 2065 s, given its rest energy is 939.6 MeV, and rest life span is 900s.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793358293\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793358296\">\r\n\r\n103<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793358298\">(a) Show that<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1835-Frame\"><span class=\"MathJax_MathContainer\"><span>(pc)2\/(mc2)2=\u03b32\u22121.<\/span><\/span><\/span><span>\u00a0<\/span>This means that at large velocities<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1836-Frame\"><span class=\"MathJax_MathContainer\"><span>pc&gt;&gt;mc2.<\/span><\/span><\/span><span>\u00a0<\/span>(b) Is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1837-Frame\"><span class=\"MathJax_MathContainer\"><span>E\u2248pc<\/span><\/span><\/span><span>\u00a0<\/span>when<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1838-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=30.0,<\/span><\/span><\/span><span>\u00a0<\/span>as for the astronaut discussed in the twin paradox?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793291622\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793291624\">\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-id1167793291627\">One cosmic ray neutron has a velocity of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1839-Frame\"><span class=\"MathJax_MathContainer\"><span>0.250c<\/span><\/span><\/span><span>\u00a0<\/span>relative to the Earth. (a) What is the neutron\u2019s total energy in MeV? (b) Find its momentum. (c) Is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1840-Frame\"><span class=\"MathJax_MathContainer\"><span>E\u2248pc<\/span><\/span><\/span><span>\u00a0<\/span>in this situation? Discuss in terms of the equation given in part (a) of the previous problem.<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793603774\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793603776\">\r\n\r\n105<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793603778\">What is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1841-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>for a proton having a mass energy of 938.3 MeV accelerated through an effective potential of 1.0 TV (teravolt)?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794054210\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794054212\">\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-id1167794054214\">(a) What is the effective accelerating potential for electrons at the Stanford Linear Accelerator, if<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1842-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=1.00\u00d7105<\/span><\/span><\/span><span>\u00a0<\/span>for them? (b) What is their total energy (nearly the same as kinetic in this case) in GeV?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793928520\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793928522\">\r\n\r\n107<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793928525\">(a) Using data from<span>\u00a0<\/span><a href=\"https:\/\/cnx.org\/contents\/af275420-6050-4707-995c-57b9cc13c358@11.1:f36a3dfd-5697-445b-a5e6-c0642ed88f6d#fs-id1165036086155\" data-page=\"1\">Potential Energy of a System<\/a>, find the mass destroyed when the energy in a barrel of crude oil is released. (b) Given these barrels contain 200 liters and assuming the density of crude oil is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1843-Frame\"><span class=\"MathJax_MathContainer\"><span>750kg\/m3,<\/span><\/span><\/span><span>\u00a0<\/span>what is the ratio of mass destroyed to original mass,<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1844-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394m\/m?<\/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-id1167793546877\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793546879\">\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-id1167793546881\">(a) Calculate the energy released by the destruction of 1.00 kg of mass. (b) How many kilograms could be lifted to a 10.0 km height by this amount of 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-id1167793500468\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793500470\">\r\n\r\n109<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793500472\">A Van de Graaff accelerator utilizes a 50.0 MV potential difference to accelerate charged particles such as protons. (a) What is the velocity of a proton accelerated by such a potential? (b) An electron?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793246774\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793246776\">\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-id1167793246778\">Suppose you use an average of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1845-Frame\"><span class=\"MathJax_MathContainer\"><span>500kW\u00b7h<\/span><\/span><\/span><span>\u00a0<\/span>of electric energy per month in your home. (a) How long would 1.00 g of mass converted to electric energy with an efficiency of 38.0% last you? (b) How many homes could be supplied at the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1846-Frame\"><span class=\"MathJax_MathContainer\"><span>500kW\u00b7h<\/span><\/span><\/span><span>\u00a0<\/span>per month rate for one year by the energy from the described mass conversion?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794095418\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167794095420\">\r\n\r\n111<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167794095423\">(a) A nuclear power plant converts energy from nuclear fission into electricity with an efficiency of 35.0%. How much mass is destroyed in one year to produce a continuous 1000 MW of electric power? (b) Do you think it would be possible to observe this mass loss if the total mass of the fuel is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1847-Frame\"><span class=\"MathJax_MathContainer\"><span>104kg?<\/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-id1167793498317\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793498320\">\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-id1167793498322\">Nuclear-powered rockets were researched for some years before safety concerns became paramount. (a) What fraction of a rocket\u2019s mass would have to be destroyed to get it into a low Earth orbit, neglecting the decrease in gravity? (Assume an orbital altitude of 250 km, and calculate both the kinetic energy (classical) and the gravitational potential energy needed.) (b) If the ship has a mass of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1848-Frame\"><span class=\"MathJax_MathContainer\"><span>1.00\u00d7105kg<\/span><\/span><\/span><span>\u00a0<\/span>(100 tons), what total yield nuclear explosion in tons of TNT is needed?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793584525\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793584527\">\r\n\r\n113<span class=\"os-divider\">.<span>\u00a0<\/span><\/span>\r\n<div class=\"os-problem-container\">\r\n<p id=\"fs-id1167793584529\">The sun produces energy at a rate of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1849-Frame\"><span class=\"MathJax_MathContainer\"><span>3.85\u00d71026<\/span><\/span><\/span><span>\u00a0<\/span>W by the fusion of hydrogen. About 0.7% of each kilogram of hydrogen goes into the energy generated by the Sun. (a) How many kilograms of hydrogen undergo fusion each second? (b) If the sun is 90.0% hydrogen and half of this can undergo fusion before the sun changes character, how long could it produce energy at its current rate? (c) How many kilograms of mass is the sun losing per second? (d) What fraction of its mass will it have lost in the time found in part (b)?<\/p>\r\n\r\n<\/div>\r\n<\/div>\r\n<\/section><\/div>\r\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793465275\"><section>\r\n<div data-type=\"problem\" id=\"fs-id1167793465277\">\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-id1167793465280\">Show that\u00a0<span class=\"MathJax_MathML\" id=\"MathJax-Element-1850-Frame\"><span class=\"MathJax_MathContainer\"><span>E2\u2212p2c2<\/span><\/span><\/span>for a particle is invariant under Lorentz transformations.<\/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>\r\n<\/div>\r\n<\/section><\/div>\r\n<\/section><\/div>\r\n<\/div>\r\n<\/div>","rendered":"<div class=\"os-glossary-container\">\n<h3 data-type=\"title\"><span class=\"os-text\">Key Terms<\/span><\/h3>\n<dl id=\"fs-id1167793938539\">\n<dt id=\"38518\">classical (Galilean) velocity addition<\/dt>\n<dd id=\"fs-id1167794142090\">method of adding velocities when<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1689-Frame\"><span class=\"MathJax_MathContainer\">v&lt;&lt;c;<\/span><\/span>\u00a0<\/span>velocities add like regular numbers in one-dimensional motion:<span> u=v+u\u2032,\u00a0<\/span>where<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is the velocity between two observers,<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>is the velocity of an object relative to one observer, and<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1691-Frame\"><span class=\"MathJax_MathContainer\">u\u2032<\/span><\/span>\u00a0<\/span>is the velocity relative to the other observer<\/dd>\n<\/dl>\n<dl id=\"fs-id1167793561609\">\n<dt id=\"53287\">event<\/dt>\n<dd id=\"fs-id1167793561614\">occurrence in space and time specified by its position and time coordinates (<em data-effect=\"italics\">x<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">y<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">z<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">t<\/em>) measured relative to a frame of reference<\/dd>\n<\/dl>\n<dl id=\"fs-id1167793984547\">\n<dt id=\"84790\">first postulate of special relativity<\/dt>\n<dd id=\"fs-id1167794139578\">laws of physics are the same in all inertial frames of reference<\/dd>\n<\/dl>\n<dl id=\"fs-id1167793787576\">\n<dt id=\"62803\">Galilean relativity<\/dt>\n<dd id=\"fs-id1167793261076\">if an observer measures a velocity in one frame of reference, and that frame of reference is moving with a velocity past a second reference frame, an observer in the second frame measures the original velocity as the vector sum of these velocities<\/dd>\n<\/dl>\n<dl id=\"fs-id1167793277651\">\n<dt id=\"96665\">Galilean transformation<\/dt>\n<dd id=\"fs-id1167793277656\">relation between position and time coordinates of the same events as seen in different reference frames, according to classical mechanics<\/dd>\n<\/dl>\n<dl id=\"fs-id1167793363172\">\n<dt id=\"8441\">inertial frame of reference<\/dt>\n<dd id=\"fs-id1167794142311\">reference frame in which a body at rest remains at rest and a body in motion moves at a constant speed in a straight line unless acted on by an outside force<\/dd>\n<\/dl>\n<dl id=\"fs-id1167794058670\">\n<dt id=\"62399\">length contraction<\/dt>\n<dd id=\"fs-id1167793692944\">decrease in observed length of an object from its proper length<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1692-Frame\"><span class=\"MathJax_MathContainer\">L0<\/span><\/span>\u00a0<\/span>to length<span>\u00a0<\/span><em data-effect=\"italics\">L<\/em><span>\u00a0<\/span>when its length is observed in a reference frame where it is traveling at speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><\/dd>\n<\/dl>\n<dl id=\"fs-id1167793277662\">\n<dt id=\"19632\">Lorentz transformation<\/dt>\n<dd id=\"fs-id1167793277667\">relation between position and time coordinates of the same events as seen in different reference frames, according to the special theory of relativity<\/dd>\n<\/dl>\n<dl id=\"fs-id1167793514956\">\n<dt id=\"3267\">Michelson-Morley experiment<\/dt>\n<dd id=\"fs-id1167793556786\">investigation performed in 1887 that showed that the speed of light in a vacuum is the same in all frames of reference from which it is viewed<\/dd>\n<\/dl>\n<dl id=\"fs-id1167793933707\">\n<dt id=\"65548\">proper length<\/dt>\n<dd id=\"fs-id1167793278452\">L0; the distance between two points measured by an observer who is at rest relative to both of the points; for example, earthbound observers measure proper length when measuring the distance between two points that are stationary relative to Earth<\/dd>\n<\/dl>\n<dl id=\"fs-id1167793409768\">\n<dt id=\"10222\">proper time<\/dt>\n<dd id=\"fs-id1167793433561\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1694-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394\u03c4<\/span><\/span><\/span><span>\u00a0<\/span>is the time interval measured by an observer who sees the beginning and end of the process that the time interval measures occur at the same location<\/dd>\n<\/dl>\n<dl id=\"fs-id1167794215993\">\n<dt id=\"16\">relativistic kinetic energy<\/dt>\n<dd id=\"fs-id1167794215998\">kinetic energy of an object moving at relativistic speeds<\/dd>\n<\/dl>\n<dl id=\"fs-id1167794041889\">\n<dt id=\"35073\">relativistic momentum<\/dt>\n<dd id=\"fs-id1167793887875\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1695-Frame\"><span class=\"MathJax_MathContainer\"><span>p\u2192,<\/span><\/span><\/span><span>\u00a0<\/span>the momentum of an object moving at relativistic velocity;<span> p\u2192=\u03b3mu\u2192<\/span><\/dd>\n<\/dl>\n<dl id=\"fs-id1167793583897\">\n<dt id=\"6785\">relativistic velocity addition<\/dt>\n<dd id=\"fs-id1167794293139\">method of adding velocities of an object moving at a relativistic speeds<\/dd>\n<\/dl>\n<dl id=\"fs-id1167794216002\">\n<dt id=\"70859\">rest energy<\/dt>\n<dd id=\"fs-id1167794216008\">energy stored in an object at rest:<span> E0=mc2<\/span><\/dd>\n<\/dl>\n<dl id=\"fs-id1167794137438\">\n<dt id=\"56141\">rest frame<\/dt>\n<dd id=\"fs-id1167793750803\">frame of reference in which the observer is at rest<\/dd>\n<\/dl>\n<dl id=\"fs-id1167793881872\">\n<dt id=\"2055\">rest mass<\/dt>\n<dd id=\"fs-id1167793510596\">mass