37 Relativity

July 13, 2022 | Author: Anonymous | Category: N/A
Share Embed Donate


Short Description

Download 37 Relativity...

Description

 

RELATIVITY

LEARNING GOALS By studying this chapter, you w/ea: w /ea: •



The two postulates of Einstein's special eoy of relaivy, and wat motvates tese posates. Wy diffeen obseves can disagee abo wete two events are smltaneos How elativity pedis tat moving clocks n sow and expementa evdence ta conims ts



How e leng of an obje canges de o te obects moton How e velocy of an obe depends on te ame of efeence fom wic t is observed How te teoy o elaivity modi es te elatonsip between velocty and momenm How to solve pobems invovng wok and knetc enegy fo pat ces movng at elaivstc speeds. Some of te key concepts of insten's geneal eoy o elatvity

?At Brookhaven

National Laboratory in New Yor, atomic nuclei are acceerated to 99.995% of the uti mate speed limit of the universe-the speed of light. Is there aso an upper imit on the k gy of a partice?

hen the year year 1905 began, Albert Einsten Einsten was an unknown 25-year-od clerk n the Swss patent ofce. By the end of that amazing year he had pubished three papers of extraordnary importance One was an analyss of Brownan motion; a second (for which he was awarded the Nobe Prze) was on the photoeectrc eect In the thrd Ensten introduced his sp h  v proposing drastc revsons n the Newtonian concepts of space and time The speca theory of reativty has made wderangng changes n our under standing of nature but Einsten based it on just two simpe postuates. One states that the aws of physcs are the same n a nertia frames of reference; the other

W

states that the speed of ight n vacuum s the same n al nerta frames These innocent-sounding propostons have farreachng impicatons. Here are three: ) Events that are smutaneous for one observer may not be smutaneous for another. 2) When two observers moving reative to each other measure a tme nterva or a ength, they may not get the same resuts (3) For the conservaton principes for momentum and energy to be vaid in al nertal systems Newton's second law and the equatons for momentum and knetc energy have to t o be revised Relatvity has mportant consequences n ll areas of physcs ncudng elec tromagnetsm atomc and nucear physics, and hghenergy physcs Athough many of the results derived n ths chapter may run counter to your intuton, the theory s in soid agreement wth experimenta observatons

37.1

Invariance of Physical Laws

Lets take a look at the two postuates that make up the specal theory of reativ ty Both postulates descrbe what s seen by an observer in an intil frame of nc, whch we ntroduced n Section 42 The theory s "specia n the sense that it appes to observers in such specia reference frames 1268

 

 Invariace of Physcal Law

269

Einstein's First Postulate

Einstein's rst postulate, caled the pp  tt, states: T   p   m   t m   f the laws difered that diference coud distinguish one inertial frame from the others or make one frame somehow more "coect than anoher. Here are two examples. Suppose you watch two chidren playing catch with a bal while the three of you are aboard a train moving with constant velocity. Your observations of the motion of the the bll, no matter how careuly done can't tell you how ast (or whether) the train is mov ing.Another This is because aws of motion the same in every inertial rame. exampeNewtons is the eectromotive orceare(em) induced in a coil o wire by a nearby moving permanent magnet. In the rame o reerence in which the coil is stationary (Fig. 37.1a) the moving magnet causes a change o magnetic ux through the coil and this induces an em. In a dierent frame o reerence in which the mgne is stationary (Fig. 37.1b) the motion of the coil through a mag netic eld induces the emf. According to the principle of relativity both o these rames of reference are equally valid. Hence the same emf must be induced in both situations shown in Fig. 371. As we saw in Chapter 29 this is indeed the case so Faradays aw is consistent with the principle of relativity Indeed ll o the laws of electromagnetism are the same in every inertial frame o reerence. Equaly signicant is the prediction o the speed o eectromagnetic radiation, derived rom Maxwell's equations (see Section 32.2). According to this analysis light and al other electromagnetic waves travel in vacuum with a constant speed now dened to equal exactlyis299,792458 m/s. useexact the approximate X 10 mis which with in one part within in(We 000often of the exact value.) As we wevalue wil c = 3.00 see the speed of ight in vacuum plays a central role in the theory of relativity Einsteins Second Postulate

During the 19th century most physicists beieved that light traveed through a hypothetica medium caled the ether just as sound waves travel through air. If so the speed o light measured by observers would depend on their motion rea tive to the ether and would thereore be dierent in dierent directions. he Micheson-Morley experiment described in Section 35.5 was an eort to detect motion of the earth relative to the ether. Einsteins conceptual leap was to recog nize that if Maxwells equations are valid in all ineria frames then the speed of ight in vacuum should also be the same in al frames and in all directions. In fact Michelson and Morley detected no ether motion across the earth, and the ether concept has been discarded Athough Einstein may not have known about this negative result it supported his bold hypothesis of the constancy o the speed of ight in vacuum. Es's sd psu ss: ss:  d  g  uu          d  dd      u

Lets think about what this means Suppose two observers measure the speed of light in vacuum One is at rest with respect to the ight source and the other is moving away from it Both are in inertial frames of reference According to the principle o relativity the two observes mus obtain the same result despite the fact that one is moving with respect to the other If this seems too easy consider the ollowing situation A spacecraft moving past the earth at 1000 m /s res a ssile straight ahead with a speed o 2000 m /s (reative to the you spacecraft) 37.2) What is problem the issiles speed reative the earth? Simple say; this(Fig is an elementary in reative velocityto(see Section 3.5). The coect answer according to Newtonian mechanics is 3000 m/s. But now suppose the spacecraft turns on a searchight pointing in the same direc tion in which the missile was red An observer on the spacecrat measures the

37.1 T        w (a)   v v        v v   .

 

CHPTER 37 Retivity

12 37.2  37.2

(a)  New (a)  Newto� to�iian mech echanic anicss ma makes kes cor corec ec p red p redcton ctonss about ab out elat elatvey vey sow  sow-o -ovn vng g  ob ob jects  jects;; b b   t makes akes c  coec oectt pedc p edcttos os   abo abot t te behavIOr of light.

(a) A

spaeship 5 movs with spd l  m/s relati e   an bseve n earh  

A

miss M s fired wth speed  I   m/s llave  h spa  spaes eshi hip p.

b

A

gh beam  s emited fm h spaceshp at spd .



Msse (

 .     m/s l  /s +  m/s � 



NEWTONAN ECHANC HOD: HOD: Newia mehas es us rrey hat he mssie mves wih speed  l  m/s reative =

t th sver n earth eart h

5' �

igh bem L)

 =  

  l



 m/s

NEWTONAN ECHANC FA FA ewtnian mhanis tes us /ry tha the lght moves a  sp sp d greae tha c elative o th sver n earth  whh wd ntad Estei's sd pstae

speed of light emted by the searchligh and obains the value c. According to Einstein's second postlate, postlate, the moion of he light after  has left l eft he sorce so rce cannot depend on the moton of the sorce. So he observer on earth who measres the speed of his same light mst also obtan he vale c, not c +  ms This resl contradicts or elemenary notion of relative velocites and it may not appear o agree wth common sense. Bu "common sense is inuton based on everyday experience and this does no usaly inclde measremens of the speed of ight.

The Ultimate Speed Limit Einseins second postuate mmedaely mples the following reslt:   p f   v  v 

,

 pd f   v

We can prove hs by showng ha ravel a c mples a logical conradcion. Sppose hat the spacecraf S in Fig  is moving a the speed of igh rela tive to an observer on he earth so that c. If he spacecraf rns on a head light the second postlate now asserts that the earth observer S measres the headlght beam o be also moving a c Thus this observer measres hat the head

uSls



lght beam and the spacecraft move together and are always at he same pont in space. Bt Einsteins second postulae also asserts ha he headligh beam moves at a speed c relative o the spacecraf so they cannot be at the same point in space This contradicory reslt can be avoded only f t s impossibe for an iner ial observer sch as a passenger on the spacecraf to move at c As we go through our discusson of relaivty you may nd yourself asking he quesion Ensten asked himself himself as a 16-year16-year-old old student "Wha "Wha  woldI woldI see ifI were rav eling at the speed of lgh? Einsten realized only years later that his qesions basic aw was that he could not travel a c

The Galilean Coordinate Transformation Les restate ths argument symbolically usng wo inertia frames of reference labeled S for the observer on earh and S for the moving spacecrat as shown n Fig  To keep things as simple as possible we have omtted the axes The -axes of the two frames lie along the same line b the orgin 0' of frame S moves relaive to the orign 0 of frame S wth constan velocty u along the com mon axs. We on earh se our clocks so that the two origins coincde a tme t  so heir separation at a later ime t s ut 

 

371 Invariance of hscal Laws 



) 11   -----�p �p x

"y Oii ° d  0  de  me,



0



 The positon of particle P can be  descrbed by the coordnates x and y in rame of eference S o by x' and  in fame 

x' 

Frame 5' moves elave  fm 5 with cn oy I ag e mm x  x'x'-ai ai..

\"

 0' -ut _  x





I

X'

aionss equaion se  Many of   the equ e wi wise rdia iae crd a   frame frame  c ierti ertia ur   i se   ur Chse sated in  f ames  ames  as sate rence f  ial refe reference inerial your iner dene yo re  only only  if you de chape are re  in s ch derrived in de N  CAUTION CAUTIO

on in  in  diecton the   diect on mus ustt be the  -diect cton stvee x -die the  po postv instance nce,, the  h. Fo insta aagrap raph. eding g paag the prec precedin ecion is  is  o the origin  O. In Fg. 373 his di ecion he   origin  ves elav elavee to he mov hee oigin oigin 0' 0'   mo whch h cion x-diecion hee posiiv posiivee x-die  dene   h must dene ef f reaiv reaivee to 0, you must movess to the e  n sead 0 move  igh; igh; if  nsead to be o the eft.

Now think about how we descrbe the moton of a partcle . Ths mght be an exploratory vehcle aunched from the spacecraft o a puse of lght from a aser We can descrbe the position of ths partcle by usng the earth coordinates (   z )  n S or the spacecraft coordnates ( '  ,  ) n S. Fgure 373 shows that these are smply related by  = x + ut





(Galean coordnate transformaton)



(371)

These equatons based on the famlar Newtonan notons of space and tme are called the Gallean coordinate transformaton If patcle  moves n the -drecton ts nstantaneous veocty  as meas dxldt, Its velocty ;  as measured by ured by an observer statonary n S s  an observer statonary n S s : = 'dt. We can derve a relatonshp between V and  by takng the dervatve wth respect to t of the rst of Eqs (371) =

d d -= + u dt dt Now ldt s the velocity  measured n S and dxdt is the velocty  measured n S so we get the Gaiean veociy transformation for one-dmensonal moton v, = ;

+

u

(Galean velocty tansformat tansformaton) on)

2

.2

Although the notaton ders this result agrees with our dscusson of reative velocites n ection 35 Now heres the fundamental problem Appled to the speed of lght n vacuum c + u. Ensteins second postulate supported subse Eq. (372) says that c quenty by a wealth of expermenta evdence says that c = c. Ths s a genune nconsstency, not an iluson and t demands resoluton If we accept ths postu ate we are forced to conclde that Eqs (37) and (372) cannot be precisely correct despte our convncng dervaton. These equatons have to be moded to brng them nto harmony wth this princple The resoluton nvolves some very fundamental modcaons in our kne matc concepts The rst dea to be changed s the seemngly obvous assumpton that the the observers n frames S and S use the same time scae formally stated as t = t. Alas we are about to show that ths everyday assumpton cannot be cor 

rectthe observers have derent scales. We must deneare thenot veloc ty n two frame S as ust =  Idt not as tme ldt; the two quantites the same The diculty les n the concept of  simutanei whch s our next topc A careful analyss of smutanety wll help us develop the appropriate modca tons of our notons about space and tme

 

122

CHPTER 37 Relativity s Your Undrsndng of Scon 

As a highspeed spaceshp ies past you t res a srobe ight that sends out a pulse of ight in al directions An oserve aboard the spaceshp measures a spherca wave fron tha speads away from the space ship with the same speed c n al directions (a) What is the shape of the wave front hat you measure? i) spheical; (i) elpsoidal with the ongest axis of the elipsod aong the direction of the spaceships motion (iii) elipsodal wih the shotes axis of he elipsoid along he drecion of the spaceships moion iv) not enough infomation s given to decide ) Is he wave fron centeed on the spaceship

37.2 4 An event has a denite poston and tme-for insance, on he pavement direcly beow the center of he Eifel Tower at mdnght on New Year's ve.

Relativity of Simultaneity

Measuring times and time intervals invoves the concept of smlanet In a given frame of reference, an even is an occurrence that has a denite position and time (Fig 37.4). When you say that you awoke at seven 0' clock, you mean that two events (your awakening and your cock showing 7:00) occurred simultaneously The fundamenta probem in measuring time intervas is this In general, two events that are simutaneous in one frame of reference are not simultaneous in a second frame that is moving reative to the rst, even if both are inertia frames

A

Thught Experiment in Simultaneity

This may seem to be contrary to common sense. To ilustrate the point, here is a version of one of Einstein's thought exper iments-menta experiments that foow concepts to their ogica concusions. magine a train moving with a speed comparable to c, with uniform veocity (Fig. 37.5) Two ightning bolts strike a passenger car one near each end. Each bot eaves a mark on the car and one on the ground at the instant the bot hits. The points on the ground are labeed  and  in the gure and the corresponding points on the car are  and  . Stanley is stationary on the ground at 0 midway between  and B. Mavis is moving with the t he train at 0' in the midde of the passenger car midway between  and B  . Both Stanley and Mavis see both ight ashes emitted from the points where the lightning strikes Suppose the two wave fronts from the ightning strikes reach Stanley at 0 simutaneousy. He knows that he is the same distance from  and  so Staney concudes that the two bolts struck B and  simutaneousy. Mavis agrees that the two wave fronts reached Staney at the same time, but she disagrees that the ashes were emitted simutaneousy Staney and Mavis agree that the two wave fronts do not reach Mavis at the same time Mavis at 0' is moving to the right with the train so she runs into the wave front from  before the wave front from  catches up to her. However, because she is in the middle of the passenger car equidistant from  and  her observation is that both wave fronts took the same time to reach her because both moved the same distance at the same speed c. (Recal that the speed of each wave front with respect to either observer is c) Thus she concudes that the ightning bolt at B strck bo the one at ' . Stanley at 0 measures the two events to be simutaneous, but Mavs at 0 ' does not! Whether or not two events at d erent x-axis locations a simultaneous depends on the state of otion of the observe You may want to argue that in this example the ightning bots reay are simultaneous and that if Mavis at 0' could communicate with the distant points without the time deay caused by the nite speed of ight, she woud reaize this. But that would be erroneous; the nite speed of information transmission is not the rea issue. If 0' is midway between A and  then in her frame of reference the time for a signal to trave from  to 0' is the same as that from B to 0 ' . Two signas arrive simutaneously at 0 ony if they were emitted simutaneousy at  and  In this exampe they o not arrive simutaneousy at 0', and so Mavis must concude that the events at  and B were not simutaneous.

 

 Relativty f mutanety

1273

5 A thought experimen in smutaneity  Ligig i  t  d  back  a rai (poi A '  ad )  and  i    pi A  d S.

A ly o

Td  t  t   s s  mv oward  it c rom   frot of t t d wy rm t i   t - back   t t

b 



A

o

(c)

Bcs Ms   g  !   t o    t !     t  lgig   t   o   i i !.



A

d



A

Saley ss t lti t  t two poi   m  tim: t  iv tt t t  t lit g i t ot  d the back o t t simu imull aeou  aeou   ll y.  y . A  POiI,  lt rom   li i     i t      o  i s  y t eaced aviis   av

Furthermore, there is no basis for saying that Stanley is right and Mavs is wrong or vice versa. Accordng to the prncple of relatvity no inertal frame of reerence is more correct than any other in the formulaton of physical aws Each observer is COect in his or her own fme of reference In other words simltaneity s not an absolte concept Whether two events are smultaneous depends on the frame of reference As we mentioned at the beginning of this section simltaneity plays an essental role n measuring time ntervals It ollows that the time interval between o eents may be dent dent in derent derent frames of reference. So our next task is to learn how to compare time intervals in dierent frames of reerence. Ts Yr Udsdg  c  Staney, who works for the rail system shown in Fig. , has carefuy synchronized the cocks at a of the ra stations At the moment that Staney measures a of he cocks striking noon Mavs is on a high-speed passenger car raveing from Ogden vie toward North Haverbrook. According to Mavs when the Ogdenvie Ogdenvie cock strike noon what ime is it n North Haverbrook? i) noon; (i before noon (iii) afer noon

 

24

CHAPE 37 

 

3703

We can derive a quantitatve relatonship between tme intervals in derent coordinate systems. To do this, let's consder another thought experiment. As before, a frame of reference  moves along the common -axis wth constant speed reative to a frame  As dscussed in Section 37.1, must be less than the speed of lght Mavs who is ridng along with frame  measures the tme nterval between two events that occur at the sme pont n space Event 1 s

t

Phys CS 

Relativity of Time Intervals

Rlivy fT

u

u

c.



when ash light been fromreected a light source Event d2 away, is when the ash returnsa to  of havng from a leaves mirror a distance as shown n Fg 376a. We label the tme interva Lto using the subscrpt zero as a reminder that the apparatus is at rest, wth ero velocty in frame  The ash of ght moves a tota distance 2d so the tme interva s

Lto

2d 

373

-

c

The roundtrp time measured by Stanley in frame  is a different interval Lt; n his frame of reference the two events occur at d erent points n space. During the time Lt the source moves relative to  a dstance Lt (Fig. 37.6b) In  the roundtrp distance is 2d perpendicular to the relatve veocty but the roundtrp distance in  is the longer distance 2/ where

u

In writing this expresson, we have assumed that both observers measure the same dstance d. We wll justify ths assumpton n the next section. The speed of ight is the same for both observers so the round-trip time measured n  is

4 We woud ike to have a relatonship between Lt and Lto that is independent of d To get ths, we sove Eq (373 for d and substtute the resut into Eq. (37.4), obtanng

-c � c  (u) 2

t

=

Lto  + 2

Lt  2

(37.5) 

6 (a Mavis, in frame of reference S', observes a light pulse emitted from a souce at 0' and reected back along the same lne. b Ho� Stanley (in frame of reference S) and Mavis observe the same light pulse The positions of 0 at the times of departure and eturn of the pulse are shown

b



Mvs beve  ligh pue eed fo  sue  0 d eee k lg he e le e..

Mirr

Souce 0'

Mvs meue e interal O

? Snley see

Sey ee  loge e el : Te gh pule  a e pee  n S, u ve  gee dsne h i S S..

o he e Lg pue fllwg  ign p

 

37 Relativty  Tm Intervas Now we square this and solve for I t 

25

It; the result is to to = 

  -

VI

U

:2 

2

 

C

Snce the quantity  - u2/ c is ess than  t is greater than to: to: Thus Stanley measures a lnger round-trip time for the light puse than does Mavis.

Time Dilation We may generalize this important result. In a particuar frame of reference sup pose hat two events occur at the same point n space The time nterval between these events as measured by an observer a rest n this same fame (which we cal the rest fme of this observer) is to to Then an observer in a second frame moving with constant speed u relative to the rest frame will measure the time interva to be t, t, where (tme dilation)



We recal that no inerial observer can travel at u = c and we note that VI -  / s imaginary for u > c Thus Eq  gives sensible results only when u < c The denominator of Eq  is always smaler than , so t is always arger than to to Thus we call this eect im ln Think of an old-fashioned penduum clock that has one second between ticks as measured by Mavis n the cock's rest frame; this is to to If the cock's rest frame is moving reatve to Stanley he measures a time between ticks t that is longer than one second In brief  bservers measure any clck t run slw  it mves relative t them (Fig  Note that ths conclusion is a drect resut of the fact that the speed of light n vacuum is the same in both frames of reference The quantity  V -  /  n Eq  appears so often in relativity that t is given ts own symbol  (the Greek letter gamma:

 This image shows an explodg star cale a uv wth a sant galay. he brghtess of a typca superova decays a a certa rae. Bt speovae hat are movg away rom s a a sbstantia  racion racion o o he speed of ligh decay more slowly,  accordance wih Eq. (37.6) he ecayig sperova s a mong "clock that rs slow

 In terms of this symbol we can express the time dlation formula Eq.  as

t  1to

(time dilaton

(378)

As a further siplication u / c is sometimes given the symbol { (the Greek letter beta then   l /� Figure  shows a graph of  as a function of the relative speed u of two frames of reference. When u s very small compared to c  / is much smaler than  and  is very nearly equal to . In that imit Eqs  and  approach the Newtonian relatonship t   to corresponding to the same time interval in all frames of reference If the relatve speed u is great enough that  is appecaby greater than 1, the speed is said to be relativistic if the derence between  and  is negigibly small, the speed u is called nn nnlativistic. lativistic. Thus u  6.00 X 0 m/ s  0.200c (for which   02 is a relativistic speed but   6.00 X 04 m /s  0.000200c (for which   00000002 is a noeativistic speed

Prope Time There is only one rame of reference in which a clock is at est and thee are in nitely many n which it is moving Therefore the time interval measured between two events (such as two ticks of the cock that occur at he same point in a

8 he aty  1/   U2  C2 as a  co co of the relatve spee u o two frames o reerece. As sped LI apprche the pd of g   pprache    y y

 6  4 

"=

�   l l22 2

' .

.  . .   . 

• 







1 1 1 1 1 1 1 1 1 I

-=  - - - __ __

o

0

0 Speed L

00

 

6

HR 37 Relativi

particular frame is a more fundamental quantty than the interval between events at dierent points We use the term propr m to descrbe the time nterval between two events that occur at the same point CAUTON

   9 9 A ame of reerece picured as a coordae system wh a grd o sychro ized clocks. 

I

-'88 88 8 8 8 I























-8 x I >F

 ·· .

The grid is three dmenoa; identcal pae f k e i rn  d behid he page, cnected y grd lie peredur  he age a ge..

Mea easu surin ring g tim time e int inter erva vals ls I is mp mpor ortan tan o o  oee h ha a   he he   i ime me    erv ervaal t    i Eq E q. (3 (37 7.6)  v vove ovess eve evens ns ha  ha occu occurr at at d  dfr  fr ent spa space poi oints nts i i h  hee fram framee of of refe refere rece ce   S. Noe aso No aso ha a ay y di  di  erece erecess betw be tween een    t an and d he pr proper oper  me me to  to are are   nt caused used   by d f  fere  rences n n he  he  mes mes re requr qured ed   or or   l lgh gh o o trav  traveel rom hos rom hosee  space space po  pos o a a  os oseerver a a rest  rest   n  S. n S.   We We ass  assum umee ha ha our our obse o bserve rverr is abl ablee o  cor  correc rec for  for d   d erence erencess in g in  gh h trans ranst t ime imes, s, jus jus as an  asron asronomer who's who's ob observi servig g  he su sun under undersands sands   ha a a eve eve   see  owobserv o eah actuallly occ actua occred 500 500   s ago  ago  o he  he  su's su surface. rface. A  Alea leaively we can use two observe ers, one s saonary aonary a  a the locaio locaio of  of  he   he rs rs even an and he oher oher a he he secod  secod,, each wi with hs or  or  her ow ow  clock. W e can synchro synchroze hese  hese  wo cloc clocks who whou dculy dculy as log log as hey hey are a res in res in the  the same same frame of  referec   referece. For exa example, we we could se send a lgh lgh puse sm smaneously ou sly to the two clocks clocks   from a  a  po poit it mdway mdway   betwee betwee them. W hen he n the pulse pulsess arrve, arrve, the the observ ob servers ers se their their cocks  cocks o  o a prearra prearraged ged   ime. (Bu (Bu note  note hat hat clocks clocks ha ha are synch are synchroiz roized ed  one rame o reerence are nt  general synchroned  any oher rame)

In thought experments, it's ofen helpfu to imagine many observers with synchronized clocks at rest at various points in a particular frame of reference We can picture a frame of reference as a coordinate grid with ots of synchronzed clocks distributed around it, as suggested by Fg379 Only when a cock is moving relative to a given frame of reference do we have to watch for ambiguities of synchronization or simultanety. Throughout this chapter we will frequently use phrases like "Stanley observes that Mavis passes the point   5.00 m y  0,   0 at time 200 s hs means that Stanley s using a grd of clocks in his frame of reference, like the grid shown in Fig 379 to record the time of an event We could restate the phrase as "When Mavis passes the point at x = 5.00 m  = 0 Z = 0 the clock at that ocation in Stanleys frame of reference reads 2.00 s We wi avoid using phrases ike "Stanley sees that Mavis is a certain point at a certain time, because there is a time deay for light to travel to Stanleys eye from the position of an event

Time Dilation DEFY the relevant ncepts:

The concep o me dlao s used whenever we compare he me nervals beween evens as measred by observers n deren neral rames o reerece

SE P the prblem usng the ollowg seps: 1 o descrbe a me nerval, you mus rs decde wha wo evens dene he begnnng and he end o he nerva You mus also deniy he wo rames o reerence n whch he me ierva s measured.  Determe wha he arge varable s.

EEE the lutin as ollows ] I may proems volvng me dlao he me nerval bewee eves as measured n one rame o reerence s he

 prper ime to to The proper me s he me erval ewee wo eves n a rame o reerence n whch he wo eves occur a he same pon n space The dlaed tme t s he longer me erval bewee he same wo eves as measured  a ame o reerence ha has a speed u relave o he rs rame. The wo evens occur a dere pos as measured n he second rame You wll need o decde  whch rame he me nerval s  to ad n whch rame  s t t and t, t, and he solve or 2. Use Eq (376) or (378) o relae t he arge varable

EVLE yur anwer:

to, Noe ha M s never smaller ha to, ad u s never greaer ha   your resus sugges oherwse you need o rehnk yor calculao - 

Time dition at O99c Hgh-eergy suaomc partcles comig rom space eract wth atom  the earh's upper amosphere prodcng usabe part ce led n A muon decays wh a mea feime o 0  0-  as measred n a frame o reerece  which i s a rest f a muon s moving a 0.990c (abou  97 X 108 m / s) relave o he earth wha will you (a observer o earh) measue s mea lietme to be?

j

DEFY: hs prolem conces the muons eme whch is he me erval beween wo evens he producion o the muo ad is subseqen decay hs leme s measured by wo der e oservers: one who observes he mo at res and anoher (yo) who observes i movg at 0990c

.

 

 

33 Rlavy of m ras ras

177

ET UP: Let  be you fame o refeence on eath, and le  be

EVALUATE Or resu predicts tha the mean etme of he muon

he muon's frame o reerence. The arget variable s he nerva beween hese events as measured n 

in the earh ame  s about seven imes onge than n the muons rame to. Ths prediction has been vered experimen ay; ndeed i was the rst experimenta conmation o the ime dilaion fomua, Eq 36

EEUTE: The tme interva between the wo events as measued n 220 X 10-6 s, is a proer tme since the two evens occur at he

same position relative to the muon Hence Ho = 220 X 106 s. The muon moves eatve to the earth between he two events, so the wo events occu at different postions as measued in  and he time nterva in that rame is t (the targe varabe) From Eq 376

_?· = 2 X I-6 S       0.990) \/

Examl 

 

=

56 6X X 10 s -

Time dilation at jetliner speeds

An aane ies rom San Fancisco to New York (about 4800 k, o 480 X 10 m) a a steady speed o 300 m/ s (about 60 mi/h) How much ime does the rip take as measued by an obseve on the ground? By an observer in the pane?