of an object as measured by an observer at rest relative to the object<\/dd>\n<\/dl>\n<dl id=\"fs-id1167793241040\">\n<dt id=\"3561\">second postulate of special relativity<\/dt>\n<dd id=\"fs-id1167793383391\">light travels in a vacuum with the same speed<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>in any direction in all inertial frames<\/dd>\n<\/dl>\n<dl id=\"fs-id1167794207045\">\n<dt id=\"85691\">special theory of relativity<\/dt>\n<dd id=\"fs-id1167794188118\">theory that Albert Einstein proposed in 1905 that assumes all the laws of physics have the same form in every inertial frame of reference, and that the speed of light is the same within all inertial frames<\/dd>\n<\/dl>\n<dl id=\"fs-id1167794216029\">\n<dt id=\"86171\">speed of light<\/dt>\n<dd id=\"fs-id1167794216034\">ultimate speed limit for any particle having mass<\/dd>\n<\/dl>\n<dl id=\"fs-id1167794070887\">\n<dt id=\"48566\">time dilation<\/dt>\n<dd id=\"fs-id1167793924861\">lengthening of the time interval between two events when seen in a moving inertial frame rather than the rest frame of the events (in which the events occur at the same location)<\/dd>\n<\/dl>\n<dl id=\"fs-id1167794127467\">\n<dt id=\"93135\">total energy<\/dt>\n<dd id=\"fs-id1167794127472\">sum of all energies for a particle, including rest energy and kinetic energy, given for a particle of mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>and speed<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>by<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1698-Frame\"><span class=\"MathJax_MathContainer\">E=\u03b3mc2,<\/span><\/span>\u00a0where\u00a0<span class=\"MathJax_MathML\" id=\"MathJax-Element-1699-Frame\"><span class=\"MathJax_MathContainer\">\u03b3=11\u2212u2c2<\/span><\/span><\/span><\/dd>\n<\/dl>\n<dl id=\"fs-id1167793777605\">\n<dt id=\"85530\">world line<\/dt>\n<dd id=\"fs-id1167793777610\">path through space-time<\/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-id1172100944609\" class=\"key-equations\" data-depth=\"1\">\n<div class=\"os-table\">\n<table id=\"fs-id1172098602739\" class=\"unnumbered unstyled\" style=\"width: 667px;height: 431px\" summary=\"Table 2.1 Refractive Indices Relevant to the Eye *This is an average value. The actual index of refraction varies throughout the lens and is greatest in center of the lens.\" data-label=\"\">\n<tbody>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Time dilation<\/td>\n<td style=\"width: 478px;height: 17px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1700-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394t=\u0394\u03c41\u2212v2c2=\u03b3\u03c4<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Lorentz factor<\/td>\n<td style=\"width: 478px;height: 17px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1701-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=11\u2212v2c2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Length contraction<\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1702-Frame\"><span class=\"MathJax_MathContainer\"><span>L=L01\u2212v2c2=L0\u03b3<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Galilean transformation<\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1703-Frame\"><span class=\"MathJax_MathContainer\"><span>x=x\u2032+vt,y=y\u2032,z=z\u2032,t=t\u2032<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Lorentz transformation<\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1704-Frame\"><span class=\"MathJax_MathContainer\"><span>t=t\u2032+vx\u2032\/c21\u2212v2\/c2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1705-Frame\"><span class=\"MathJax_MathContainer\"><span>x=x\u2032+vt\u20321\u2212v2\/c2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1706-Frame\"><span class=\"MathJax_MathContainer\"><span>y=y\u2032<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1707-Frame\"><span class=\"MathJax_MathContainer\"><span>z=z\u2032<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 35px\">\n<td style=\"width: 189px;height: 35px\" data-align=\"left\">Inverse Lorentz transformation<\/td>\n<td style=\"width: 478px;height: 35px\" data-align=\"left\">t\u2032=t\u2212vx\/c21\u2212v2\/c2<\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1709-Frame\"><span class=\"MathJax_MathContainer\"><span>x\u2032=x\u2212vt1\u2212v2\/c2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1710-Frame\"><span class=\"MathJax_MathContainer\"><span>y\u2032=y<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\"><\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1711-Frame\"><span class=\"MathJax_MathContainer\"><span>z\u2032=z<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Space-time invariants<\/td>\n<td style=\"width: 478px;height: 17px\" data-align=\"left\">(\u0394s)2=(\u0394x)2+(\u0394y)2+(\u0394z)2\u2212c2(\u0394t)2<\/td>\n<\/tr>\n<tr style=\"height: 35px\">\n<td style=\"width: 189px;height: 35px\" data-align=\"left\"><\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1713-Frame\"><span class=\"MathJax_MathContainer\"><span>(\u0394\u03c4)2=\u2212(\u0394s)2\/c2=(\u0394t)2\u2212[(\u0394x)2+(\u0394y)2+(\u0394z)2]c2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 35px\">\n<td style=\"width: 189px;height: 35px\" data-align=\"left\">Relativistic velocity addition<\/td>\n<td style=\"width: 478px;height: 35px\" data-align=\"left\">ux=(ux\u2032+v1+vux\u2032\/c2),uy=(uy\u2032\/\u03b31+vux\u2032\/c2),uz=(uz\u2032\/\u03b31+vux\u2032\/c2)<\/td>\n<\/tr>\n<tr style=\"height: 35px\">\n<td style=\"width: 189px;height: 35px\" data-align=\"left\">Relativistic Doppler effect for wavelength<\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1715-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03bbobs=\u03bbs1+vc1\u2212vc<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 35px\">\n<td style=\"width: 189px;height: 35px\" data-align=\"left\">Relativistic Doppler effect for frequency<\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1716-Frame\"><span class=\"MathJax_MathContainer\"><span>fobs=fs1\u2212vc1+vc<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 18px\">\n<td style=\"width: 189px;height: 18px\" data-align=\"left\">Relativistic momentum<\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1717-Frame\"><span class=\"MathJax_MathContainer\"><span>p\u2192=\u03b3mu\u2192=mu\u21921\u2212u2c<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Relativistic total energy<\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1718-Frame\"><span class=\"MathJax_MathContainer\"><span>E=\u03b3mc2,where\u03b3=11\u2212u2c2<\/span><\/span><\/span><\/td>\n<\/tr>\n<tr style=\"height: 17px\">\n<td style=\"width: 189px;height: 17px\" data-align=\"left\">Relativistic kinetic energy<\/td>\n<td style=\"width: 478px\" data-align=\"left\"><span class=\"MathJax_MathML\" id=\"MathJax-Element-1719-Frame\"><span class=\"MathJax_MathContainer\"><span>Krel=(\u03b3\u22121)mc2,where\u03b3=11\u2212u2c2<\/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-id1167793568935\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"28720_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-1-invariance-of-physical-laws\/\"><span class=\"os-number\">1.1<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Invariance of Physical Laws<\/span><\/a><\/h4>\n<ul id=\"fs-id1167793912156\" data-bullet-style=\"bullet\">\n<li>Relativity is the study of how observers in different reference frames measure the same event.<\/li>\n<li>Modern relativity is divided into two parts. Special relativity deals with observers in uniform (unaccelerated) motion, whereas general relativity includes accelerated relative motion and gravity. Modern relativity is consistent with all empirical evidence thus far and, in the limit of low velocity and weak gravitation, gives close agreement with the predictions of classical (Galilean) relativity.<\/li>\n<li>An inertial frame of reference is a reference frame in which a body at rest remains at rest and a body in motion moves at a constant speed in a straight line unless acted upon by an outside force.<\/li>\n<li>Modern relativity is based on Einstein\u2019s two postulates. The first postulate of special relativity is that the laws of physics are the same in all inertial frames of reference. The second postulate of special relativity is that the speed of light<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>is the same in all inertial frames of reference, independent of the relative motion of the observer and the light source.<\/li>\n<li>The Michelson-Morley experiment demonstrated that the speed of light in a vacuum is independent of the motion of Earth about the sun.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167794052056\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"41148_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-2-relativity-of-simultaneity\/\"><span class=\"os-number\">1.2<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativity of Simultaneity<\/span><\/a><\/h4>\n<ul id=\"fs-id1167794071141\" data-bullet-style=\"bullet\">\n<li>Two events are defined to be simultaneous if an observer measures them as occurring at the same time (such as by receiving light from the events).<\/li>\n<li>Two events at locations a distance apart that are simultaneous for an observer at rest in one frame of reference are not necessarily simultaneous for an observer at rest in a different frame of reference.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167794159499\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"16808_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-3-time-dilation\/\"><span class=\"os-number\">1.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Time Dilation<\/span><\/a><\/h4>\n<ul id=\"fs-id1167793473277\" data-bullet-style=\"bullet\">\n<li>Two events are defined to be simultaneous if an observer measures them as occurring at the same time. They are not necessarily simultaneous to all observers\u2014simultaneity is not absolute.<\/li>\n<li>Time dilation is the lengthening of the time interval between two events when seen in a moving inertial frame rather than the rest frame of the events (in which the events occur at the same location).<\/li>\n<li>Observers moving at a relative velocity<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>do not measure the same elapsed time between two events. Proper time<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1720-Frame\"><span class=\"MathJax_MathContainer\">\u0394\u03c4<\/span><\/span>\u00a0<\/span>is the time measured in the reference frame where the start and end of the time interval occur at the same location. The time interval<span> \u0394t<\/span><span>\u00a0<\/span>measured by an observer who sees the frame of events moving at speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is related to the proper time interval<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1722-Frame\"><span class=\"MathJax_MathContainer\">\u0394\u03c4<\/span><\/span>\u00a0<\/span>of the events by the equation:<span data-type=\"newline\"><br \/>\n<\/span><\/p>\n<div class=\"unnumbered\" data-label=\"\" data-type=\"equation\" id=\"fs-id1167794210772\">\n<div class=\"MathJax_Display\">\u0394t=\u0394\u03c41\u2212v2c2=\u03b3\u0394\u03c4,<\/div>\n<\/div>\n<p>where<span data-type=\"newline\"><br \/>\n<\/span><\/p>\n<div class=\"unnumbered\" data-label=\"\" data-type=\"equation\" id=\"fs-id1167794139375\">\n<div class=\"MathJax_Display\">\u03b3=11\u2212v2c2.<\/div>\n<\/div>\n<\/li>\n<li>The premise of the twin paradox is faulty because the traveling twin is accelerating. The journey is not symmetrical for the two twins.<\/li>\n<li>Time dilation is usually negligible at low relative velocities, but it does occur, and it has been verified by experiment.<\/li>\n<li>The proper time is the shortest measure of any time interval. Any observer who is moving relative to the system being observed measures a time interval longer than the proper time.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167793466427\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"55108_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-4-length-contraction\/\"><span class=\"os-number\">1.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Length Contraction<\/span><\/a><\/h4>\n<ul id=\"fs-id1167793301194\" data-bullet-style=\"bullet\">\n<li>All observers agree upon relative speed.<\/li>\n<li>Distance depends on an observer\u2019s motion. Proper length<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1725-Frame\"><span class=\"MathJax_MathContainer\">L0<\/span><\/span>\u00a0<\/span>is the distance between two points measured by an observer who is at rest relative to both of the points.<\/li>\n<li>Length contraction is the decrease in observed length of an object from its proper length<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1725-Frame\"><span class=\"MathJax_MathContainer\">L0<\/span><\/span>\u00a0<\/span>to length<span>\u00a0<\/span><em data-effect=\"italics\">L<\/em><span>\u00a0<\/span>when its length is observed in a reference frame where it is traveling at speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em>.<\/li>\n<li>The proper length is the longest measurement of any length interval. Any observer who is moving relative to the system being observed measures a length shorter than the proper length.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167793547990\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"1528_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-5-the-lorentz-transformation\/\"><span class=\"os-number\">1.5<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">The Lorentz Transformation<\/span><\/a><\/h4>\n<ul id=\"fs-id1167793547997\" data-bullet-style=\"bullet\">\n<li>The Galilean transformation equations describe how, in classical nonrelativistic mechanics, the position, velocity, and accelerations measured in one frame appear in another. Lengths remain unchanged and a single universal time scale is assumed to apply to all inertial frames.