,

DENTFY Here we are nterested n what our two observers DENTFY

measure o the time interval between the apane depating om San rancisco and andng in New York.

ET UP The arget variables ae the ime ntervas beween hese evens as measued in the rame o reerence o he ground  and n he ame of reference of the aiane S'

om Eq. 376, 

=

100 00X 0 160 X 104s)\  1

The radica cant be evauaed with adequate pecision wih an ordinay caculato. But we can approxmae it using he bnomal theorem (see Appendx B):

(J - 00 X ) 

=

I 

(100 X 0) + ...

 (�))  (�

The emaining erms are o he orde o 0 or smaer and can be dscaded The approximae resut or o s

to

=

 050 X 0) 60 X 0s ) (I (I

EEUTE The wo evens occu at dieren postons San ran cisco and ew York) as measured n  so the ime interval meas ured by ground observes coresponds o  in Eq 376 To nd

The proper ime  measured n the airplane s very sighy ess (by ess than one pat in 10 than he ime measured on the ground.

 we simpy divde the distance by he speed:

EVAUATE We dont noice such eects in eveyday ie But

/

=

480 X 10 m 300 m/ s

=

60 X 10 S

(about 4 hos)

In the arplanes rame  San Fancsco and New York passing under he pane occur a the same poin (he position of the plane). The tme inerva in the airplane is a proper time, coresponding o  n Eq 36 We have s2 (300 m/ s2 (3.00 X 0 m/s) m/s)

pesen-day atomic cocks (see Section 3 can attain a precision o about one part in 10 A cesium cock aveing a ong dsance n an ariner has been used to measure hs efec and hereby ve y Eq 36 even at speeds much ess han c.

00 X 0  -

Exam     

Just when is it proper?

Mavis boards a spaceshp and then zips past Saney on eah at a eatve speed of 000c At the insant she passes, both start tmers. (a) At he instant when Staney measures that Mavis has aveled 00 X 107 m past him what does Maviss timer read? (b) At the insan when Mavis eads 0.400 s on her ime, what does Staney ead on hs?

·t

are when Mavis passes Stanley and when Saney measues Mavis as havng aveed a distance o 900 X 107 m the arge variabes ae the tme inervals between these two evens as measued in  and in  The wo events in part (b) are when Mavis passes Staney and when Mavs measures an eapsed ime o 0400 s the taget variable is the time inerval between these wo events as measued n S As we wil see understanding his exampe hnges on undesanding the diference between these two pars o evens

DENTY This pobem nvoves ime daton or wo di dirnt rnt

EEUTE a) The wo events, Mavis passing the earth and Mavis

sets of events the sarting and stopping o Mavss tmer and the starting and stopping of Staneys timer. ET UP: Let  be Staneys rame o eerence, and et  be Mavss ame o eerence. The two evens o nteest in pat (a)

eaching x = 900 X 107 m as measured by Staney, occur at dier en postons n Saneys rame but at he same poston in Mavs's rame ence the time interva in Saney ame S is !t while the time interva in Mavis's ame S is the prope time  As measued Cninued

 

128

CHPR 37 Reliviy

by Stanley, Mavis moves at 0.600 0.600(300  08 ms) .0  0 m/s and traves the 900  07 m n a ime 6r (900 X 07 m/( 0 X 0 m/s 0500 s From Eq 36 Mavis's timer reads an eapsed time of 







1 tYI - u2 /C2 0.00 sY  - (0 (06 600 00  0400 s b I is emptingbut wrongto answer that Staneys tmer reads 000 s. We are now consdering a dier pair of evens the starting and the reading of Staneys timer hat boh occ at the same point in Staney' earh frame S. These two evens occ a dierent positions n Mavis's frame S', so the ime interva of 000 s that she measures between these evens s eua to 6t. 





In her frame Staney passes her a time zero and is a distance behind her of ( I 0  0 m/s(000 s) 20 X 07 m a ime 0.400 s The ime on Saneys timer is now the t he proper time: =

Mo



  tYI -

U /2



0 400 sY sY11 - (0 (06 600 00 



0.30 0.3 0 s

diference between 0.00 s and 0320 s sti tro EVALUATE: I the diference bes you consder the foowing: Staney taking proper account of the transit tme of a signa from x = 900  07 m says that Mavis passed that point and his timer read 0500 s at the same insant Bu Mavs says ha those wo events occurred at dierent positions and were nt simtaneosshe passed the point at the insant his tmer read 030 s. his exampe shows the reaivty of simutaneity

The Twin Paadox Equatons (376) and (37.8 fo tme dlaton suggest an apparent paradox called the w paradx Conside dentcal twn astonauts named Eatha and Astd Eartha emans on eath whle he twn Astd takes o on a hgh-speed tp though the galaxy Because of tme dlaton, Eatha observes Astrid's heatbeat and al othe e pocesses poceedng moe slowly than he own Ths to Eatha, Astid ages moe slowly; when Astd etus to eath she s yonge has aged less than Eatha Now here s the paadox: Al netal ames ae equvalent Can't Astid make exacty the same aguments to conclude that Eartha s n fact the younge? Then each twn measues the other to be younge when theye back togethe, and that's a paadox To esolve the paadox, we recognze that the twns ae  identcal n all respects Whle Eatha emans in an appoxmatey netal ae at al tmes Astd must cc wth espect to that inetial fame dring pats o he tp n oder to leave tun aound and etun to eath. Eatha's refeence fae s always appoximately netal Astd's s oten far rom netal Ths thee s a eal phys cal deence between the ccumstances o the two twns Cae analyss shows that Eatha s coect when Astd etus she s younge than Eatha

standi ng on the Ts You Us of Sco  Samir who is standing ground starts his sopwach at he nstant tha Maria es past him in her space ship at a speed of 0600 same instant Maria starts her a As at the measured n Samirs frameAtofhe reference what is the readng onstopwatch Marias sopwatch instant that Samirs sopwach reads  I 00 s?  0.0 s; ii ess than 0.0 s; ii more than 0.0 s b As meased in Maras frame of reference what is the reading on Samirs Sa mirs sopwatch at the instan tha Marias stopwatch reads 00 s? i 00 s ii ess than 00 s iii ii i more than than 00 s

374

 v

t

Physc 

Rlatvy f Lngh

Relativit of Lengt

Not only does the tme nterval between two events depend on the observes fame of reeence but the sc between two ponts may also depend on the obsever's rame of refeence. The concept of smutanety s involved Suppose you want to measue the length of a movng ca One way s to have two asss tants make maks on the paveent at the postons of the font and ea bumpes Then you measue the dstance between the maks But you assstants have to make the maks  h sm m I one maks the postion of the font bumpe at one tme and the othe maks the poston of the ea bumpe hal a second late you wont get the ca's tue ength Snce weve leaned that sultanety sn't an absolute concept we have to poceed wth cauton

 

34 Relivy of Legh

279

Lengths Parallel to the Relative Moton To develop a relationship beween lengths tha are measured parallel to he direction of motion n various coordnate systems, we consider another thought exper iment. We attach a ight source to one end of a ruler and a mirror o the other end. The ruler is at rest in reference frame ' and its length in this frame is o (Fg 37  lOa). Then the time o required for a light pulse to make he round trip from source to mirror and back s

2o o

=

  

c

(37. (3 7.9) 

This is a proper time interval because departure and retu occur at the same point in  In reference frame  the ruler is moving to the rght wih speed  durng his travel of the ight pulse (Fig 37Ob) The length of the ruler n  is I, and the time of travel from source to mirror as measured in  is [ Durng this interval the ruer with sorce and mirror attached moves a distance  [ The toal length of path d from source o mirror is not  but rather

30 The light pulse travels wth speed , so t is also true that

371  Combining Eqs. (37.1) and (37 l) to elimnate d we nd

c

-

31



Dividng the dstance I by c  does n mean that lght travels with speed c  but raher tha the disance the pulse travels in  is greater than t. n the same way we can show that the time  for the return trip from mirror to source is -



-?

(a)

=



  

c

+



3m

aVi

So urce  

io 

 

�  l   

The ler is sttnay n Mvs Mv s's fme  eeence  .. The lght puse tav tav ls  sne 0  m he lgh surce  th mir

r

/

The rle ms t peed u  Ses ae  eeee  The gh puse raes a stce 1 (e ength  e e measured  S) pu a addnl dsane I �([ m e ght source  te mrr.

      A ruler is at es in Mavis's fame 5 A light plse is emjtted from a source at one end of the ruler, reected by a mrror at the othe end and retuned o the sorce position. () Motion of the lght pulse as measured n Stanleys rame 5

 

28

C HAPTE R 37 Relativy The

total It I, +It +It2 It c-u+c+u c(lu/c2) It It It time

for the round trip, as measured n S s

=



l_

l_ 

37.14

We also know that and are reated by Eq. (376) because is a proper time in S Thus EQ (379) for the round-trip time in the rest frame S of the ruler becomes

Finally combning Eqs (3714) and (375) to eliminate obtain

l lR   2  l 

1 -?  c y

l

It

(5)

and simpifyng we

(ength contraction)

-u2/c2

6

shorter

l

[We have used the quantity y  lvl dened in Eq (377)] Thus the length measure measured d in S in which the ruer is movng is than the ength measured in its rest frame S UION

L  s  his is not an optca usion! The rer reay s shorer in reference rame  than t is in ' A ength measured in the frame n whch the body is at rest (the rest frame of the body) s called a prpr gh; thus L is a proper ength n S and the length measured in any other frame moving reatve to S is This eect is caled gh r When is very smal in comparison to y approaches  Thus in the imt of sma speeds we approach the Newtonan reatonship L = This and the corre sponding result for time diation show that Eqs (37) the Gailean coordnate transformation are usualy sufciently accurate for relative speeds much smaler than f is a reasonable fraction of however the quantity V can be appreciaby less than . Then can be substantially smaler than  and the eects of ength contraction can be substantia (Fig 37.1).

u

     The speed at whic electrons traverse he k beam ine of the Stanfod Linea Acceerator Center s sower han c by ess than 1 cm/s. As measured in the reference frame of such an eectron, the beam ine (whch exends from the top o he bottom of his photograph) is ony about 5 cm ong'

Beam lie

c

c u

less than l. l

c l

-u2/C2

Lengths Perpendicular to the Relative Motion We have derived Eq. (3716) for engths measured n the drection to the relative motion of the two frames of reference engths that are measued r to the drection of moton are contracted To prove ths consider two dentical meter sticks One stick is at rest in frame S and ies along the pos tive -axis with one end at 0, the origin of S The other is at rest in frame S and lies aong the positive -ais with one end at 0 the origin of S Frame S moves in the positive direction relative to frame S Observers taney and Mavs at rest in Sand S  respectively station themselves at the 50-cm mark of ther stcks At the instant the two orins coce te two sticks e aong he same line At ths instant Mavs makes a mark on taney' taney ' stick at the point that t hat coincides with her own 50-cm mark and tanley does the same to Maviss stick uppose for the sake of argument that taney observes Maviss stick as longer than his own Then the mark tanley makes on her stick s its center In that case Mavis will think tanley stick has become shorter since half of ts length coincides with than haf her sticks length length o Mavis observes movng stcks getting shorter and tanley observes them getting longer. But this mplies an an asymmetry between the two frames that contradicts the basc postulate of relativit relativityy that tells us al ineial frames are equivalent We conclude that consstency with the postuates of relativty relativty requires that both observers measure the rulers as having the ength even though to each observer one of them is stationary and the other is

endicular

not

less

same

parallel pe

below

 

8

C H A PT E R 37 Ravy

at rest We wnt to nd he length  I mesured by observers on erh. From E 3716 f

= 10) 

-

:=

(0.9 .990 902 400m)V - (0

rest o mease he length I, wo observers wh synchron synchronzed cocs coesure the postons of the two ends of the space p ltneosly n the earth's reerence frame, as sown n Fg. 373. ese wo measements will  ppear smtaneous to n observer n e spaceshp)

56.4 m

VL Tis answer mkes sense: he spaceship s shorter n

  

 frme n wch t s in moon thn n a frme n whch  s a

-

Hw fr r r h bsrvrs? Te two observers menoned n Exmple 37 re 56.4 m aprt on he eJh How  p does the t he spcesp spcesp crew mese them o be? . DNFY he two sets of observers are the same s n xm ple 37.4, bt now he dsnce beng mesred is te separaton beween the wo erh observers. S  Te dstnce between the erth observers as mesued on  rrr engh, snce he wo observers are at rest n the eart s   r

ert rame (Thnk of  lengt of ppe 564 m ong ha exends from 0 to O2 n Fg 37.13. s pipe s a res in he erth frme,  o  leng is a oer lengt he earh is movng relave to te spacesp a 0990c, so the spaceshp crew will mease a dsnce sorer thn 56.4 m beween he wo erth observers Te vale t tey mesre s or target varbe. U: W 

V Ths nswer does  sy that the crew measres ther

spcesp o be boh 400 m long and 796 m long he observers on earh measre he spceshp to hve  contraced ength of 56.4 m becse tey are 56 m pa wen tey measre the pos pos ons of the ends a wh tey measre to be the sme nstant. (Vewed from te spaceshp frame, te observers do not measre hose postons smltaneously. Te crew hen measres he 56.4 m proper lengh to be contraced o 796 m Te key pon s that the measremens made n xmple 374 (n whch he erth observers mese te dsance between te ends of te spceshp) re dffer dffer ent from those made nbetween ths example (n observers) whch the spceshp crew meases the disnce the erth

= 5 m and = 0990c te length  I hat the 

crew bers mese s 1

=

lo�  - < = 



56.m)V  (0 (09 990 90) )