<\/li>\n<li>Newton\u2019s laws of mechanics obey the principle of having the same form in all inertial frames under a Galilean transformation, given by<span data-type=\"newline\"><br \/>\n<\/span><\/p>\n<div class=\"unnumbered\" data-label=\"\" data-type=\"equation\" id=\"fs-id1167793384555\">\n<div class=\"MathJax_Display\">x=x\u2032+vt,y=y\u2032,z=z\u2032,t=t\u2032.<\/div>\n<\/div>\n<p>The concept that times and distances are the same in all inertial frames in the Galilean transformation, however, is inconsistent with the postulates of special relativity.<\/li>\n<\/ul>\n<p>The relativistically correct Lorentz transformation equations are<span data-type=\"newline\"><br \/>\n<\/span><\/p>\n<div class=\"unnumbered\" data-label=\"\" data-type=\"equation\" id=\"fs-id1167793831535\">\n<div class=\"MathJax_Display\">\n<p>Lorentz transformation<br \/>\n<span data-type=\"newline\">t=t\u2032+vx\u2032\/c21\u2212v2\/c2<br \/>\nx=x\u2032+vt\u20321\u2212v2\/c2<br \/>\ny=y\u2032<br \/>\nz=z\u2032<\/span><\/p>\n<p>Inverse Lorentz transformation<br \/>\n<span style=\"font-size: 14pt\">t\u2032=t\u2212vx\/c21\u2212v2\/c2<br \/>\n<\/span><span style=\"font-size: 14pt\">x\u2032=x\u2212vt1\u2212v2\/c2<br \/>\n<span data-type=\"newline\">y\u2032=y<br \/>\nz\u2032=z<\/span><br \/>\n<\/span><\/p>\n<\/div>\n<\/div>\n<p><span data-type=\"newline\"><br \/>\n<\/span>We can obtain these equations by requiring an expanding spherical light signal to have the same shape and speed of growth,<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>, in both reference frames.<\/p>\n<ul id=\"fs-id1167793547997\" data-bullet-style=\"bullet\">\n<li>Relativistic phenomena can be explained in terms of the geometrical properties of four-dimensional space-time, in which Lorentz transformations correspond to rotations of axes.<\/li>\n<li>The Lorentz transformation corresponds to a space-time axis rotation, similar in some ways to a rotation of space axes, but in which the invariant spatial separation is given by<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1729-Frame\"><span class=\"MathJax_MathContainer\">\u0394s<\/span><\/span>\u00a0<\/span>rather than distances<span> \u0394r,\u00a0<\/span>and that the Lorentz transformation involving the time axis does not preserve perpendicularity of axes or the scales along the axes.<\/li>\n<li>The analysis of relativistic phenomena in terms of space-time diagrams supports the conclusion that these phenomena result from properties of space and time itself, rather than from the laws of electromagnetism.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167793499870\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"75851_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-6-relativistic-velocity-transformation\/\"><span class=\"os-number\">1.6<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Velocity Transformation<\/span><\/a><\/h4>\n<ul id=\"fs-id1167794051357\" data-bullet-style=\"bullet\">\n<li>With classical velocity addition, velocities add like regular numbers in one-dimensional motion:<span> u=v+u\u2032,<\/span><span>\u00a0<\/span>where<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is the velocity between two observers,<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>is the velocity of an object relative to one observer, and<span> u\u2032<\/span><span>\u00a0<\/span>is the velocity relative to the other observer.<\/li>\n<li>Velocities cannot add to be greater than the speed of light.<\/li>\n<li>Relativistic velocity addition describes the velocities of an object moving at a relativistic velocity.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167794296163\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"36417_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-7-doppler-effect-for-light\/\"><span class=\"os-number\">1.7<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Doppler Effect for Light<\/span><\/a><\/h4>\n<ul id=\"fs-id1167793960641\" data-bullet-style=\"bullet\">\n<li>An observer of electromagnetic radiation sees relativistic Doppler effects if the source of the radiation is moving relative to the observer. The wavelength of the radiation is longer (called a red shift) than that emitted by the source when the source moves away from the observer and shorter (called a blue shift) when the source moves toward the observer. The shifted wavelength is described by the equation:<span data-type=\"newline\"><br \/>\n<\/span><\/p>\n<div class=\"unnumbered\" data-label=\"\" data-type=\"equation\" id=\"fs-id1167794330470\">\n<div class=\"MathJax_Display\">\u03bbobs=\u03bbs1+vc1\u2212vc.<\/div>\n<\/div>\n<p>where<span> \u03bbobs\u00a0<\/span>is the observed wavelength,<span> \u03bbs<\/span><span>\u00a0<\/span>is the source wavelength, and<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is the relative velocity of the source to the observer.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167794051790\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"68539_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-8-relativistic-momentum\/\"><span class=\"os-number\">1.8<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Momentum<\/span><\/a><\/h4>\n<ul id=\"fs-id1167793976155\" data-bullet-style=\"bullet\">\n<li>The law of conservation of momentum is valid for relativistic momentum whenever the net external force is zero. The relativistic momentum is<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1736-Frame\"><span class=\"MathJax_MathContainer\">p=\u03b3mu,<\/span><\/span>\u00a0<\/span>where<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>is the rest mass of the object,<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>is its velocity relative to an observer, and the relativistic factor is<span> \u03b3=11\u2212u2c2.<\/span><\/li>\n<li>At low velocities, relativistic momentum is equivalent to classical momentum.<\/li>\n<li>Relativistic momentum approaches infinity as<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>approaches<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>. This implies that an object with mass cannot reach the speed of light.<\/li>\n<\/ul>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167794314613\" class=\"key-concepts\" data-depth=\"1\">\n<h4 id=\"57975_copy_1\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-9-relativistic-energy\/\"><span class=\"os-number\">1.9<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Energy<\/span><\/a><\/h4>\n<ul id=\"fs-id1167794314620\" data-bullet-style=\"bullet\">\n<li>The relativistic work-energy theorem is<span> Wnet=E\u2212E0=\u03b3mc2\u2212mc2=(\u03b3\u22121)mc2.<\/span><\/li>\n<li>Relativistically,<span> Wnet=Krel\u00a0<\/span>where<span> Krel\u00a0<\/span>is the relativistic kinetic energy.<\/li>\n<li>An object of<span>\u00a0<\/span><em data-effect=\"italics\">mass<\/em><span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>at velocity<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>has kinetic energy<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1741-Frame\"><span class=\"MathJax_MathContainer\">Krel=(\u03b3\u22121)mc2,<\/span><\/span>\u00a0where\u00a0<span class=\"MathJax_MathML\" id=\"MathJax-Element-1742-Frame\"><span class=\"MathJax_MathContainer\">\u03b3=11\u2212u2c2.<\/span><\/span><\/span><\/li>\n<li>At low velocities, relativistic kinetic energy reduces to classical kinetic energy.<\/li>\n<li>No object with mass can attain the speed of light, because an infinite amount of work and an infinite amount of energy input is required to accelerate a mass to the speed of light.<\/li>\n<li>Relativistic energy is conserved as long as we define it to include the possibility of mass changing to energy.<\/li>\n<li>The total energy of a particle with mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>traveling at speed<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>is defined as<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1743-Frame\"><span class=\"MathJax_MathContainer\">E=\u03b3mc2,<\/span><\/span>\u00a0<\/span>where\u00a0<span class=\"MathJax_MathML\" id=\"MathJax-Element-1744-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=11\u2212u2c2<\/span><\/span><\/span><span>\u00a0a<\/span>nd<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>denotes the velocity of the particle.<\/li>\n<li>The rest energy of an object of mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>is<span> E0=mc2,\u00a0<\/span>meaning that mass is a form of energy. If energy is stored in an object, its mass increases. Mass can be destroyed to release energy.<\/li>\n<li>We do not ordinarily notice the increase or decrease in mass of an object because the change in mass is so small for a large increase in energy. The equation<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1746-Frame\"><span class=\"MathJax_MathContainer\">E2=(pc)2+(mc2)2<\/span><\/span>\u00a0<\/span><span>\u00a0<\/span>relates the relativistic total energy<span>\u00a0<\/span><em data-effect=\"italics\">E<\/em><span>\u00a0<\/span>and the relativistic momentum<span>\u00a0<\/span><em data-effect=\"italics\">p<\/em>. At extremely high velocities, the rest energy<span> mc2<\/span><span>\u00a0<\/span>becomes negligible, and<span> E=pc.<\/span><\/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-id1167793269073\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"28720_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-1-invariance-of-physical-laws\/\"><span class=\"os-number\">1.1<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Invariance of Physical Laws<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793869864\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793953460\">\n<p>1<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793640552\">Which of Einstein\u2019s postulates of special relativity includes a concept that does not fit with the ideas of classical physics? Explain.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793499879\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794101041\">\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-id1167793927571\">Is Earth an inertial frame of reference? Is the sun? Justify your response.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794003397\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794334344\">\n<p>3<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794023568\">When you are flying in a commercial jet, it may appear to you that the airplane is stationary and Earth is moving beneath you. Is this point of view valid? Discuss briefly.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167794175883\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"16808_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-3-time-dilation\/\"><span class=\"os-number\">1.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Time Dilation<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793376295\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793395185\">\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-id1167793887481\">(a) Does motion affect the rate of a clock as measured by an observer moving with it? (b) Does motion affect how an observer moving relative to a clock measures its rate?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794325147\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793945117\">\n<p>5<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793558006\">To whom does the elapsed time for a process seem to be longer, an observer moving relative to the process or an observer moving with the process? Which observer measures the interval of proper time?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793262959\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793624997\">\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-id1167793220373\">(a) How could you travel far into the future of Earth without aging significantly? (b) Could this method also allow you to travel into the past?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167793299668\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"55108_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-4-length-contraction\/\"><span class=\"os-number\">1.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Length Contraction<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793362235\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793362237\">\n<p>7<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793280699\">To whom does an object seem greater in length, an observer moving with the object or an observer moving relative to the object? Which observer measures the object\u2019s proper length?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794090542\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793926426\">\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-id1167793926428\">Relativistic effects such as time dilation and length contraction are present for cars and airplanes. Why do these effects seem strange to us?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793441636\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793441638\">\n<p>9<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794296704\">Suppose an astronaut is moving relative to Earth at a significant fraction of the speed of light. (a) Does he observe the rate of his clocks to have slowed? (b) What change in the rate of earthbound clocks does he see? (c) Does his ship seem to him to shorten? (d) What about the distance between two stars that lie in the direction of his motion? (e) Do he and an earthbound observer agree on his velocity relative to Earth?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167793238016\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"36417_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-7-doppler-effect-for-light\/\"><span class=\"os-number\">1.7<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Doppler Effect for Light<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794329262\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793896608\">\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-id1167793989777\">Explain the meaning of the terms \u201cred shift\u201d and \u201cblue shift\u201d as they relate to the relativistic Doppler effect.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793787639\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794188024\">\n<p>11<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793251224\">What happens to the relativistic Doppler effect when relative velocity is zero? Is this the expected result?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794100180\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793877466\">\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-id1167793895380\">Is the relativistic Doppler effect consistent with the classical Doppler effect in the respect that<span> \u03bbobs<\/span><span>\u00a0<\/span>is larger for motion away?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793591205\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794069449\">\n<p>13<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794022158\">All galaxies farther away than about<span> <span class=\"MathJax_MathML\" id=\"MathJax-Element-1750-Frame\"><span class=\"MathJax_MathContainer\">50\u00d7106ly<\/span><\/span>\u00a0<\/span>exhibit a red shift in their emitted light that is proportional to distance, with those farther and farther away having progressively greater red shifts. What does this imply, assuming that the only source of red shift is relative motion?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167793435694\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"68539_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-8-relativistic-momentum\/\"><span class=\"os-number\">1.8<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Momentum<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793629296\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793237831\">\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-id1167793938240\">How does modern relativity modify the law of conservation of momentum?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794326162\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793985685\">\n<p>15<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794210766\">Is it possible for an external force to be acting on a system and relativistic momentum to be conserved? Explain.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167794032273\" class=\"review-conceptual-questions\" data-depth=\"1\">\n<h4 id=\"57975_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-9-relativistic-energy\/\"><span class=\"os-number\">1.9<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Energy<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794032281\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794032283\">\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-id1167794032285\">How are the classical laws of conservation of energy and conservation of mass modified by modern relativity?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793788572\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793788574\">\n<p>17<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793788576\">What happens to the mass of water in a pot when it cools, assuming no molecules escape or are added? Is this observable in practice? Explain.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793495017\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793495020\">\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-id1167793495022\">Consider a thought experiment. You place an expanded balloon of air on weighing scales outside in the early morning. The balloon stays on the scales and you are able to measure changes in its mass. Does the mass of the balloon change as the day progresses? Discuss the difficulties in carrying out this experiment.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793638889\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793638891\">\n<p>19<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793638893\">The mass of the fuel in a nuclear reactor decreases by an observable amount as it puts out energy. Is the same true for the coal and oxygen combined in a conventional power plant? If so, is this observable in practice for the coal and oxygen? Explain.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794296573\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794296575\">\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-id1167794296577\">We know that the velocity of an object with mass has an upper limit of<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>. Is there an upper limit on its momentum? Its energy? Explain.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793633482\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793633484\">\n<p>21<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793633486\">Given the fact that light travels at<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>, can it have mass? Explain.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794097177\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794097180\">\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-id1167794097182\">If you use an Earth-based telescope to project a laser beam onto the moon, you can move the spot across the moon\u2019s surface at a velocity greater than the speed of light. Does this violate modern relativity? (Note that light is being sent from the Earth to the moon, not across the surface of the moon.)<\/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-id1167793603932\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"16808_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-3-time-dilation\/\"><span class=\"os-number\">1.3<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Time Dilation<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793862957\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794051776\">\n<p>23<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793355328\">(a) <span>What is\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1751-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0if\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1752-Frame\"><span class=\"MathJax_MathContainer\"><span>v=0.250c?<\/span><\/span><\/span><span>\u00a0(b) If\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1753-Frame\"><span class=\"MathJax_MathContainer\"><span>v=0.500c?<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793379179\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794146271\">\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-id1167793928666\"><span>(a) What is\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1754-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0if\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1755-Frame\"><span class=\"MathJax_MathContainer\"><span>v=0.100c?<\/span><\/span><\/span><span>\u00a0(b) If\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1756-Frame\"><span class=\"MathJax_MathContainer\"><span>v=0.900c?<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793442208\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794327628\">\n<p>25<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794327630\"><span>Particles called\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1757-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c0<\/span><\/span><\/span><span>-mesons are produced by accelerator beams. If these particles travel at\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1758-Frame\"><span class=\"MathJax_MathContainer\"><span>2.70\u00d7108m\/s<\/span><\/span><\/span><span>\u00a0and live\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1759-Frame\"><span class=\"MathJax_MathContainer\"><span>2.60\u00d710\u22128s\u00a0<\/span><\/span><\/span><span>when at rest relative to an observer, how long do they live as viewed in the laboratory?<\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793516837\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793516839\">\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-id1167794097955\"><span>Suppose a particle called a kaon is created by cosmic radiation striking the atmosphere. It moves by you at\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1760-Frame\"><span class=\"MathJax_MathContainer\"><span>0.980c,<\/span><\/span><\/span><span>\u00a0and it lives\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1761-Frame\"><span class=\"MathJax_MathContainer\"><span>1.24\u00d710\u22128s<\/span><\/span><\/span><span>\u00a0when at rest relative to an observer. How long does it live as you observe it?<\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793401205\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793401207\">\n<p>27<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793418092\">A neutral<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1762-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c0<\/span><\/span><\/span>-meson is a particle that can be created by accelerator beams. If one such particle lives<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1763-Frame\"><span class=\"MathJax_MathContainer\"><span>1.40\u00d710\u221216s<\/span><\/span><\/span><span>\u00a0<\/span>as measured in the laboratory, and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1764-Frame\"><span class=\"MathJax_MathContainer\"><span>0.840\u00d710\u221216s<\/span><\/span><\/span><span>\u00a0<\/span>when at rest relative to an observer, what is its velocity relative to the laboratory?<\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793261501\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793261503\">\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-id1167793248364\"><span>A neutron lives 900 s when at rest relative to an observer. How fast is the neutron moving relative to an observer who measures its life span to be 2065 s?<\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793291690\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793291692\">\n<p>29<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span style=\"font-size: 14pt\">If relativistic effects are to be less than 1%, then<\/span><span style=\"font-size: 14pt\">\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1765-Frame\" style=\"font-size: 14pt\"><span class=\"MathJax_MathContainer\">\u03b3<\/span><\/span><span style=\"font-size: 14pt\">\u00a0<\/span><span style=\"font-size: 14pt\">must be less than 1.01. At what relative velocity is<\/span><span style=\"font-size: 14pt\">\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1766-Frame\" style=\"font-size: 14pt\"><span class=\"MathJax_MathContainer\">\u03b3=1.01?<\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793992264\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793992266\">\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-id1167793385868\"><span>If relativistic effects are to be less than 3%, then\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1767-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0must be less than 1.03. At what relative velocity is\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1768-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=1.03?<\/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-id1167794071932\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"55108_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-4-length-contraction\/\"><span class=\"os-number\">1.4<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Length Contraction<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793543353\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793268123\">\n<p>31<span class=\"os-divider\">.<span><\/span><\/span><\/p>\n<div class=\"os-review-problems-container\">\n<div class=\"os-review-problems\">\n<div class=\"os-section-area\">\n<section id=\"fs-id1167794071932\" class=\"review-problems\" data-depth=\"1\">\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793543353\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793268123\"><span style=\"font-size: 14pt\">A spaceship, 200 m long as seen on board, moves by the Earth at 0.970<\/span><em style=\"font-size: 14pt\" data-effect=\"italics\">c<\/em><span style=\"font-size: 14pt\">. What is its length as measured by an earthbound observer?<\/span><\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793638126\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793638128\">\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-id1167793638130\">How fast would a 6.0 m-long sports car have to be going past you in order for it to appear only 5.5 m long?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793377362\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793377364\">\n<p>33<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793377366\">(a) How far does the muon in<span>\u00a0<\/span>Example 1.3<span>\u00a0<\/span>travel according to the earthbound observer? (b) How far does it travel as viewed by an observer moving with it? Base your calculation on its velocity relative to the Earth and the time it lives (proper time). (c) Verify that these two distances are related through length contraction<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1769-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=3.20.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793432903\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793432905\">\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-id1167794095197\">(a) How long would the muon in<span>\u00a0<\/span>Example 1.3<span>\u00a0<\/span>have lived as observed on Earth if its velocity was<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1770-Frame\"><span class=\"MathJax_MathContainer\"><span>0.0500c?