7.96 m

-

Conceptual Exampe  ..6 Mvig wh   As ws stated n ample 37,  mon hs, o averge, a proper fetme o 220  0 s and a dlted lfetme of 56 X 0 s n a frame n wch ts speed s 0990. Mlpyng consn speed by tme to nd dstnce gves 0.990(300  108 108m/s) m/s)    1-6 s = 653 m and 0.990(300  08 m/s) X (5.6 X 10 s = 630 m Interpre tese tw dstances 1 ') U   wil ey wil they ers,, th ervers obsserv t   ob .99 90c pt vess    0.9 on   move age   muon verage If an ver y  cay n to  deca hen  nd he onee po ted d at on ete asur uree   t to be  cre meas pe,   ampe, y. For exam wy  m w 63 nt 463 point her   poi noher t   no laerr  t - s lae 10.6   X 10 5.6 5  n nta and nd    a   mounta p  of a     to top th   t t  evel el   wth d  ev ed creee d  be cr cou ud is  is   mon co

heen mov h ovee  st str rg g t down o o   dec ecaay t     se se   4630 30  m  belo low w.

owever n observer movn t an average mon wl say hat t trveled ny 653 I becse  exsted or ony 0  0 s To show ha ha  answ s copeey consstent

consder he montan. Te 630m dsance s s heght, a proper length n the drecton o moon. Relve to te observer travelng wth ths mon he mountain moves p  0990 wth the 4-m engh contrcted to 

=

=

1



-

= C

630m)Vl - (0990)

653 m

hus we see tat lengt contracon s conssten wth tme da ton e same s true for an eecn movng t speed u n  lnear cceerator (see Fg. 371 Compared o he vales measred by  physicist alongsde acceerator an observer rdn along wthstandng te elecon wold he measre the cceeror's engt and the me to travel tat length to boh be shorter by a actor of V I - U2/C2

-

 

37 The L 

How an Object M

v  g

18

Near c Wuld Appea Appear

Let's hjnk a  abou e viual appeaance of a movng ee-dimenonal ody. f we coud see e poon of all poin of e ody mulaneouly, i WGd appea o nk ony n he decion of moion. Bu e don't ee all e pon mulaneouly; lig fom poin fae fom u ake longe o reac u an doe lgh fom poin nea o u, o e ee e fae pon a e poion e ad  eale me. Suppoe e ave a ecangula od   fae paallel o e oodnae plane Wen e look endon a e cene of e cloe face of uc a od a e, e ee only a face. (ee e cene od n compue-geneaed Fg. 3714a) Bu en a od i moving pa u oad e ig a an appeciable facon of e peed of lig, e may ao ee i le ide becaue of e eale-ime eec u decied. Ta i e can ee ome poin a e couldn ee en e od a a e ecaue e od move ou of e ay of e ig ay fom oe poin o u. Conveely, ome ig a can ge o u en e od i a e i locked by e moving od. Becae of all al l  e od in Fg. 37.4 and 37.l4c appea roaed and dioed.

4 Computer simuato of the appea ance of an aray of 2 rods wth sqae cross sectio The centeigores od is viewed end-on he smuaion coo chages in the aray caused by the Dopper eect see Section .6.

a Ara a s



Test Your Understnding of Section 4

A mniature spaceship is yng past you, movng horizotally a a substatia facton of the speed of lgh A a ceran insant, you obseve that the ose and ai of he spaceshjp agn exacly with the two ends of a meter stick hat you hold in your hands. Ran the folowig distaces n ode fo ongest to shotes: (i) he pope legth of the meter sic; i he proper length of the spaceshp ii the legth of he spaceshp measued in your frame of efeece (v) the ength of the mete stic meased n he spaceship's fame of efeece









b) Aa movn o   a D

37.5 Th Lornz Transformaions In ecion 37. e dicued e Galilean coodnae anfomaion equaion, Eq. 37.). Tey elae e coodinae x  z of a poin in fame of refeence  o e coodinae x,  Zl ) o e pon in a econd fame 5 Te econd ame move  conan peed u elaive o 5 in e poive diecion along e common x-x-ai. Ti anfomaion alo aume a e ime cale i e ame in e o fame of efeence a epeed by e addiional elaionip  t = . Ti Galilean anfomaon a e ave een, i valid only n e lm en u appoace zeo We ae no eady o deive moe geneal anfoma ion a ae conen  e pnciple of elaviy Te moe geneal ela ionip ae called e  

The rent Crdinate ransfrmatin Ou  queion i i: Wen an even occu a pon x y z ) a ime , a oeved in a fame of efeence  a ae e e coodinae x  l ) and ime  t of e even a oeved n a econd fame  moving elave o 5 i con an peed u n e + xdecion? To deive e coodinae anfomaion e efe o Fig. 3715 (ne page) ic i e ame a Fig. 37.3 A efoe, e aume a e ogin concde a e niial me   0  . Ten in S e diance fom 0 o 0' a ime  t i ill ut. e coordin te  x i a pper length in S o in S i i conaced y e faco ( 3716). 6). u e diance diance x fom 0 o P, a een in /y \1 - U2 U2/C /C2 2 a n Eq. (371 S i no imply x

 u +  x a n e Galilean coodnae anfomaion u {2 377 X  u +  x I ?

M -

c-

   I I

 Arra mov o   a Dg

(



_   -

j\

\ i \  1 ' /N

 

CHPTER 37 Relativy

1284

5 A d     , ' is    h, so     /  d  (x UI) =

-

y Fram  m ovs relative t frae S w  city u lng he cmmn x-. x-.  ''-a as

 0'

Org 0 a ond a me I

=  = 



s

 x ' �   I ------- . _-lP  

T



y

 

Tle 1.e ent nt  a/o];! a/o ];!(( j" �l �l is   te ptm   ;];]     an   t s easued • i the w         (x  z.  n fr  Sa San n

e

a

 y.  )  r  

1   x 0   t      /1 1-

-0+

_

Song hs quon for  x' w obn

X

 x - u

3718

Equon  s p of h Lonz coodn nsformon; noh p s h quon gng t' n ms of  x nd  To obn hs w no ht h pncp of  qus  th  form of h nsfomon fom S o S' b dnc o h fom  o S Th on dnc s  chng n h sgn of h  oc componn u Thus fom Eq   mus b u h

 x'



R

-ut' +  x

2

I -c

39

W now qu Eqs  nd  o mn  hs gs us n quon fo ' n ms of  x nd t W  h gbc ds fo ou o wok ou h su s

'

 - ux/ ux/c2 c2

30

V - U2 / C

As w dscssd prous nghs ppndcu o h dcon of  moon  no ffcd b h moon so '  y nd z' = . Cocng  hs nsfomon quons w h 

 x'  y' z'





 y z

(Lonz coodnt nsfomon)

372 

'

Ths quons  h Lorenz coordinate ransformaion, h sc gnrzon of h Gn coodn nsfomon, Eqs  nd t ' For us of u h ppoch zo h dcs n h dnomnos nd  pproch , nd h ux/c2 rm ppochs zo. In hs m Eqs  bcom dnc o Eqs  ong wh t t' n gn hough boh h coodns nd m of n n n on fm dpnd on s coodns nd m n noh fm 



Space and ime have become inerined; we can no longer say hat length and time hae absolute absol ute meanings ndependen of he .am .amee of reference Fo hs r son w f o m nd th hr dmnsons of spc coc s  foudmnson n cd p nd w c (x y Z ) ogh h p  of n n

 

37 he Lorentz asfomations

The Lorentz Velocity Transformati Transformation We can use Egs.  to derive the relativistic eneaization of the Gaiean veocty transformation, Eg  We consider ony one-dimensiona moton aon the axis and use the term "veocity as bein short for the -component of the veocity. Suppose that in a time dt a partice moves a distance dx, as meas ured in frame . We obtain the correspondin dstance dx' and time dt' in  by takin dieentas of Egs. : =

dx' y(x - U t) dt' = =y(t y(t -u x/c2 We divide the rst eguation by the second and then divide the numerator and denomnator denomna tor of the resut by b y t to obtain

x' dt'

dx  u t u dx c2 t

Now dx/dt is the veocity  in  and dx' / dt' is the veocty ; in  so we nay obtain the reatvistic eneraizaton

Lorentz veocity transformaton

(3 22)

When u and  are much smaer than c the denominator in Eg.  approaches , and we approach the noneativistic esut � = -u. The oppo ste extreme is the case  c; then we nd =

c -u uc/c22 uc/c

 =-

x

]

_

c(-u/c) =c 1 -u/c

Ths says that anythin movin with veocity  =c measured in S aso has veocty � c measured in  despte the reative moton of the two frames So Eg.  is consistent with Enstein's postuate that the the speed of iht in vac uum s the same in a inertia ames of reference =

The principe of reativity tes us there is no fundamental disinction between he two frames frames  and . Thus the expression for for  n terms of : must have the same form as Eg  with V chaned to � and vice versa and the sin of u reversed. Cayn out these operations with Eg.  we nd

 =

      +

ujc2

Lorentz veocity transformation

72)

This can aso be obtaned aebraicaUy by sovin Eg.  for  Both Egs.  and  are Lorentz veloci tnsfomation for one-dimensiona motion CAUTION   cc c c  cd cd Keep in mnd tha he Lorenz ransfoatio equations given by Eqs. (3721), (3.22 an (373 assme ta frame ' is movig n the positive x-diecio wt velociy u elative to fame . Yo shol always se p yor coordinate system to olow tis coveton

When u is ess than c the orentz v eoci y trnsformatons show us that a body movin with a speed ess than c in one frame of reference aways has a

85

 

* 3 7 6 Th Dr f f gn W

Exampe    88

1287

Rtiv vocitis

(a) A spaceship movng away from the earth wh speed 0.900e fires a robot space probe n he same recton as ts moion, with speed 0700e elave to the spaceshp Wha s he probe's veocity reatve o he earth? b) A scoutshp tries to catch p wh he spaceshp by raveng a 0950e reatve o the earth Wha s the veocty of the scoushp reatve o the spaceship?

the veocty of he probe reatve to S; the arget varabe n part b) s the veocty of the scoushp reatve o S.

EXECU (a) We are given he veocity of the pobe eatve to the spaceshp, v; = 0700e We se Eq veocy v, reatve to the earth:

v:  u 0700e  0900e v = 1  uv:/e  1 + 0900e0700ee

i

IDENIFY:: Ths exampe uses he Lorenz velocity transformation IDENIFY E UP et the earth's rame of reerence be S and e he space shps frame of reference be S' (Fg 3716) The reative veocty of the two frames s

u

=

y

u,  090c

u

000c

u;  000 � 

Scoutship

Robo spce   --Spaceship 0 --------- -  --x   prbe

=

0982e

(b) We are given the veocy of the scoutshp reatve o he eah v  0950e We use Eq 3722) o determine ts veocy v  elave to the spaceshp

0700e. The target varabe in par (a) is

    The spaceshp, robot space probe, and scoutshp

(3723) to etemne ts

v'  = 

v   - u 

l

- 

uvJe2 uvJe2

0950e - 090 0900e 0e _ 0345e 0.900e 0.900e  0950ec?

VLU Its nsructve o compare our results to what we wou have obtane had we se he Galean veocy transfor maon forma Eq 37.2) n part (a) we wou have found he pobe's veocty reatve o the eath o be v = v  u  0.700e + 0900e = 1600e. Ths value is geater han the speed of ght an so must be incorect n part (b) we woud have fond the scosps veocy relative to the spaceship to be v = the greater reatvscay v -u v =0.95 0.950e - s 0900e 0900 e = seven 0.050etimes vaue 0.30e amost han thecorec nco 45e rec Galean vaue

 Y Udd  S 5

(a n frame S events P and P2 occur at the same , - an -coordnates but even P occurs befoe event P. n frame S whch event occurs rst? b) n fame S events P3 an P4 occu at the same tme l and he same - and -coornaes but event P3 occurs at a less posve -coornate than even P• n rame S' whch event occurs rst?

I

*376 The Doppler Effect

for Electromagnetic Waves An additional mportant consequence of relatvisc kinematics s the Dopper efect for eectromagnetc waves. In our previous discusson of the Doppler eect (see Secton 168) we quoted wthout proof the formua, Eq. 630) for the freqency sht that resuts from moton of a source of eectromagnetc waves rela tive to an observe We can now derive that resut Here's a statement of the problem A source of ght is movng wth constant speed  toward Stanley who s statonay n an nertal frame (Fg 7l7) As measured n its rest frame the source emts light waves wth frequency fa and perod T  Il. What s the frequency f of these waves as receved by Stanley? Mving sorce emi waves of reqcy fo fo Frs wve t mtd ere.

Soce el scond sco nd wave e hr

:= I _�  - �

Potio o rst wv e  h i h h cn rt  emit emit Soay eer  eet e  eecyI > l b. taley

A

 

 The Dopper eect for lght A gh  source movng a speed . reatve to San ey emts a wave crest then traves a dis ance uT toward an observer and emts the next crest n Staneys reference rame S, the secon crest s a dstance  behnd the rst cres

 

 Rlivic Monu

Example 37.9

A jet

1289

from a black hole

A number of galaxies have spemassive black hoes at heir cen tes (see Secton 12.8) As maea swis aound such a back hole, it is heated becomes ionized and generates strong mag netc eds. The esing magneic foces see some of he mateia into hgh-speed jets tha bast ot of the gaaxy and into integaactic space (Figre 3719) The be ight we obseve from he e in Fg. 3.19 has a eqency of  666 X 04 Hz, bt in the fame of efeence of the e materia he igh has a fe qency of 5.55 X 10 H (in the infaed egion o he eeco 37     This image shows a fastmoving et 5000 ight-yeas in engh emanating from he center of he gaaxy M87. The igh rom the et is emted by fast-moving eectons spiraing aond magnetc eld ines (see Fg. 2.16)

magnetic spectum) At wha speed is the et mateia movng owad s?

i

DENTFY: Ths pobem nvoves he Doppe efec for eecro magnetc waves ET UP: The fequency we obseve is  f  6  6 66 X 104 Hz and the feqency in the fame of the souce is  fa= 555 X 10 Hz  Snce  f > fa the souce is appoaching us and therefore we se Eq (3.25) to nd he taget variabe u. 