<\/span><\/span><\/span><span>\u00a0<\/span>(b) How far would it have traveled as observed on Earth? (c) What distance is this in the muon\u2019s frame?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793363299\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793363301\">\n<p>35<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793960774\"><strong data-effect=\"bold\">Unreasonable Results<\/strong><span>\u00a0<\/span>A spaceship is heading directly toward Earth at a velocity of 0.800<em data-effect=\"italics\">c<\/em>. The astronaut on board claims that he can send a canister toward the Earth at 1.20<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>relative to Earth. (a) Calculate the velocity the canister must have relative to the spaceship. (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167793362177\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"1528_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-5-the-lorentz-transformation\/\"><span class=\"os-number\">1.5<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">The Lorentz Transformation<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793362185\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793362187\">\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-id1167793362189\">Describe the following physical occurrences as events, that is, in the form (<em data-effect=\"italics\">x<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">y<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">z<\/em>,<span>\u00a0<\/span><em data-effect=\"italics\">t<\/em>): (a) A postman rings a doorbell of a house precisely at noon. (b) At the same time as the doorbell is rung, a slice of bread pops out of a toaster that is located 10 m from the door in the east direction from the door. (c) Ten seconds later, an airplane arrives at the airport, which is 10 km from the door in the east direction and 2 km to the south.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793506346\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793506348\">\n<p>37<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793506351\">Describe what happens to the angle<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1771-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b1=tan(v\/c),<\/span><\/span><\/span><span>\u00a0<\/span>and therefore to the transformed axes in<span>\u00a0<\/span>Figure 1.17, as the relative velocity<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>of the S and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1772-Frame\"><span class=\"MathJax_MathContainer\"><span>S\u2032<\/span><\/span><\/span><span>\u00a0<\/span>frames of reference approaches<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794336770\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794336772\">\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-id1167794336774\">Describe the shape of the world line on a space-time diagram of (a) an object that remains at rest at a specific position along the<span>\u00a0<\/span><em data-effect=\"italics\">x-<\/em>axis; (b) an object that moves at constant velocity<span>\u00a0<\/span><em data-effect=\"italics\">u<\/em><span>\u00a0<\/span>in the<span>\u00a0<\/span><em data-effect=\"italics\">x-<\/em>direction; (c) an object that begins at rest and accelerates at a constant rate of in the positive<span>\u00a0<\/span><em data-effect=\"italics\">x-<\/em>direction.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793581706\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793581708\">\n<p>39<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793581710\">A man standing still at a train station watches two boys throwing a baseball in a moving train. Suppose the train is moving east with a constant speed of 20 m\/s and one of the boys throws the ball with a speed of 5 m\/s with respect to himself toward the other boy, who is 5 m west from him. What is the velocity of the ball as observed by the man on the station?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794137014\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794137016\">\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-id1167794137018\">When observed from the sun at a particular instant, Earth and Mars appear to move in opposite directions with speeds 108,000 km\/h and 86,871 km\/h, respectively. What is the speed of Mars at this instant when observed from Earth?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793510460\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793510462\">\n<p>41<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793510464\">A man is running on a straight road perpendicular to a train track and away from the track at a speed of 12 m\/s. The train is moving with a speed of 30 m\/s with respect to the track. What is the speed of the man with respect to a passenger sitting at rest in the train?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793510479\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793510481\">\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-id1167793510483\">A man is running on a straight road that makes<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1773-Frame\"><span class=\"MathJax_MathContainer\"><span>30\u00b0<\/span><\/span><\/span><span>\u00a0<\/span>with the train track. The man is running in the direction on the road that is away from the track at a speed of 12 m\/s. The train is moving with a speed of 30 m\/s with respect to the track. What is the speed of the man with respect to a passenger sitting at rest in the train?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793603752\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793603755\">\n<p>43<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793603757\">In a frame at rest with respect to the billiard table, a billiard ball of mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>moving with speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>strikes another billiard ball of mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>at rest. The first ball comes to rest after the collision while the second ball takes off with speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>in the original direction of the motion of the first ball. This shows that momentum is conserved in this frame. (a) Now, describe the same collision from the perspective of a frame that is moving with speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>in the direction of the motion of the first ball. (b) Is the momentum conserved in this frame?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794163815\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794163817\">\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-id1167794163819\">In a frame at rest with respect to the billiard table, two billiard balls of same mass<span>\u00a0<\/span><em data-effect=\"italics\">m<\/em><span>\u00a0<\/span>are moving toward each other with the same speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em>. After the collision, the two balls come to rest. (a) Show that momentum is conserved in this frame. (b) Now, describe the same collision from the perspective of a frame that is moving with speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>in the direction of the motion of the first ball. (c) Is the momentum conserved in this frame?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794160228\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794160231\">\n<p>45<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794160233\">In a frame S, two events are observed: event 1: a pion is created at rest at the origin and event 2: the pion disintegrates after time<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1774-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c4<\/span><\/span><\/span>. Another observer in a frame<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1775-Frame\"><span class=\"MathJax_MathContainer\"><span>S\u2032<\/span><\/span><\/span><span>\u00a0<\/span>is moving in the positive direction along the positive<span>\u00a0<\/span><em data-effect=\"italics\">x<\/em>-axis with a constant speed<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em>and observes the same two events in his frame. The origins of the two frames coincide at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1776-Frame\"><span class=\"MathJax_MathContainer\"><span>t=t\u2032=0.<\/span><\/span><\/span><span>\u00a0<\/span>(a) Find the positions and timings of these two events in the frame<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1777-Frame\"><span class=\"MathJax_MathContainer\"><span>S\u2032<\/span><\/span><\/span><span>\u00a0<\/span>(a) according to the Galilean transformation, and (b) according to the Lorentz transformation.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167793354906\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"75851_copy_2\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-6-relativistic-velocity-transformation\/\"><span class=\"os-number\">1.6<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Velocity Transformation<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793593202\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794065574\">\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-id1167794065576\">If two spaceships are heading directly toward each other at 0.800<em data-effect=\"italics\">c<\/em>, at what speed must a canister be shot from the first ship to approach the other at 0.999<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>as seen by the second ship?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793618179\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793618181\">\n<p>47<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793618183\">Two planets are on a collision course, heading directly toward each other at 0.250<em data-effect=\"italics\">c<\/em>. A spaceship sent from one planet approaches the second at 0.750<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>as seen by the second planet. What is the velocity of the ship relative to the first planet?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793462690\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793462692\">\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-id1167793503978\">When a missile is shot from one spaceship toward another, it leaves the first at 0.950<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>and approaches the other at 0.750<em data-effect=\"italics\">c<\/em>. What is the relative velocity of the two ships?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793450526\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793515300\">\n<p>49<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793515302\">What is the relative velocity of two spaceships if one fires a missile at the other at 0.750<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>and the other observes it to approach at 0.950<em data-effect=\"italics\">c<\/em>?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793371632\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793371634\">\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-id1167793371636\">Prove that for any relative velocity<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>between two observers, a beam of light sent from one to the other will approach at speed<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>(provided that<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is less than<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>, of course).<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793372830\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793372832\">\n<p>51<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794098950\">Show that for any relative velocity<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>between two observers, a beam of light projected by one directly away from the other will move away at the speed of light (provided that<span>\u00a0<\/span><em data-effect=\"italics\">v<\/em><span>\u00a0<\/span>is less than<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>, of course).<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167794125603\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"36417_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-7-doppler-effect-for-light\/\"><span class=\"os-number\">1.7<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Doppler Effect for Light<\/span><\/a><\/h4>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794028783\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794328906\">\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-id1167793662487\">A highway patrol officer uses a device that measures the speed of vehicles by bouncing radar off them and measuring the Doppler shift. The outgoing radar has a frequency of 100 GHz and the returning echo has a frequency 15.0 kHz higher. What is the velocity of the vehicle? Note that there are two Doppler shifts in echoes. Be certain not to round off until the end of the problem, because the effect is small.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-section-area\">\n<section id=\"fs-id1167793999292\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"68539_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-8-relativistic-momentum\/\"><span class=\"os-number\">1.8<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Momentum<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794170660\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793290850\">\n<p>53<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794027273\">Find the momentum of a helium nucleus having a mass of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1778-Frame\"><span class=\"MathJax_MathContainer\"><span>6.68\u00d710\u221227kg<\/span><\/span><\/span><span>\u00a0<\/span>that is moving at 0.200<em data-effect=\"italics\">c<\/em>.