EXECUTE: We need to sove q. 37.25) fo u. That takes a ite ageba; we' eave t as an execise fo yo o show ha the est is

 f  fo l l   -   e If +   66 666 X LO Hz /555 X 10Hz Hz u=

We have  fifo we nd

=

u=

20

so

12.0  - I = 0.986e  :  ) -e 12. 12 .0 + 

EVALUATE Becase the feqency shif s qie sbstantia  woud have been eroneos o use the appoximate expresson  f  fl l  ule Had yo ied o do so yo wod have fond   c   = c6 c6.. 66 X O H  5.55  0Hz/5.55 X 0Hz 0Hz= 110c This rest cannot be coec because the et matea canno rave faster than ight 

37.7 Rivisi Mnu Newton's laws of motio have the same form  al ertal fames of eference Whe we use transformatos to change from one nertal frame to aother, the laws should be invariant (uchagng) But we have just learned that the prcple of elatvty forces us to replace the Gallean transformatons wth the moe genera Lorentz trasformatos As we wl see ths requres correspondg genealzatons  the laws of moton and the dentos of mometum and eergy. The prncple of conservaton of mometum states that whn two bodis intract, th total momntu is constant povded that the et external force actg o the bodes  an erta refeece frame s zero for exampe f they form an so lated system teacting only wth each other). If conservaton of momentum s a vald physcal aw t must be vald in ll n erti al frames of referece Now hees the problem: Suppose we look at a collson n one nertal coordnate system S and d that momentum s coserved hen we use the Lorentz trasformaton to obtan the veloctes n a secod iertal system S'. We d that f we use the 

Newtonan deito of momentum e momentum s not conserved n m) the second system! If we are convced that the prncple of relatvty and the Lorentz transformaton ae corect the only way to save momentum coservato s to generalze the dfntion of momentum. We wont deve the correct elatvstc geeralzato of momentum but here s the result. Suppose we measue the mass of a partcle to be m whe t s

at rest reatve to s We often call

m

the rest mass We wll use the term

 

1290

 H A PTE R 37 elativy

. Graph of the magnitude of he momentum of a partice of est mass  as a unction o speed . Also shown is the Newtonan predction, whch ives corect resuts ony at speeds much ess than c

material patce for a partice tha has a nonzero rest mass. When such a pa cle has a velocity V, ts rsc momnum p s (reatvstic momentum)

Relativic momnu boms nfnt  u poh 

When the paticle's speed v is much less than c this s approximately equa to the Newtonan expression p = mv but n general the momentum is greater in mag ntude than m Fgure  In fact, as v approaches c the momentum approaches innity

p 5/1c

I

3nlc

HAPPENS!� II I I I

:

DOESN''T DOESN

2

I

HAPPEN

4m

Relativity Newton's Second Law, and Relativistic Mass

mc I

'  - -L          

o

. .4c .6 .8

3727)

 u



What about the relativistic generalization of Newtons second aw? n Newtonian mechancs the most general form of the second aw s

d  F=-

Nwonn m inorly ds h momnum boms nnt oly i  bome ii.



378)

dt

That s the net force F on a patce eqas the tme rate of change of ts momen tum Experiments show that ths rest s sti vad n reatvstic echancs, pro vided that we use the reatvstc momentum gven by Eq . That s, the relativisticay correct generaizaton of Newtons second aw s

3729) Becase momentum s no longer drecty proportiona to veocty, the rate of change of momentum s no longer drecty proportona to the acceeraton As a resut, constant foe does not cause constant acceeon. or exampe, when the net force and the velocty are both aong the -axs, Eq . gves 

-

(F and  along the same line)

3730)

where a is the acceeraton, also along the axis Solvng Eq . for the accel eration a gives

 

 

a=F 1_U 1_ U 32 17 C

We see that as a particle's speed ncreases the acceeraton caused by a given force contnuousy decreases As the speed approaches c the acceleraton approaches zero, no matter how great a force is appled Thus it s impossble to acceerate a patcle wth nonzero rest ass to a speed equal to or greater than c We again see that the speed of ight n vacm represents an utmate speed imit Equation . for relatvstc momentum is sometmes nterpreted to mean that a rapdy movng partce undergoes an ncrease n mass If te mass a zero veocity the rest mass) is denoted by 17, then the "relatvstc mass  m s gven by 

ndeed we moecues consder the of a contane), system of particles as rapdy movng when dealgas n moton a stationary the tota such rest mass of the system s the sum of the relatvistc masses of the partcles, not the sm of thei rest masses However, f bndy apped the concept of relativstc mass has its ptfals s Eq . shows, the relativistc generalizaton of Newtons second aw is not =

F

m, and we w show n Section . that the reatvstic knetic energy of

 

77 Ratiis Momnu

9

K = rel

a partcle s not � m 2. The use of relatvistc mass has ts supporters and detractors, some qute strong n the opnons. We will mostly deal wth ndvd ual patcles so we wll sdesep he controversy and use Eq  as the gen eralzed denton of momentum wth m as a constant for each paicle ndependen of ts state of moon We wl use he abbrevaton

1

y V -V = 2 C  C2 2  We used hs abbrevaton in Secton  with u replaced by u, the relative speed  of wo coordnate systems. Here u s the speed of a parcle n a partcua coord nate system-that s the speed of the partcle's rest ame wth respect o that system In terms of y Eqs  and 0 become

p = ymv

3731 31 )

(elatvstic momentum) 

v

(F and  along he same lne)

3732)

In near accelerators (used n medcne as wel as nuclear and elementary partcle physics; see Fg  the net foce F and the velocty v of he acceler ated patcle are along the same stragh lne But for much o the path n mos circular acceleatos the partce moves n unform ccuar motion a constan speed Then the ne force and velocty ae perpendcular, so he force can do no work on the parce and the kinetc energy and speed reman consant Thus the denomnator n Eq 9 is consant and we obtan

.

v

m  a yma (F and perpendcular) 3733) 33) 1   (I _ V 2/C  2/C  ) 2 Recal from Section 4 hat f he particle moves n a ccle the net foce and acceleraton are drected nward along the radus r and a  /r  /r..  What about the geneal case in whch F and v ae neither along the same line no pependicular? Then we can resolve the net orce F at any nstant nto com ponents paalel to and perpendcuar to V. The esultng acceeraton wll have cOesponding components obtaned fom Eqs  and  Because of the deent y3 and y factors the acceleaton components wll not be popor tonal to the net foce components That is unless the net foe on a relativistic  particle is either alog the same lie as the partce's eoci or perpendicular perp endicular to it the t he etforce and acceletio vectors a not parael. parael.

=

F

Relatiistic dynamics of an electron





An electro res mass 911 10-3 kg charge 160 10- C) is moving opposie o an eecric eld of magiude 5.00 10 N/C Al other forces are egligible i compariso to he elecric eld force a) Fnd he magiudes of momentum ad of acceeraio a he isas whe v 00 090 ad 099 b) ind the coresponding acceeraios if a ne oce of he same magide is perpedicuar o he veocy.



E

 I Oc,

. In addiion o he expessios from this sectio fo rel ativistic momeum and acceeraio, we need he relaionship beween elecric force ad elecric ed from Chaper 21  par a) we use 7.1 o determie he magnde of momentum and . o deermine he magnde of accel

DNTY: ST U





eatio due o a force along the same le as he velociy.  pa b he orce is perpendcuar o the velocy so we se 7 o deermie he magiude of acceeration

g

EXECUTE: EXECUT E:  

 V  VV//

(a) T o d bo boh h   he m mag agiude iude of mome momem

magide of acceeraion we eed he values of'

nd  h h  

o each o e ach of h hee three sp speeds eeds W e nd '  '  = 1.00 1.002. 2.29, 29, ad  ad  709. he he

vaues o he momentum magnude are



P  (1.00(9 'W X 0-3 kg0010(00  08m/s = 7 X 1O- 1O-4kgm 4kgm/s /s a  OOO .9911 911  10 10-- kg(090 kg(090(00 (00 X 10 m/s P2  .9  56  0 kg ° m/s at  = 090

u  

CHAPTER 37 Relatity

1292

P3 = (7.09)(9l1  0-  kg)(099)(00  8 m/s) 19 X 102 g· m/s at U = 099c 

he aeleraions at he wo higher speeds are smaller by a a tor o y

= \qE= (60  O-C)(500 x 0N/C) = 800  0-4 N From Eq 7  a = ym When u = O OO O O and y = 00,

hese aeeraions are arger than the orresponding ones in par a by ators o y2

From Chaper , he magniude of he ore on he eleron s

(I

=

 ?  800 0-4  88  0 /s (.00)3(9.1  X 0-3  kg) =

The aeleraions a the wo higher speeds are smaler by ators o y: hese las wo aeleraons are only8.% only8.% and 08%, respeivey o the vaues predied by nonrelavisi mehanis b rom E 7. a = jym if F and v are perpendiuar. When u = 00 I Oc and y = 00 

=

800  0 N  X 0 m/s2 = 88 (.00)(9.  0-3 kg)

EVALUATE: u ress n par a show ha a higher speeds, he relaivsi vaues o momenum dier more and more rom he nonrelaivis values ompued sing p =  mu Noe hat he momenm a 099c s more han hree times as grea as a 090 beause of he inrease in he aor y ur resuls aso show that he aeleration drops o very uikly as u appoahes c A the Sanord Linear Aeleraor Cen ter an essentially onstant eleri ore s used o aelerate ele trons o a speed ony slighly less han c I he aeleraon were onsan as predied by Newtonian mehanis, hs speed would e aaned aer the elerons had traveled a mere 15 m In a eause of the derease o aeleraon wih speed, a pah lengh o  km s needed

Aording o relativsti mehanis when you doube he speed o a parile, the magniude o its momenum inreases by i a ator o ; i a faor greaer han ; iii a ator between  and  that depends on he mass o the parle s Your Undrsndng of Scon 

37.8 Relativistic Work and Energy When we developed the relationship between work and kinetic energy in Chapter 6, we used Newton's aws of motion When we generalze these laws according to the principe of reativity we need a corresponding generaization of the eqation for kinetc energy.

Relativistic Kinetic nerg We se the workenergy theorem beginning with the denition of work. When the net force and dispacement are n the same direction, the work done by that force is W  f x. We sbstiute the epression for F from Eq. 0 the appicable relativistic version of Newton's second law. In moving a partce of rest mass m from pont X to point X2

(37.34) To derive the generazed epression or kinetic energy K as a uncton of speed  we wold ike to convert ths to an integral on u. To do ths, rst remember that the kinetic energy of a particle eqals the net work done on i in moving it from rest to the speed u: K = W. Thus we let the speeds be zero at point X and  at pont X' SO as not to confuse the variable of integraton with the na speed we change  to Ux in Eq.  That is,  s the varying x-component of the velocity of the par ice as the net force accelerates it from rest to a speed  We aso reaize that x and  are the innitesima changes n X and  respectivey n the time interval . Becase   x/ and a   we can rewrte a x in Eq.  as ad x

 

 -d x 

 ,



d-





x 

=  A

v   



 

7. Riv k d 

93

Making these substitutions gives us

fv

K= W = 0 (1

mVrdv r _

�  /e2)3 2

(37.35) 35)

We can evaluate this integal by a simple change of variabe; the nal result is (relativistic kinetic energy)

336) 36)

As v appoaches e, the kinetic energy approaches innty. Iq.  is J coect, it must also approach the Newtonian expresson K = !mv2 when u • is much smaller than e (Fig. 21 To verify ths we expand the radical using the binomial theorem in the orm



Graph of the knec energy of a parce of es mass m as a function of parce speed u Aso shown s the Newtonan pedcto, whch gves correc reslts ony at spees ch ess tan c

(1+x)"= 1+nx+ +nx+n(nn(n- 1)x2/ 1)x2/+ + n ou case n

=

K

-� and x = -v2/e2 and we get

Relativsc knet knet energy beome fn s  pphes 

t

... . . �

HAPPN5!� Combning this with K =

(I

-

1)me2, we nd

 u -1 m v2 -+ -+ K =  +-+  e2 8 e4

(I

1 ?  v4 u+   + +  = u+ 2 8 e2

)?

(3737 37

When u is much smaller than e al the erms in the series inq inq  except the rst are negigiby small and we obtain the Newtonian expression mv2

Rest Energy and E = mc Equation  for the kinetic energy

o a moving partice incudes a term me2 VI - u2 u2/e /e22 that depends on the motion and a second energy term me2 that is independent o the motion t seems that the kinetic energy o a paricle is the dierence between some total energy E and an energy me2 that it has even when it is at rest. Thus we can ewriteq ewriteq

 as (total energy o a partice)

(338

For a partice at rest K = 0), we see that E = me2 The energy me2 associated with rest mass m rather than motion is caled the res energ o the particle. here is in act direct experimental evidence hat rest energy eally does exst. he simplest exampe is the decay o a neutra  pion. his s an unstable subatomc partcle o rest mass "; when  decays t dsappears and electromagnetic adiation appears I a neutal pion has no kinetic energy beore its decay the tota enegy o the radiaton ater its decay is ound to equa exactly mTe2 In many other undamenta paticle transormations the sum o the rest masses o he patices changes. n every case there is a corresponding energy change consistent with the assumption o a rest energy me2 associated with a rest mass  Histoically the principles o consevaton o mass and o energy devel oped quite independenty. The theory o relativty shows that they are actually two special cases o a singe boader conservaton principle the  principl f

HAPPN

I 'mc-

?

�=



7

-

 

Newnn e ny red  ne eergy eme eme nnte ny  v eme n nn nee.