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793219303\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793442787\">\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-id1167794169326\">What is the momentum of an electron traveling at 0.980<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-id1167793931807\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794328891\">\n<p>55<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794284915\">(a) Find the momentum of a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1779-Frame\"><span class=\"MathJax_MathContainer\"><span>1.00\u00d7109-kg<\/span><\/span><\/span><span>\u00a0<\/span>asteroid heading towards Earth at 30.0 km\/s. (b) Find the ratio of this momentum to the classical momentum. (Hint: Use the approximation that<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1780-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=1+(1\/2)v2\/c2<\/span><\/span><\/span><span>\u00a0<\/span>at low velocities.)<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794039506\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793376189\">\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-id1167793495147\">(a) What is the momentum of a 2000-kg satellite orbiting at 4.00 km\/s? (b) Find the ratio of this momentum to the classical momentum. (Hint: Use the approximation that<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1781-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=1+(1\/2)v2\/c2<\/span><\/span><\/span><span>\u00a0<\/span>at low velocities.)<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794026700\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794071266\">\n<p>57<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793848355\">What is the velocity of an electron that has a momentum of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1782-Frame\"><span class=\"MathJax_MathContainer\"><span>3.04\u00d710\u221221kg\u00b7m\/s<\/span><\/span><\/span><span>\u00a0<\/span>? Note that you must calculate the velocity to at least four digits to see the difference from<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793933416\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794135652\">\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-id1167793637938\">Find the velocity of a proton that has a momentum of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1783-Frame\"><span class=\"MathJax_MathContainer\"><span>4.48\u00d710\u221219kg\u00b7m\/s.<\/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-id1167794181332\" class=\"review-problems\" data-depth=\"1\">\n<h4 id=\"57975_copy_3\" data-type=\"document-title\"><a href=\"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/chapter\/1-9-relativistic-energy\/\"><span class=\"os-number\">1.9<\/span><span class=\"os-divider\"><span>\u00a0<\/span><\/span><span class=\"os-text\">Relativistic Energy<\/span><\/a><\/h4>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794181339\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794181341\">\n<p>59<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794181343\">What is the rest energy of an electron, given its mass is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1784-Frame\"><span class=\"MathJax_MathContainer\"><span>9.11\u00d710\u221231kg?<\/span><\/span><\/span><span>\u00a0<\/span>Give your answer in joules and MeV.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793554163\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793554165\">\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-id1167793554167\">Find the rest energy in joules and MeV of a proton, given its mass is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1785-Frame\"><span class=\"MathJax_MathContainer\"><span>1.67\u00d710\u221227kg.<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793547214\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793372797\">\n<p>61<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793372799\">If the rest energies of a proton and a neutron (the two constituents of nuclei) are 938.3 and 939.6 MeV, respectively, what is the difference in their mass in kilograms?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793938876\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793938878\">\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-id1167793938880\">The Big Bang that began the universe is estimated to have released<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1786-Frame\"><span class=\"MathJax_MathContainer\"><span>1068J<\/span><\/span><\/span><span>\u00a0<\/span>of energy. How many stars could half this energy create, assuming the average star\u2019s mass is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1787-Frame\"><span class=\"MathJax_MathContainer\"><span>4.00\u00d71030kg<\/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-id1167793978530\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793978532\">\n<p>63<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793978534\">A supernova explosion of a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1788-Frame\"><span class=\"MathJax_MathContainer\"><span>2.00\u00d71031kg<\/span><\/span><\/span><span>\u00a0<\/span>star produces<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1789-Frame\"><span class=\"MathJax_MathContainer\"><span>1.00\u00d71044J<\/span><\/span><\/span><span>\u00a0<\/span>of energy. (a) How many kilograms of mass are converted to energy in the explosion? (b) What is the ratio<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1790-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394m\/m<\/span><\/span><\/span><span>\u00a0<\/span>of mass destroyed to the original mass of the star?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793384967\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793384969\">\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-id1167793384971\">(a) Using data from<span>\u00a0<\/span><a href=\"https:\/\/cnx.org\/contents\/af275420-6050-4707-995c-57b9cc13c358@11.1:f36a3dfd-5697-445b-a5e6-c0642ed88f6d#fs-id1165036086155\" data-page=\"1\">Potential Energy of a System<\/a>, calculate the mass converted to energy by the fission of 1.00 kg of uranium. (b) What is the ratio of mass destroyed to the original mass,<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1791-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394m\/m?<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793928250\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793928252\">\n<p>65<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793928254\">(a) Using data from<span>\u00a0<\/span><a href=\"https:\/\/cnx.org\/contents\/af275420-6050-4707-995c-57b9cc13c358@11.1:f36a3dfd-5697-445b-a5e6-c0642ed88f6d#fs-id1165036086155\" data-page=\"1\">Potential Energy of a System<\/a>, calculate the amount of mass converted to energy by the fusion of 1.00 kg of hydrogen. (b) What is the ratio of mass destroyed to the original mass,<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1792-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394m\/m<\/span><\/span><\/span><span>\u00a0<\/span>? (c) How does this compare with<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1793-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394m\/m\u00a0<\/span><\/span><\/span>for the fission of 1.00 kg of uranium?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794186600\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794186602\">\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-id1167794186604\">There is approximately<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1794-Frame\"><span class=\"MathJax_MathContainer\"><span>1034J<\/span><\/span><\/span><span>\u00a0<\/span>of energy available from fusion of hydrogen in the world\u2019s oceans. (a) If<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1795-Frame\"><span class=\"MathJax_MathContainer\"><span>1033J<\/span><\/span><\/span><span>\u00a0<\/span>of this energy were utilized, what would be the decrease in mass of the oceans? (b) How great a volume of water does this correspond to? (c) Comment on whether this is a significant fraction of the total mass of the oceans.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793371355\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793371357\">\n<p>67<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793371359\">A muon has a rest mass energy of 105.7 MeV, and it decays into an electron and a massless particle. (a) If all the lost mass is converted into the electron\u2019s kinetic energy, find<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1796-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>for the electron. (b) What is the electron\u2019s velocity?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793371384\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793371386\">\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-id1167793641954\">A<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1797-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c0<\/span><\/span><\/span>-meson is a particle that decays into a muon and a massless particle. The<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1798-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c0<\/span><\/span><\/span>-meson has a rest mass energy of 139.6 MeV, and the muon has a rest mass energy of 105.7 MeV. Suppose the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1799-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03c0<\/span><\/span><\/span>-meson is at rest and all of the missing mass goes into the muon\u2019s kinetic energy. How fast will the muon move?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793641984\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793641987\">\n<p>69<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793641989\">(a) Calculate the relativistic kinetic energy of a 1000-kg car moving at 30.0 m\/s if the speed of light were only 45.0 m\/s. (b) Find the ratio of the relativistic kinetic energy to classical.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793626891\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793626893\">\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-id1167793626895\">Alpha decay is nuclear decay in which a helium nucleus is emitted. If the helium nucleus has a mass of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1800-Frame\"><span class=\"MathJax_MathContainer\"><span>6.80\u00d710\u221227kg<\/span><\/span><\/span><span>\u00a0<\/span>and is given 5.00 MeV of kinetic energy, what is its velocity?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793605318\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793605320\">\n<p>71<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793605322\">(a) Beta decay is nuclear decay in which an electron is emitted. If the electron is given 0.750 MeV of kinetic energy, what is its velocity? (b) Comment on how the high velocity is consistent with the kinetic energy as it compares to the rest mass energy of the electron.<\/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-id1165039371212\" class=\"review-additional-problems\" data-depth=\"1\">\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793374981\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793374983\">\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-id1167793374986\">(a) At what relative velocity is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1801-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=1.50?<\/span><\/span><\/span><span>\u00a0<\/span>(b) At what relative velocity is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1802-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=100?<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793551988\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793551990\">\n<p>73<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793551992\">(a) At what relative velocity is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1803-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=2.00?<\/span><\/span><\/span><span>\u00a0<\/span>(b) At what relative velocity is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1804-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=10.0?<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793384944\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793384946\">\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-id1167793384949\"><strong data-effect=\"bold\">Unreasonable Results<\/strong><span>\u00a0<\/span>(a) Find the value of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1805-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>required for the following situation. An earthbound observer measures 23.9 h to have passed while signals from a high-velocity space probe indicate that 24.0 h have passed on board. (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793376212\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793376214\">\n<p>75<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793376216\">(a) How long does it take the astronaut in<span>\u00a0<\/span>Example 1.5<span>\u00a0<\/span>to travel 4.30 ly at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1806-Frame\"><span class=\"MathJax_MathContainer\"><span>0.99944c<\/span><\/span><\/span><span>\u00a0<\/span>(as measured by the earthbound observer)? (b) How long does it take according to the astronaut? (c) Verify that these two times are related through time dilation with<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1807-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=30.00<\/span><\/span><\/span><span>\u00a0<\/span>as given.