 

94

CHAPTR 37 tivit v f  d y In some physical phenomena, nether the sum

     Although the contro room of a nucear power pant is very compex, the physica principe whereby such a pant operates is a smpe one: Part of the rest energy of atomic nucei is converted to therma ther ma energy, energy, which in turn is used to produce steam to drive eectric generators.

of the rest asses of the partcles nor the total energy othe than est energy is separately conserved but there s a ore general conservaton principle: In an solated system when the sum of the rest masses changes thee s always a change n 1/ ties the total energy othe than the rest energy. This change s equa in magntude but opposite n sign to the change n the sum of the rest asses. This ore general mass-energy consevaton law s the fundamental pnciple nvolvedundergoes n the generaton ofapower through reactons. When a uraniu nucleus sson n nuclear reactonuclear the sum of the rest asses of the resuting fragents is  h the rest ass of the parent nucleus. An aount of energy s eleased that equas the mass decrease Ultplied by  Most of this energy can be used to produce steam to opeate turbnes for electric powe gener ators (Fg 22 We can also relate the total enegy E of a partcle (knetc enegy plus rest energy) directly to its oentu by cobining q. 2 for relatvistic oentu and Eq. 8 for total energy to elmnate the partcle's velocity. The simplest procedure s to rewrite these equatons n the followng fors: and Subtractng the second of these fro the st and reaangng we nd (total energy rest energy and moentum)



Agan we see that for a particle at rest   = 0, E =  quation 9 also suggests that a partcle may have energy and moen tum even when t has no rest mass In such a case  = 0 and

E  

(zero rest mass)

(37.40)

In fact zero rest mass partces do exst. Such patcles always tavel at the speed of ght in vacuu One exaple s the h the quantum of eectromagnetic radiation (to be discussed in Chapter 8 Photons ae etted and absorbed du ng changes of state of an atoic or nuclea system when the energy and momen tu of the syste change.

Example 

nrgtic ctrons

(a) Find the rest energy of an eectron  m =  0  0-31 kg q = - = 602  09 C in joues and n eectron volts (b) ind the speed of an eectron that has been acceerated by an electrc ed from rest, throgh a potentia increase of 200 V typca of TV picture tubes or of 500 MV a votae ray machne)

1

DNIFY: his proem uses the ideas of rest enery reatvstic

From the denition of the eectron vot in Section , 1 eV = 602  0-19 . Using tis we nd

m? = 

1  5 X

 eV eV  602 X 0-19  0 eV  05 eV

X

0-14 

(b) In calclations sch as ths it is often convenient to wor with the uantity  dened from the modied  :

inetic enery, and (from Chapter  eectrc potenta enery =

We usetothe to stated nd thetota restenergy energy and ndrelationship te speed that S Eq U  ives me22the me

U a) Te rest enery s m2 = 0  01 kg 2 X = 1 X 01 J

Sovin this for u, we et

u=e 08 m/s

- ( l fy ) 2

The tota energy  of the acceerated eectron is the sum of its rest enery m and the inetc enery V"a that it gains from te

 

37.

work done on i by the electic ed in moving rom poin a o point b: E=ym= ym= nC2 + eV'

or

V,)( y=I+c An eecron acceleraed hrough a potenia ncease of Vw=0.0 = 0.0 kV gans an amount of energy 00 keY, so fo this eecton we have 00  103 eV or 0511  06 eV = 109

y=  + and u

 c\  (/092 (/092= = 0. = 85  07 m/s

Newtonian Mechancs and Reltivity

1295

Repeaing the calcuaton for Vba =500 = 500 V we nd VbalnC   98 y= 08 and u 0.99. =

VALUATE These esuts make sense: With V V= = 00 kV he

added kinetc enegy of 00 keV keV is less than 4% of the res energy o 05 e eV and the nal speed is abou onefourth of the speed of light. With Vba = 500 V he added kinetc kinet c enegy of 500 eV is much greate than the rest energy and the speed is close o  The eecron ha accel eaed fom rest through a poential increase of 500 V had a kneic energy of 500 e By convention we cal such an eec ton a "500eV electron A 5.00eV eecron has a rest energy of 0511 eV as do al electrons) a ineic energy of 500 eV and a toa energy of 5.5 e Be careful no to confuse hese d eent enegies. CUN

hee elec eees



A r  Two protons each with M= M=   0- kg) are intiay mov ng wh equa speeds in opposite directions They coninue o exist

In hs colision the kinetic energy o wo proons is tans fomed into he rest energy of a new partice a pion

    

afe a headon collison tha). also produces a neua of mass  02 n = .40 =.40 g Fg f he proons andpion the pion ae at rest ater he colsion nd he nital speed of the potons Enegy s conserved in the colison

BFOR Proton

1

Proton

IDENTFY: This poblem uses he idea of relaivisic otal energy

whch is conserved in the collision ST UP We equate the unknown) toa enegy of he two poons before the collision to the combined rest energes of the two po tons and the pion ate the collsion. We then use E. 8) o solve for he speed of each proon EXECUT The oal energy of each proton before he colsion is yM By conservation o enegy (yM (yM

(M2 +  40 X 02 kg  --  0 y  1 + -  +    M (  10 10    27 g

AFTR +

Pio 2.40 X

EVALUATE The iniial kineic energy o each proton s





so u

 c\  ( fy2



0.0



- kneic I M2 energy ythe 00M2 The rest energy o= a proton is 98These eV so is ( (98 eV eV= 5 eV are " 5eV proons) ou can verify that the rest energy of the pion is wice this o 5 e All the kineic enegy lost in ths completey neastic colision is transformed into the rest energy of he pon 

A proton s acceeraed fom res by a constan orce that always points in the drection of the paice's moton Compared to the amount of knetic energy tha he proon gains during he st meer o its travel how much kinetic energy does the proon gan durng one meer o tavel whle t s moving at  99% of he speed o ight? i ght? ) the same amoun; ii) a greater amount ii) a smaler amoun Test Your ndersanding of ection 8

I

37.9

108 kg)

Newtonian Mechanics and Relativity

The sweeping changes equied by the pinciple of elativity go to the vey oots o Newtonian mechaics, incdng the concepts o length and ime he euations o motion and the consevation principles. Ths it may appea that we

 

1296

C H A PTE R 37 Relativy

h dsrod h foundons on whch Nwonn mchncs s bu. In on sns hs s ru,  h wonn formuon s s ccur whnr spds r sm n comprson wh h spd o gh n cuum. n such css m don, ngh conrcon, nd h modcons of h ws of moon r so sm h h h r unobs unobsrb rb. . In fc, r on of h prncps prncps of Nwonn mchncs sus s  spc cs of h mor gnr rsc formuon. Th ws of Nwonn mchncs r no wng; h r incomplete. Th .4 Withou nformaton ro osde the spaceship, e asb'onat cannot dstingish situaton () fom sitaton (). (a) An astonau spcip

s

abo o drop he wa in a

apprximatey r   mng of rsc mchncs. Th corrc whn spdscs r sm n compson o c, nd hr bcom xc corrc n h m whn  spds pproch zro. Thus r dos no comp dsro h ws o wonn mchncs bu geneizes hm. won's ws rs on  r sod bs of xprmn dnc, nd  woud b r srng o dnc  nw hor h s nconssn wh hs dnc. Ths s  comon p n h dopmn of phsc hor. Whnr  nw hor s n pr conc wh n odr, sbshd hor h nw mus d h sm prdcons s h od n rs n whch h od hor s suppord b xpr mn dnc. Er nw phsc hor mus pss hs s cd h d l

The General Theory of Reativity b In gavy avy-- fr ee pace. the no aeleae its s e wa wah h wa a a = g a it

() O e ear ' uae, e wah aeeae owwar  a =  a i he

oor

A hs pon w m sk whhr h spc hor of r gs h n word on mchncs or whhr  further gnrzons r possb or ncssr. For xmp nr ms h occupd  prgd poson n ou dscus son. Cn h prncp of r b xndd o nonnr rms s w? Hrs n xmp h usrs som mpcons of hs quson A su dn dcds o go or Ngr s wh ncosd n  rg woodn box. Dur ng hr r f sh cn o ough h r nsd h box Sh dosn' f o h oor bcus boh sh nd h box r n fr f wh  downwrd ccron of 9.8 m /s2. Bu n rn nrpron, from hr pon of w, s h sh dosn f o h oor bcus hr gron nrcon wh h rh hs suddn bn ud o. As ong s sh rmns n h box nd  rmns n fr f sh cnno  whhr sh s ndd n fr f or whhr h gron nrcon hs nshd. A smr probm occurs n  spc son n orb round h rh. Objcs n h spc son seem o b wghss bu whou ookng ousd h s on hr s no w o drmn whhr gr hs bn ud o o whhr h son nd  s conns r ccrng owrd h cnr of h rh. gur 3724 mks  smr pon or  spcshp h s no n r  bu m b ccrng r o n nr rm o b  rs on h rh's surc Ths consdrons form h bss o Ensns l y f lvy f w cnno dsngush xprmn bwn  unform gron d   prcur ocon nd  unform ccrd rfrnc frm, hn hr cnno b n r dsncon bwn h wo. Pursung hs concp, w m r o rp rsn an gron d n rms of spc chrcrscs of h coordn ssm. Ths urns ou o rqur n mor swpng rsons of our spc-m concps hn dd h spc hor of r. n h gnr hor of r  h gomrc proprs of spc r cd b h prsnc o mr (g. 3725 Th gnr hor of r hs pssd sr xprmn ss ncud ng hr proposd b Ensn. On s hs o do wh undrsndng h roon of h xs of h pn Mrcur's pc orb cd h  precession of he  periheion Th prhon s h pon o coss pproch o h sun.) A scond s concs h pprn bndng of gh rs from dsn srs whn h pss nr h sun Th hrd s s h gravitaona red sh h ncrs n w-

 

3. Newtonian echaics ad Relaviy

1297

5 A wo-dimensional representaio of cved space. We magne he space (a pane) as being isoe as shown by a masse objec (he sun) Ligh fom a isan sa so e oows he disoe sface on is way o he eah The dashe lne shows he ec ion fom which he gh appears o be comng The eec s gealy exaggeaed; o he sun, he maxmm deviaion is ony 000048°

length of ight proceeding outward from a massive source. Some detals of the general theory are more dfcult to test, but this theory has played a central role in investigations of the formation and evouton of stars black holes and studies of the evolution of the universe. The genera theory of reatvity may seem to be an exotic bit of knowedge with ]jttle practcal application In fact this theory plays an essential role in the global positoning system (GPS) which makes it possibe to determne your position on the earth's sace s ace to within a few meers sing a handheld recever (Fig. 3726 he heart of the GPS system is a collection of more than wo dozen satelites in very precise orbits. Each satelte emts carefully timed radio signas and a GPS receiver simultaneously detects the signals from several satel]jes. he recever then calculates the time delay between when each signal was emtted and when it was received and uses ths information o calculae the receivers position. o ensure the proper ting of the signals, its necessary to include cor rectionsto due the specia theoryasofwel reaivity the saelites arethe moving reatve thetoreceiver on earth as the (because general theory (because satel ltes are higher in the earth's gravitatonal ed than the receiver he corrections due to relativity are smal-less than one part in l0 9 -but are crucial to the superb precision of the GPS system

uses ado 6 Aobiing GPS eceie fom he GS saees osgnas dee mine s posiion. To accoun o he eecs of eaiviy he eceive mus be une o a sighy highe fequency (10 MHz han he fequency emed by he saees 09999995 M).

 

CHAPTER

SUMRY

Invariance of physical aws. simutaneity: simutaneity: All of the fundamental laws of physics have the same form in all inerial frames of reference. The speed of light in vacuum is the same in al inertial rames and is independent of the motion of the source Simultaneity is not an absolute concept; evens ha are simultaneos in one frame are not necessaiy simltaneous in a second frame moving relaive o he rst Time diation diation If wo events occur at the same space point n a particular frame of reference, the time interval  between the events as measred in that frame is called a proper ime interval If this frame moves with consan velocity u relative to a second frame, the time interva between the events as observed in the second frame is onger than M his eect s called tme dilatin (Examples

)

=

 

1

S ight() � = " � /S'' - uL l s  /S us"!s !s   100  mls  = 



� 



V - =2: 2:/

37137.3)

Length contraction If two points are at rest in a partic lar frame of reference, the dstance L between the points as measured in that frame is caled a proper length f this frame moves with constant velocity u relative o a second frame and the distances are meas



� .

L beween red to the motion, the distance the poinsparallel as measured in the second frame is shorter than  his effect is called length contraction See Exampes 374376) The Lorentz tansformations The orentz coordinae transformations relate the coordinates and time of an event in an inertial frame to to the coordinates and time of the same event as observed in a second nertal frame ' moving at velocity u relative to the rst For one dimensional moton a particles velocities VI in and  in  are related by the orentz velocity transformation See Examples and

377

 x- ut = "(x  ut) VI  U2 U2/C /C22 y' = Y z' = Z t  x/c c ux/ / d t   " ( - ux VI - u u/ /

y

 x' =

?

37.8.

F

r--

.  

_  



 

_

/If

p

=+ \

x O

 ' +  x

 he Doppe effect fo eectromagnetic waves he Doppler effect is he freqency shft in light from a souce due to the relative motion of source and observer For a surce moving toward the observer with speed u, Eq gives the received frequencyf in terms of he emie frequenyf   a. See Example

3725)

f

uf u  



Saionay b b  d ligh  q

u

Moving source emt ligh f fqy

> o· 

1  "0 "0

379.