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793599601\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793599603\">\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-id1167793599605\">(a) How fast would an athlete need to be running for a 100-<span class=\"MathJax_MathML\" id=\"MathJax-Element-1808-Frame\"><span class=\"MathJax_MathContainer\"><span>m<\/span><\/span><\/span><span>\u00a0<\/span>race to look 100 yd long? (b) Is the answer consistent with the fact that relativistic effects are difficult to observe in ordinary circumstances? Explain.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793219328\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793219331\">\n<p>77<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793219333\">(a) Find the value of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1809-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>for the following situation. An astronaut measures the length of his spaceship to be 100 m, while an earthbound observer measures it to be 25.0 m. (b) What is the speed of the spaceship relative to Earth?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793422000\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793422003\">\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-id1167793422005\">A clock in a spaceship runs one-tenth the rate at which an identical clock on Earth runs. What is the speed of the spaceship?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793422027\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794095442\">\n<p>79<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794095444\">An astronaut has a heartbeat rate of 66 beats per minute as measured during his physical exam on Earth. The heartbeat rate of the astronaut is measured when he is in a spaceship traveling at 0.5<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>with respect to Earth by an observer (A) in the ship and by an observer (B) on Earth. (a) Describe an experimental method by which observer B on Earth will be able to determine the heartbeat rate of the astronaut when the astronaut is in the spaceship. (b) What will be the heartbeat rate(s) of the astronaut reported by observers A and B?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794326142\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794326144\">\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-id1167794326147\">A spaceship (A) is moving at speed<span>\u00a0<\/span><em data-effect=\"italics\">c\/<\/em>2 with respect to another spaceship (B). Observers in A and B set their clocks so that the event at (<em data-effect=\"italics\">x, y, z, t<\/em>) of turning on a laser in spaceship B has coordinates (0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0) in A and also (0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0<em data-effect=\"italics\">,<\/em><span>\u00a0<\/span>0) in B. An observer at the origin of B turns on the laser at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1810-Frame\"><span class=\"MathJax_MathContainer\"><span>t=0<\/span><\/span><\/span><span>\u00a0<\/span>and turns it off at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1811-Frame\"><span class=\"MathJax_MathContainer\"><span>t=\u03c4<\/span><\/span><\/span><span>\u00a0<\/span>in his time. What is the time duration between on and off as seen by an observer in A?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793245244\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793245246\">\n<p>81<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793245248\">Same two observers as in the preceding exercise, but now we look at two events occurring in spaceship A. A photon arrives at the origin of A at its time<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1812-Frame\"><span class=\"MathJax_MathContainer\"><span>t=0<\/span><\/span><\/span><span>\u00a0<\/span>and another photon arrives at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1813-Frame\"><span class=\"MathJax_MathContainer\"><span>(x=1.00m,0,0)<\/span><\/span><\/span><span>\u00a0<\/span>at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1814-Frame\"><span class=\"MathJax_MathContainer\"><span>t=0<\/span><\/span><\/span><span>\u00a0<\/span>in the frame of ship A. (a) Find the coordinates and times of the two events as seen by an observer in frame B. (b) In which frame are the two events simultaneous and in which frame are they are not simultaneous?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793937391\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793937393\">\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-id1167793937395\">Same two observers as in the preceding exercises. A rod of length 1 m is laid out on the<span>\u00a0<\/span><em data-effect=\"italics\">x<\/em>-axis in the frame of B from origin to<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1815-Frame\"><span class=\"MathJax_MathContainer\"><span>(x=1.00m,0,0).<\/span><\/span><\/span><span>\u00a0<\/span>What is the length of the rod observed by an observer in the frame of spaceship A?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793609489\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793609491\">\n<p>83<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793609493\">An observer at origin of inertial frame S sees a flashbulb go off at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1816-Frame\"><span class=\"MathJax_MathContainer\"><span>x=150km,y=15.0km,<\/span><\/span><\/span><span>\u00a0<\/span>and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1817-Frame\"><span class=\"MathJax_MathContainer\"><span>z=1.00km<\/span><\/span><\/span><span>\u00a0<\/span>at time<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1818-Frame\"><span class=\"MathJax_MathContainer\"><span>t=4.5\u00d710\u22124s.<\/span><\/span><\/span>At what time and position in the S<span class=\"MathJax_MathML\" id=\"MathJax-Element-1819-Frame\"><span class=\"MathJax_MathContainer\"><span>\u2032<\/span><\/span><\/span><span>\u00a0<\/span>system did the flash occur, if S<span class=\"MathJax_MathML\" id=\"MathJax-Element-1820-Frame\"><span class=\"MathJax_MathContainer\"><span>\u2032<\/span><\/span><\/span><span>\u00a0<\/span>is moving along shared<span>\u00a0<\/span><em data-effect=\"italics\">x<\/em>-direction with S at a velocity<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1821-Frame\"><span class=\"MathJax_MathContainer\"><span>v=0.6c?<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793562268\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793562270\">\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-id1167793562272\">An observer sees two events<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1822-Frame\"><span class=\"MathJax_MathContainer\"><span>1.5\u00d710\u22128s<\/span><\/span><\/span><span>\u00a0<\/span>apart at a separation of 800 m. How fast must a second observer be moving relative to the first to see the two events occur simultaneously?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793770701\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793770704\">\n<p>85<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793770706\">An observer standing by the railroad tracks sees two bolts of lightning strike the ends of a 500-m-long train simultaneously at the instant the middle of the train passes him at 50 m\/s. Use the Lorentz transformation to find the time between the lightning strikes as measured by a passenger seated in the middle of the train.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793282608\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793282610\">\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-id1167793282612\">Two astronomical events are observed from Earth to occur at a time of 1 s apart and a distance separation of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1823-Frame\"><span class=\"MathJax_MathContainer\"><span>1.5\u00d7109m\u00a0<\/span><\/span><\/span>from each other. (a) Determine whether separation of the two events is space like or time like. (b) State what this implies about whether it is consistent with special relativity for one event to have caused the other?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793570072\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793570074\">\n<p>87<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793570076\">Two astronomical events are observed from Earth to occur at a time of 0.30 s apart and a distance separation of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1824-Frame\"><span class=\"MathJax_MathContainer\"><span>2.0\u00d7109m\u00a0<\/span><\/span><\/span>from each other. How fast must a spacecraft travel from the site of one event toward the other to make the events occur at the same time when measured in the frame of reference of the spacecraft?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793541239\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793541241\">\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-id1167793541243\">A spacecraft starts from being at rest at the origin and accelerates at a constant rate<span>\u00a0<\/span><em data-effect=\"italics\">g<\/em>, as seen from Earth, taken to be an inertial frame, until it reaches a speed of<span>\u00a0<\/span><em data-effect=\"italics\">c\/<\/em>2. (a) Show that the increment of proper time is related to the elapsed time in Earth\u2019s frame by:<\/p>\n<div class=\"unnumbered\" data-type=\"equation\" id=\"fs-id1167793541259\">\n<div class=\"MathJax_MathML\" id=\"MathJax-Element-1825-Frame\"><span class=\"MathJax_MathContainer\"><span>d\u03c4=1\u2212v2\/c2dt.<\/span><\/span><\/div>\n<\/div>\n<p id=\"fs-id1167793542713\">(b) Find an expression for the elapsed time to reach speed<span>\u00a0<\/span><em data-effect=\"italics\">c\/<\/em>2 as seen in Earth\u2019s frame. (c) Use the relationship in (a) to obtain a similar expression for the elapsed proper time to reach<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>\/2 as seen in the spacecraft, and determine the ratio of the time seen from Earth with that on the spacecraft to reach the final speed.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793377862\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793377865\">\n<p>89<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793355655\">(a) All but the closest galaxies are receding from our own Milky Way Galaxy. If a galaxy<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1826-Frame\"><span class=\"MathJax_MathContainer\"><span>12.0\u00d7109ly<\/span><\/span><\/span><span>\u00a0<\/span>away is receding from us at 0.900<em data-effect=\"italics\">c<\/em>, at what velocity relative to us must we send an exploratory probe to approach the other galaxy at 0.990<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>as measured from that galaxy? (b) How long will it take the probe to reach the other galaxy as measured from Earth? You may assume that the velocity of the other galaxy remains constant. (c) How long will it then take for a radio signal to be beamed back? (All of this is possible in principle, but not practical.)<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794170763\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794170765\">\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-id1167794170767\">Suppose a spaceship heading straight toward the Earth at 0.750<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>can shoot a canister at 0.500<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>relative to the ship. (a) What is the velocity of the canister relative to Earth, if it is shot directly at Earth? (b) If it is shot directly away from Earth?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794170800\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793466382\">\n<p>91<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793466384\">Repeat the preceding problem with the ship heading directly away from Earth.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793466404\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793466406\">\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-id1167793466408\">If a spaceship is approaching the Earth at 0.100<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>and a message capsule is sent toward it at 0.100<em data-effect=\"italics\">c<\/em><span>\u00a0<\/span>relative to Earth, what is the speed of the capsule relative to the ship?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793397968\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793397970\">\n<p>93<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793397972\">(a) Suppose the speed of light were only 3000 m\/s. A jet fighter moving toward a target on the ground at 800 m\/s shoots bullets, each having a muzzle velocity of 1000 m\/s. What are the bullets\u2019 velocity relative to the target? (b) If the speed of light was this small, would you observe relativistic effects in everyday life? Discuss.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793397989\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793397991\">\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-id1167793397994\">If a galaxy moving away from the Earth has a speed of 1000 km\/s and emits 656 nm light characteristic of hydrogen (the most common element in the universe). (a) What wavelength would we observe on Earth? (b) What type of electromagnetic radiation is this? (c) Why is the speed of Earth in its orbit negligible here?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793887713\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793887715\">\n<p>95<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793887717\">A space probe speeding towards the nearest star moves at<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1827-Frame\"><span class=\"MathJax_MathContainer\"><span>0.250c<\/span><\/span><\/span><span>\u00a0<\/span>and sends radio information at a broadcast frequency of 1.00 GHz. What frequency is received on Earth?