Reativistic momentum and enegy: enegy: For a particle of rest mass m moving with velocity the reativistic momenum s given by Eq or and the relaivisic kinetic energy K is given by Eq The

p

V, (3727) (373 3736

£ is The total energym the sum the inetic energy and the res energy totaof energy can also be expressed n erms of the magnitde of momentum p and rest mass m. See Exampes 3703712



=

Inv

VI   / /

-

 mv  

K

Relasc kec 1 nergy , :

[

/ ESN  

/   HAPPEN

 

Nwan ki nergy

�o- --  

298  

Answers t Tes Your Undersanding Qesins

199

N mchc  h pcl   h f lvy The special theory of anics ics echan nian   mech  of  Newto  New tonian ciples ples of   pinci s. All the the pin chanic anics. ian   me mech tonian n of New N ewton lizatio ation  genera neraliz ty   s a ge reativity reativi are present as limiting cases when all the speeds are small compared to e. Futher generalizaion to nclude nonnetial frames of reference and heir relationship to gravtatonal elds leads to the gen era theory of relativity

Key Terms

special theory of relativity, 6 principle of reativity 6 Gallean coordinate transformation  simutaneity  event,  time dilaton  poper tme, 6

twin paradox  proper length 0 length contraction 0 Lorentz transformaions,  spacetime  spacetime coordnates  rest mass, 

Answe to Chapte Opening Question

? .

o. Whie the speed of light c s the utimate "speed limit for any partce, there is no upper limit on a particle's kinetic energy (see Fig 3721). As the speed approaches e a small increase in speed coresponds to a large increase in kinetic energy

Answes to est ou Understanding Questions 37 :    

You too wil measre a sphercal wave front that epands at the same speed e n all diectons. This is a consequence of Einsteins second postulate he wave front that you measure is no centered on the current position of the spaceship; rather it is centered on the point P where the spaceship was located at the instant that it emitted the ight pulse For eam ple suppose he spaceshp is moving at speed e/ 2. When yor watch shows that a time I has elapsed since the pse of ligh was emtted your measrements will show that the wave font is a sphere of radis et cenered on P and hat the spaceship s a dis ance e/ 2 from P.

2 :  n Mavss frame of reference the two events

(the gdenville clock striking noon and the North Haverbook clock striking noon) are not sinultaneous. Figure 375 shows tha the event toward the front of the ral car occurs rst. Since the rail car is moving toward North averbrook that clock struck noon before the one on gdenvile. gdenvile. So according to Mavis it is after noon in North Haverbrook 37   33 :     he statement hat moving clocks rn slow refes to any cock that is moving relatve o an observer Maria and her stopwatch are moving relative to Sami, so Samir measures Maias stopwatch to be running slow and o have ticked of fewer seconds than hs own sopwatch Samr and hs topwach ae moving relative to Maria so she likewise meases Samis stopwatch to be runnng slow. Each observer's measuement is cor rect for his or her own frame of refeence BOlh observers conclude that a moving stopwatch runs sow This is consistent with the prin cipe of relativity (see Section 371), which states that the laws of physics are the same in all inertial fames of reference 374 :       You measure the rest length of the stationary meer stick and the contraced length of he oving spaceshp to both be  meter The rest length of the space ship s greate than the contracted ength that you mease and so

a =g

relativistic momentum, 0 total energy  rest energy,  cOIespondene principle 6 general theory of relativty, 6

must be greater than 1 mete. A miniature observer on board the spaceship would measure a contracted length for the meter stick of less than 1 meter. Note that in your rame of reference the nose and tail of the spaceship can simultaneously align with the two ends of he meter stick, since in yor frame of reference they have the same lengh of I meter. n he spaceships frame these two alignments cannot happen simutaneously because he mete stick s shorte han the spaceship Section 372 tells us that this shoudn't be a sur prse; two evens hat ae simultaneos to one obsever may not be simltaneous to a second observer moving relative to the rst one. 3 :  > b 4 a) he last of Eqs. (3721) tels s the times of the two events in : I I ' = YI - ux Je  and 1 2' = Y (  - UX/ e ) . n frame  the two events occur at the same -coordinate so XI  X and event P occurs before event P2 so '  1, Hence you can see that  < 1  and event PI happens before P2 in frame  too hs says that if event P happens before P n a fame of reference  where the two events occur at the same position hen P happens before P2 n any oher fame moving el ative to  (b) n fame 5 the two events occr at deren coordinates such tha 3  X4 and events P3 and P4 occur at he ux))/e ) same time so   14 ence you can see that f) f)''  Y - ux s greater than '  Y  1 - uX/e )  so even P happens befoe P in frame  This says that even though the two events are simuta neous in frame , they need not be simultaneous in a frame moving relative to . 37 7 :  Equation (3727) tels us that the magnitude of momentum of a partice with mass /1 and speed  is  p  V1 - /e. f  inceases by a factor of 2 the nmera to m increases by a factor of 2 and the denominator V - /C decreases Hence  p ncreases by a factor greate than 2. (Note that in ode o doble the speed, the initial speed must be less than e/2 hat's because he speed of light s the ltimate speed limi.) 378 :  As the proton moves a disance  the constant force of magnitude F does work W  Fs and increases the kineic energy by an amount !K    Fs This is true no matter what the speed of the proton before moving this distance hus the con stant force increases the proton's kinetic energy by the same amount during the rst meter of travel as dring any sbsequent meer of travel (ts tre that as the proton approaches the ultmate speed imt of e the increase in the protons peed is less and less with each subseqent meer of travel That's not what the quesion is asking however)

 



CHPTER  Rltivy

PROBLEMS

o d wk   mnphom mnphom

Discussion Questions Q37.1. You are standing on a tran platform watchng a hgh-spee train pass by. A igh insie one o the rain cars s tue on and then a ite later it is rne o a) Who can measre the proper time nterval or the raton o he lght: yo or a passenger on the train? ) Who can measre the proper engh o the train car yo or a passenger on he train? c) Who can measure he proper lengh o a sign atache o a post on the rain platorm, yo or a passen ger on the rain? In each case explain yor answer Q37.2 f simltaneity is no an absolute concept does ha mean tha we mst discard the concep o causality?  event  is to cause even   ms occr rst s i possible that n some rames  appears o be he case o B an in others,  appears to be he cause of ? Explain Q373. A rocket is moving o the rgh at � the spee o light rea ive o he earh A ligh blb in he cener o a room inse he rocket sudenly s on Call the light hiting he ron en o the room event A an the ight hitting the ack o he room event  (Fig 377) Which event occurs rst,  or  or are they simta neous as vewe y a) an asronat riding in he rocke and b) a person a rest on the earth?

Fgr  Qeston Q373

how do massess paricles sch as photons and neurnos acqure his speed? Can't hey sart rom rest an accelerate? Explan Q37.11. he spee o light reaive o stil waer is 225  0 m/s  the waer is moving past us he speed o light we measue depends on the speed o he waer Do hese acts violate Enseins secon posuae? Expain Q3712. hen a monochromatc lgh sorce moves owar an oserver ts wavelength appears to e shorter than the vae meas ured when he sorce s a res Does hs conract the hypohess that the spee o light is he same or al observers? Expan Q33 n prncple does a ho gas have more mass than the same gas when i is cold? Explain n pracice wod hs be a measa le eec? Explain Q314. Why do yo think he deveopmen o Newonan mechan ics preceded the more rened relativistc mechancs by so many years?

xercises ection   Relativity of imutaneity 371 Suppose he two ghtning bots shown n g 375a are simulaneos to an observer on the train Show hat hey are not simulaneous to an observer on the grond hich ightnng srke does the gron observer measre o come rs?

ection   Reatvity of Time Intervas 37.2. he posiive mon (f+, an nstable paricle lives on aver

speed o light were J 0 m /s instead o 3.00  08 m/s?

age 2.20  0-6 s measre in is own rame o reerence) eore decayng a)  such a partcle s moving wth respec to the labo ratory with a speed of 0.900, what average ietme is measured n the laboraory? b) What average dstance measre n he abo raory oes the paice move beore ecayng? 373 How ast ms a rocket trave relaive to the earh so that me in the rocket "slows down to half is rae as measure by earth-based oservers? Do presen-day jet planes approach sch speeds?

Q37S. The average ife span in the Unied Sates is abou 70 years

374 A spaceship ies past Mars with a spee o 095c reave o

Q374 Wha o you hink would be erent in everyay lie i he

Does this mean that t is mpossible or an average person to travel a isance greater than 70 ighyears away rom the earh? A lightyear s the disance lght ravels n a year) Expan Q376. Yo are holding an eiptcal servng plater. How woud you nee to travel or the serving platter to appear rond to anoher observer? Q37.7 wo events occur at he same space pont n a paricuar inerial rame o reerence and are simltaneos n that frame s i possble ha hey may no be smulaneos n a eren nera rame? Explain Q37.8. A hgh-spee train passes a train platorm Larry s a pas senger on he train Aam s sanding on the train platorm an Davd s rng a bicyce towar he plaorm n he same directon as the train is travelng Compare the ength o a rain car as meas ure by Larry Aam and David Q39 he heory o relativiy sets an upper limit on the speed ha a paricle can have Are there aso lmits on the energy and momentum o a paricle? Expain Q37.0 A studen asserts that a material particle ms aways have a speed sower han ha o light an a massess particle ms aways move a exacly the speed of ight s she correc?  so

he srace o the panet When he spaceship is rectly overhea a signal light on the Maran srace blnks on and then o An observer on Mars measres that the signal ligh was on or 75 0 fS a) Does the observer on Mars or he pilo on he spaceshp meas ure the proper tme? b) What is the raion o the ligh plse measre by the plo o he spaceship? 37.5 he negaive pion ( 7- ) is an nsae parice with an aver age letime of 260  0- s measred in the rest frame o the pon a) I he pon s mae o rave a very hh speed reave o a laboratory its average lieime is measure in he aoraory to be 4.20 X 0 s Caclate he speed o he pion expressed as a fraction o c. b) Wha distance, measre in the laoraory does the pon rave drng ts average ifeime? 376 As yo pilot yor space tlity vehcle at a constant speed oward he moon, a race pio ies past you n her spaceracer at a constant spee o 000c relatve o you. A the nstant the space racer passes you boh o yo sar imers a zero a) A he nsan when yo measre that the spaceracer has traveled 1 0  0 m pas you wha does he race plo read on her timer? b) When he race pilot reas he vae caclated in part a) on her mer wha oes she measre to be yor disance rom her? c) A he instant

 



Exercises when the race pilot reads the value calculated n part (a) on her timer, what do you read on yours? 377 A spacecraft ies away from the eath with a speed of 4.S0 X 106 m/s relative to the earth and then returns at the same speed. The spacecraft carries an atomc cock that has been care fully synchronized with an identical clock that remains at rest on eah The spacecraft returns to its startng point 35 days (l year) later as measured by the clock that remaned on earth. What s the dierence n the elapsed times on the two clocks measured in hours? Which clock the one in the spacecraft or the one on earth shows the shorest elapsed time? 378 An alien spacecraft is ying overhead at a great distance as you stand in your backyard You see its searchight bnk on for 0190 s The rst ofcer on the spacecraft measures that the searchlght is on for 12.0 ms (a) Which of these two measured times is the proper time? (b) What is the speed of the spacecraft relative to the earh expressed as a fraction of the speed of light ?

runway as measured by a pilot of a spacecraft ying past at a speed of 4.00 X 10 m / s relative to the earth? (b) An observer on earth measures the time interval from when the spacecraft is directly over one end of the runway until t is directy over the other end What result does she get? (c) he piot of the spacecraft measures the time it takes hm to travel from one end of the nway to the other end What vaue does he get?

Seco   The orez rasfomao  (37.21) Solve Eqs to obtan  and in terms of and t 34show that the resulting transformationt has the sameform as and the original one except for a change of sgn for  3715 An observer in frame S' is movng to the right + direction) at speed  0.00e away from a stationary observer in frame S. The observer n S measures the speed ' of a paricle movng to the right away from her. What speed v does the observer n 0400c; (b) ' 0900e S measure for the partice if (a) ' 0990e? (c) ' 36 Space piot Mavis zips past Stanley at a constant speed rea tive to him of O.SOOe. Mavis and Staney start timers at zero when the front of Mavis's shp s directly above Stanley When Mavis reads 500 s on her timer, she turns on a brght light under the front of her spaceship (a) Use the orentz coordnate transformation derived in Exercise 37.14 and Example 377 to calcuate  and  as measured by Stanley for the event of turnng on the light (b) se 







Seco  Relavy of Legh 379 A spacecraft of the rade Federation ies past the planet Cor uscant at a speed of 0.00e. A scientist on Coruscant measures the length of the moving spacecraf to be 740 m he spacecraft ater lands on Coruscant, and the same scentist measures the ength of the now stationary spacecraft What value does she get? 3710 A meter stick moves past you at great speed Its motion rela tve to you is paallel to its long axis If you measure the ength of 0304S m ) -for the movng meter stck to be .00 f (  ft example by comparing comparing it to t o a foot ruer that is at rest relatve to you-at what speed is the meter stick moving reative to you? 37 Why A A W Bombadd by Muon? Muons are unsta ble subatomic partcles that decay to electrons with a mean ife time of 2.2 J hey are produced when cosmic rays bombard the upper atmosphere about 10 k above the earth's surface, and they travel very cose to the speed of lght The probem we want to address s why we see any of them at the earths suface (a) What s the greatest distance a mon could travel durng ts 2.2Js lifetme? (b) Accordng to you answer n pa (a) t would seem that muons could never make it to the ground But the 2.2-Js lifetme is measured n the frame of the muon and muons are mov ng very fast At a speed of 0.99ge. what s the mean ifetime of a 

muon by an observer rest this on the eah? Howwhy far would as themeasured muon trave in this tme?atDoes result explain we nd muons n cosmic rays? (c) From the pont of view of the muon, it still Lives for ony 22 , so how does t make it to the ground? What s the thckness of the 0 km of atmosphere through which the muon must trave, as measured by the muon? t is now clear how the muon is able to reach the ground? 37 An unstabe pacle s created in the upper atmosphere from a cosmic ray and travels straight down toward the surface of the earh with a speed of 0.99540c relatve to the earth. A scientist at rest on the earths suface measures that the partcle is created at an altitude of 45.0 km (a) As measured by the scientist, how much tme does it take the partice to travel the 45.0 k to the surface of the earth? (b) Use the lengthcontraction formula to caculate the distance from where the partice is created to the surface of the earth as measured n the particle's frame (c) n the pacles frame how much time does it take the patice to travel from where it is created to the suface of the earth? Calculate this time both by the time dilation fomula and from the dstance calcuated n part (b) o the two results agree? 373 As measured by an observer on the earth, a spacecraft run way on earth has a length of 300 m (a) What is the ength of the

the time diation formula, Eq (37 to calculate the time inerval between the two events (the front of the spaceship passing over head and turning on the light) as measured by Stanley. Compare to the vaue of t you calcuated in par (a) (c) Multipy the time inter val by Mavis's speed both as measured by Stanley to calcuate the dstance she has traveled as measured by hm when the light turns on Compare to the value of  you calculated in part (a) 3717 A pursuit spacecraf from the planet Tatoone is attempting to catch up with a rade Federation cruiser As measured by an observer on Tatoone, the cruiser is traveing away from the planet with a speed of 000e. he pursuit shp s traveng at a speed of O.SOOe relative to atooine in the same direction as the cruiser. (a) For the pursuit ship to catch the cruiser, shoud the speed of the cruiser relative to the pursuit shp be positve or negative? (b) What is the speed of the cruiser relative to the pursuit ship? givesvelocity the transformaton for only the 378 Equaton 3723 component of an objects Suppose the obect consid ered in the derivation also moved n the /direction Find an expression for uy in terms of the components of , , and e, which represents the transformation for the component of the velocty (Hint: Apply the orentz transformatons and relationships ike Ux dxd, ; cL'dt', and so on, to the components) 3719 Two paices are created n a highenergy accelerator and move o in opposite directions The speed of one particle, as measured n the aboratory, is 050e, and the speed of each pat ce reative to the other is 0950c What s the speed of the second particle, as measured n the aboatory? 370 Two particles in a highenergy accelerator experiment are approachng each other headon each with a speed of 0.9520e as measured in the laboratory What is the magnitude of the veocity of one partcle reative to the other? 37 Two partcles in a hghenergy accelerator experiment approach each other headon with a relative speed of 0.S90e Both patcles travel at the same speed as measured in the laboatory. What is the spd of each partcle as measured n th laboratory? 37 An enemy spaceship is movng toward your starghter with a speed, as measured in your frame, of 0400e The enemy ship =



 

102

CHAPTR 37 Rv

res a missile toward you at a speed of 0.700 eative to the enemy shp (Fig. 3728) (a) What is the speed of the missie ea tive to you? Express your answer in terms of the speed of Light. (b) If you measure that the enemy ship s 8.00  106 an away rom you when the missie is red, how much time, measured in your frame, w it take the missie to reach you? iure      Exercise 3722

Em

�

Stfht

 An imperia spaceship, moving at hig speed reative to the panet Arrakis, res a rocket toward the panet with a speed of 0.920 eatve to the spaceship. An observer on Arakis measures ha te rocket is approaching wit a speed of 0.30. What is the speed of the spaceship reative to Aakis? s the spaceshp moving owad or away from Arrakis?

*Secton 6 The Doppler Eect fo Electomagnetc Waves *4 Rewrte Eq. 3.25 to nd the reative veocity it between

the source observer in termsofof igt the ratio of the eectromagnetic observed frequency andand theansource frequency What reative veocity  wi produce (a) a 5.0% decrease in frequency and (b) an ncease by a factor of 5 of te obseved ight? *5 Tel It to the Judge (a) How fast must you be approac ng a red trafc ight  = 75 nm for it to appea ap pea yeow  = 575 nm? Express your answer in terms of te speed of ight (b) If you used this as a reason not to get a ticket for running a red ght, how much of a ne woud yo get for speeding? Assume that the ne is $100 fo each komeer per hou that you speed exceeds the posed imit of 90 /h * Sow that when the source of eectromagnetic waves moves away from us at 0.00, the frequency we measure is haf he vaue measured n the rest frame of the source Section Relatvstic Momentum  (a) A partice wit mass m moves aong a straight ine under the acton of a force F directed aong the same ine. Evauate the deivative in Eq. (3.29) to show that the acceeration a  dv/dt of the parice is given by a  / (I v2/ ) 3 (b) Evauate the deivative in Eq (37.29) to nd the expression fo the magni tude of the acceeration n terms of F, m, and / if the force is per pendicuar to the veocity.  When Should you Use Reativiy? As you have seen, reativistic cacuatons usuay invove te quantty y. Wen y is apprecaby greater than 1 we must use eativistic formuas instead of Newtonian ones. Fo what speed v (in terms of ) is the vaue of y (a) 10% greater than I; (b) 10% greater than I (c) 00% greater than ? 9 (a) At what speed s the momentum of a partice twice as great as the resut obtained from the nonreativistic expression ? Express your answer in terms of the speed of ight. (b) A force is appied to a partice aong its diection of motion. At wat speed is the magnitude of force required to produce a given acceeration twice as great as the foce required to produce the same acceera tion when he partice is at rest? Express you answer n tems of e speed of ght. -

 Relativistic Baseball. Cacuae he magntude of the

force required to give a 0145-kg basea an acceeration a = 1.00 m/s in the directon of the baseba's initia veocity when ths veocity has a magnitude of (a) 100 m/s; (b) 0.900 (c) 0.990 (d) Repeat parts (a), (b), and (c) if the force and acce eration are perpendicua to the veocity Secton 8 Reatvstc Wok and Enegy  What is the speed of a partce whose kinetc energy is equa to (a) its est energy and (b) ve times its rest energy?  Annihilation In potonaniproton annihation a proton and an aniproton (a negatvey charged proton) colide and disap pear, producing eectromagnetic radiation. If each partice has a mass of 1.7  10 kg and they are at rest just before the annhi ation nd the tota energy of the radiation Give you answers in oues and in eectron vots.  A proton (rest mass   O kg has tota energy that is .00 times ts rest energy. What are (a) the kinetc energy of te proton (b) the magnitude of the momentum of the poton (c) the speed of the proton? 4 (a) How much work must be done on a partice with mass  to accelerae it (a) fom rest to a speed of 0090 and (b) fom a speed of 0900 to a speed of 0990? (Express the answers in terms of .) (c) How do your answers in parts (a) and (b)

compare? 5 (a) By wha percentage does your rest mass increase when you cimb 30 m to the top of a tenstory buiding? Are you aware of this ncease? Expain (b) By how many grams does te mass of a 2.0g sping with force constant 200 N/cm change wen you compress it by .0 cm? Does the mass incease o decrease? Woud you notice the change in mass if you wee hoding the spring? Expain.  A 0.0kg person is standing a res on eve ground. How fast woud she have to rn to (a) doube he ota energy and (b) increase her tota energy by a factor of O?  An Antimatter Reacto When a partice meets its antipatice, they annihiate each other and their mass is converted to ight energy Te Unied States uses approximatey 1.0 X 10 ] of energy pe year. (a) If a ths energy came from a fuurstic anti matte reactor, how much mass of matter and antimatte fue woud be consumed yeary? (b)  this fue had the density of iron 7.8 g/cm and were stacked in bricks to form a cubica pie, how high woud it be? (Before you get your hopes up antimatter eactos ae a log way in the futuref they ever wi be feasibe)  A J ("psi) patce has mass 5.52  0 kg. Compe the rest enegy of the  patice in MeY 9 A patice has rest mass 4  0 kg and momentum 210  10 10 18 kg  m/s (a) What is te tota energy (kinetic pus est enegy) of te partice? (b) Wha s the kinetic energy of the partice? (c) What s te ratio of he knetc energy to e ret energy of te partice? 4 Starting from Eq (3.39), sow that in te cassica imit pc 1C) the energy approaces the cassica kinetic energy !mv pus te rest mass enegy . 4 Compue the kinetic enegy of a proton (mass 17  10 kg using both the nonreativisic and eativistic expres sions, and compute the ratio of the two resuts (reativistic dvded by nonreativisic) for speeds of (a) 8.00  10 m/s and (b) 2.85  0 m/s. 4 What is the kinetic energy of a proton moving at (a) 0100 (b) 0.500 (c) 0.900? How muc work must be done o (d) increase

 

 a nd e) inease the pro the proton's speed fom 000c to 0.500c and ons speed from 0500c to 0900? f How do the last two esults ompare to results obtaned in the nonelativsti imit? 4 a) Though what potentia dfeene does doe s an eletron eletron have to be aelerated, starting from rest to ahieve a speed s peed of 0980c? b) What is the kineti energy of the eletron at this speed? Express your answe in joules and in eletron vots   44  44 Creating a Particle. wo protons eah with rest mass M = 67  0- kg are initialy moving with equa speeds in opposite heanpotons ontinue exist after a oll  patile son that dietions aso produes see to Chapter 44). he est  mass of the  is m = 9.5 X 0 kg a)  the two protons and the To are al at rest after the olision, nd the nitia speed of the protons, expressed as a fraton of the speed of ight b) What is he kneti energy of eah proton? Expess Ex pess you answer in Me. ) What is the rest enegy of the , expessed in MeV? d) Disuss the reationship re ationship between the answers to parts b) and ). 45 Find the speed of a patile whose relatvsti relatvsti kinei energy is 50% geate than the Newtonian vaue va ue for the same speed 46 Energy of Fusion. In a hypothetal nuear fuson ea to, two deuterium nuei ombine or "fuse to form one heium nueus The mass of a deuterum nuleus expressed n ato mass unts u), s 20136 u; the mass of a helium h elium nuleus s 4005 u  u = .6605402  0 kg. kg . a) How muh energy energy s reeased when 0 kg of deuterim undergoes fusion? b) he annual onsumption of eletia enegy in the United States is of the order of 0  0 J. How muh deuterum must eat to pro due ths muh energy? 4 The sun produes energy by nuea fuson reations n whih matte s onverted into energy By measurng the amount of enegy we eeive fom the sun we kow that it is podung enegy at a rate of 38  0 W. a) a ) How many kiogams of mat ter does the sun ose eah seond? Approximatey how many tons of matter is this? b) At this rate, how ong would it take the sun to use up al its mass? 48 A O.OOg O.OO g spek of dust dus t is aeerated from est to a speed of 0900 by a onstant 00  0 N fore. a) If the noneativis ti fom of Newtons seond law 2F = a is used how fa does the objet tave to reah its nal speed? b) Using the oret rela tvsti teatmen t of Setion 37.8distane how farisdoes the objet reah itsteatment na speed? ) Whih geater? Why? tavel to

Probles   4  4 Ater being produed in a olision between elementary pa pa tiles, a positive pion (7+ must trave down a 20kmong tube to eah an expeimental aea. A 7  patle has an aveage ife time measued in its rest frame) of 260  0- s the 7+ we ae onsidering has this fetime a) How fast must the + travel f it is not to deay before it eahes the end of the tube? Sine u wll be very ose to c, write u = (1 - D)c and give you answe in terms of  rather than u) b) The 7 + has a rest enegy of 39.6 MeV. What is the total energy of the 7+ at the speed alu lated in part a)? 50 A ube ube of metal wth sides of length a sits at rest in a rame S wth one edge paael to the axis heefore in S the ube has volume 3 Fame S' moves along the axis with a speed u. As measued by an obsever in frame S what is the voume of the metal ube? 51 The staships of the Solar Federation are marked with the symbol of the fedeation, a irle, while starships of the

303

enebian Empire ae maked wth the empies symbol an eipse whose major axis is 40 times longer than its mino axs (  140 in Fg 3.29) How fast eatve to an observe does an empre ship have to travel for its markng to be onfused wth the marking of a federation shp? =

Figure 3729 Problem 375

datn

Emp

5 A spae probe is sent to the viinity of the star Capea,

whih is 422 ightyears from the earth A lightyear is the dis tane light travels in a year) he pobe travels with a speed o 099O An astronaut reruit on board is 9 years old when the probe leaves the eath. What is her bioogial age when the probe reahes Capela? 5 A partile partile is said to be xtLy Lativitic when its kineti energy is muh greater than its rest energ energy. y. a) What is the speed of a partile expressed as a fraton of c) suh that the tota enegy  ten tmes the rest energy? b) hat s the perentage diferene between the eft and right sides of Eq 3.39) if c s neg eted for a partile partile with the speed alulated in part a)? 54 Everyday Time Dilation. wo atomi oks are are fuy synhronized ne remains in New York, and the other s oaded on an airiner that tavels at an average speed of 250 m/ and then etus to New York When the pane p ane returns the eapsed time on the ok that stayed behind is 400 h By how muh wi the readings of the two oks dier and whih lok wil show the shorer elapsed time? Hint: Sine u , you an simplify V - U2/ C2 by a binomia b inomia expansion.) 55 he Large Hadron Collider (LHC) Physiists and engineers fom aound the world have ome together to build the argest aeerator in the world, the Large Hadron Coider HC) at the CERN aboratoy in Geneva, Switzerland S witzerland The mahine wi aeleate protons to kneti energes of 7 eV n an undergound ng 27 on kmthe n HC, rumferene Fo the latest newsspeed and moe  willnfor mation visit www.ern.h) a) What pro tons reah in the LHC? Sine u is very ose to , write u =  - c and give you answer in terms of . b) Find the relativisti mass, , of the aeleated protons in tems of ther rest mass 56 A nuea bomb ontainng 800 kg of plutonium explodes The sum of the rest masses of the produts of the exposon is ess than the ogina ogina rest mass by one part in 10 a) ow muh energy s eeased in the exploson? b) f the exploson takes plae n 400 s, what is the average power developed by the bomb? (c) What mass of wae oud the eleased enegy ift o  o a heiht heiht o 1.00 k? 5 erenkov Radiation. The Russian physist P A erenkov disoveed that a haged partle traveing in a soid with a speed exeedng the speed of light in that materal adiates eletomag neti adation his is anaogous to the soni boom produed by an airaft moving faster than the speed of sound in a see Setion 69. erenkov shared the 958 Nobel Pize fo this dis overy) What is the minmum kneti energy in eletron volts) that an eletron must have whie traveling nside a slab of rown gass ( n 52 n order to reate this eenkov radiation? 

View more...

Comments

Copyright ©2017 KUPDF Inc.
SUPPORT KUPDF