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793887738\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793887740\">\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-id1167793887742\">Near the center of our galaxy, hydrogen gas is moving directly away from us in its orbit about a black hole. We receive 1900 nm electromagnetic radiation and know that it was 1875 nm when emitted by the hydrogen gas. What is the speed of the gas?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793522406\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793522408\">\n<p>97<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793522410\">(a) Calculate the speed of a<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1828-Frame\"><span class=\"MathJax_MathContainer\"><span>1.00-\u03bcg<\/span><\/span><\/span><span>\u00a0<\/span>particle of dust that has the same momentum as a proton moving at 0.999<em data-effect=\"italics\">c<\/em>. (b) What does the small speed tell us about the mass of a proton compared to even a tiny amount of macroscopic matter?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793607675\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793607677\">\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-id1167793607679\">(a) Calculate<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1829-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>for a proton that has a momentum of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1830-Frame\"><span class=\"MathJax_MathContainer\"><span>1.00kg\u00b7m\/s.<\/span><\/span><\/span><span>\u00a0<\/span>(b) What is its speed? Such protons form a rare component of cosmic radiation with uncertain origins.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793619921\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793619923\">\n<p>99<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793619925\">Show that the relativistic form of Newton\u2019s second law is (a)<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1831-Frame\"><span class=\"MathJax_MathContainer\"><span>F=mdudt1(1\u2212u2\/c2)3\/2;<\/span><\/span><\/span><span>\u00a0<\/span>(b) Find the force needed to accelerate a mass of 1 kg by 1<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1832-Frame\"><span class=\"MathJax_MathContainer\"><span>m\/s2<\/span><\/span><\/span><span>\u00a0<\/span>when it is traveling at a velocity of<span>\u00a0<\/span><em data-effect=\"italics\">c<\/em>\/2.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793316092\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793316094\">\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-id1167793316096\">A positron is an antimatter version of the electron, having exactly the same mass. When a positron and an electron meet, they annihilate, converting all of their mass into energy. (a) Find the energy released, assuming negligible kinetic energy before the annihilation. (b) If this energy is given to a proton in the form of kinetic energy, what is its velocity? (c) If this energy is given to another electron in the form of kinetic energy, what is its velocity?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793637706\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793637708\">\n<p>101<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793637711\">What is the kinetic energy in MeV of a \u03c0-meson that lives<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1833-Frame\"><span class=\"MathJax_MathContainer\"><span>1.40\u00d710\u221216s<\/span><\/span><\/span><span>\u00a0<\/span>as measured in the laboratory, and<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1834-Frame\"><span class=\"MathJax_MathContainer\"><span>0.840\u00d710\u221216s\u00a0<\/span><\/span><\/span>when at rest relative to an observer, given that its rest energy is 135 MeV?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793246023\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793246025\">\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-id1167793246027\">Find the kinetic energy in MeV of a neutron with a measured life span of 2065 s, given its rest energy is 939.6 MeV, and rest life span is 900s.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793358293\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793358296\">\n<p>103<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793358298\">(a) Show that<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1835-Frame\"><span class=\"MathJax_MathContainer\"><span>(pc)2\/(mc2)2=\u03b32\u22121.<\/span><\/span><\/span><span>\u00a0<\/span>This means that at large velocities<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1836-Frame\"><span class=\"MathJax_MathContainer\"><span>pc&gt;&gt;mc2.<\/span><\/span><\/span><span>\u00a0<\/span>(b) Is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1837-Frame\"><span class=\"MathJax_MathContainer\"><span>E\u2248pc<\/span><\/span><\/span><span>\u00a0<\/span>when<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1838-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=30.0,<\/span><\/span><\/span><span>\u00a0<\/span>as for the astronaut discussed in the twin paradox?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793291622\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793291624\">\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-id1167793291627\">One cosmic ray neutron has a velocity of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1839-Frame\"><span class=\"MathJax_MathContainer\"><span>0.250c<\/span><\/span><\/span><span>\u00a0<\/span>relative to the Earth. (a) What is the neutron\u2019s total energy in MeV? (b) Find its momentum. (c) Is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1840-Frame\"><span class=\"MathJax_MathContainer\"><span>E\u2248pc<\/span><\/span><\/span><span>\u00a0<\/span>in this situation? Discuss in terms of the equation given in part (a) of the previous problem.<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793603774\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793603776\">\n<p>105<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793603778\">What is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1841-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3<\/span><\/span><\/span><span>\u00a0<\/span>for a proton having a mass energy of 938.3 MeV accelerated through an effective potential of 1.0 TV (teravolt)?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167794054210\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794054212\">\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-id1167794054214\">(a) What is the effective accelerating potential for electrons at the Stanford Linear Accelerator, if<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1842-Frame\"><span class=\"MathJax_MathContainer\"><span>\u03b3=1.00\u00d7105<\/span><\/span><\/span><span>\u00a0<\/span>for them? (b) What is their total energy (nearly the same as kinetic in this case) in GeV?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793928520\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793928522\">\n<p>107<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793928525\">(a) Using data from<span>\u00a0<\/span><a href=\"https:\/\/cnx.org\/contents\/af275420-6050-4707-995c-57b9cc13c358@11.1:f36a3dfd-5697-445b-a5e6-c0642ed88f6d#fs-id1165036086155\" data-page=\"1\">Potential Energy of a System<\/a>, find the mass destroyed when the energy in a barrel of crude oil is released. (b) Given these barrels contain 200 liters and assuming the density of crude oil is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1843-Frame\"><span class=\"MathJax_MathContainer\"><span>750kg\/m3,<\/span><\/span><\/span><span>\u00a0<\/span>what is the ratio of mass destroyed to original mass,<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1844-Frame\"><span class=\"MathJax_MathContainer\"><span>\u0394m\/m?<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793546877\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793546879\">\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-id1167793546881\">(a) Calculate the energy released by the destruction of 1.00 kg of mass. (b) How many kilograms could be lifted to a 10.0 km height by this amount of energy?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793500468\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793500470\">\n<p>109<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793500472\">A Van de Graaff accelerator utilizes a 50.0 MV potential difference to accelerate charged particles such as protons. (a) What is the velocity of a proton accelerated by such a potential? (b) An electron?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793246774\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793246776\">\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-id1167793246778\">Suppose you use an average of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1845-Frame\"><span class=\"MathJax_MathContainer\"><span>500kW\u00b7h<\/span><\/span><\/span><span>\u00a0<\/span>of electric energy per month in your home. (a) How long would 1.00 g of mass converted to electric energy with an efficiency of 38.0% last you? (b) How many homes could be supplied at the<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1846-Frame\"><span class=\"MathJax_MathContainer\"><span>500kW\u00b7h<\/span><\/span><\/span><span>\u00a0<\/span>per month rate for one year by the energy from the described mass conversion?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167794095418\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167794095420\">\n<p>111<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167794095423\">(a) A nuclear power plant converts energy from nuclear fission into electricity with an efficiency of 35.0%. How much mass is destroyed in one year to produce a continuous 1000 MW of electric power? (b) Do you think it would be possible to observe this mass loss if the total mass of the fuel is<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1847-Frame\"><span class=\"MathJax_MathContainer\"><span>104kg?<\/span><\/span><\/span><\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793498317\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793498320\">\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-id1167793498322\">Nuclear-powered rockets were researched for some years before safety concerns became paramount. (a) What fraction of a rocket\u2019s mass would have to be destroyed to get it into a low Earth orbit, neglecting the decrease in gravity? (Assume an orbital altitude of 250 km, and calculate both the kinetic energy (classical) and the gravitational potential energy needed.) (b) If the ship has a mass of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1848-Frame\"><span class=\"MathJax_MathContainer\"><span>1.00\u00d7105kg<\/span><\/span><\/span><span>\u00a0<\/span>(100 tons), what total yield nuclear explosion in tons of TNT is needed?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"os-hasSolution\" data-type=\"exercise\" id=\"fs-id1167793584525\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793584527\">\n<p>113<span class=\"os-divider\">.<span>\u00a0<\/span><\/span><\/p>\n<div class=\"os-problem-container\">\n<p id=\"fs-id1167793584529\">The sun produces energy at a rate of<span>\u00a0<\/span><span class=\"MathJax_MathML\" id=\"MathJax-Element-1849-Frame\"><span class=\"MathJax_MathContainer\"><span>3.85\u00d71026<\/span><\/span><\/span><span>\u00a0<\/span>W by the fusion of hydrogen. About 0.7% of each kilogram of hydrogen goes into the energy generated by the Sun. (a) How many kilograms of hydrogen undergo fusion each second? (b) If the sun is 90.0% hydrogen and half of this can undergo fusion before the sun changes character, how long could it produce energy at its current rate? (c) How many kilograms of mass is the sun losing per second? (d) What fraction of its mass will it have lost in the time found in part (b)?<\/p>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div class=\"\" data-type=\"exercise\" id=\"fs-id1167793465275\">\n<section>\n<div data-type=\"problem\" id=\"fs-id1167793465277\">\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-id1167793465280\">Show that\u00a0<span class=\"MathJax_MathML\" id=\"MathJax-Element-1850-Frame\"><span class=\"MathJax_MathContainer\"><span>E2\u2212p2c2<\/span><\/span><\/span>for a particle is invariant under Lorentz transformations.<\/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<\/div>\n<\/section>\n<\/div>\n<\/section>\n<\/div>\n<\/div>\n<\/div>\n","protected":false},"author":615,"menu_order":11,"template":"","meta":{"pb_show_title":"on","pb_short_title":"1. Relativity","pb_subtitle":"Chapter 1 Review","pb_authors":[],"pb_section_license":""},"chapter-type":[],"contributor":[],"license":[],"class_list":["post-96","chapter","type-chapter","status-publish","hentry"],"part":3,"_links":{"self":[{"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapters\/96","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":11,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapters\/96\/revisions"}],"predecessor-version":[{"id":403,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapters\/96\/revisions\/403"}],"part":[{"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/parts\/3"}],"metadata":[{"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapters\/96\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/wp\/v2\/media?parent=96"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/pressbooks\/v2\/chapter-type?post=96"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/wp\/v2\/contributor?post=96"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/pressbooks.bccampus.ca\/bcitphys8400\/wp-json\/wp\/v2\/license?post=96"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}