Using equations (2-20), show that

y'u=(1-uxvc2)yv,yu

Short Answer

Expert verified

The required equation γu=1-uxvc2γgγvis obtained.

Step by step solution

01

Write the given data from the question

The equation 2.20 is given as,

ux'=ux-v1-uxvc2uy'=uyγv1-uxvc2uz'=uzγv1-uxvc2

02

Determine the equation to prove the equation

The expression to calculate the velocity transformation for velocity of object in direction is given as follows.

u'x=ux-v1-uxvc2 ...(i)

Here, is the velocity component in the x direction,v is the velocity of frame S'relative to S, and c is the velocity of the light.

The expression to calculate the velocity transformation for velocity of object iny direction is given as follows.

uy'=uyγv(1-uxvc2) ...(ii)

The expression to calculate the velocity transformation for velocity of object in z

direction is given as follows.

uz'=1γv(1-uxvc2) ...(iii)

03

Prove the equation γu'=(1-uxvc2)γvγu.

The Lorentz factor is written out for the velocity u'as,

γu'=11-u'c2γv'=11-u'c22

The velocityu'2is expand as,

γu'=11-ux'2+uy'2+uz'2c2γu'=11-1c2ux'2+uy'2+uz'2

Substitute ux-v1-uxVc2for ux', uyγv1-uxVc2for u'yand uzγv(1-uxVc2for uz'into above equation.

γu'=11-1c2ux-v1-uxvc22+uyγv1-uxvc22+uzγv1-uxvc22γu'=11-1c2ux-v21-uxvc22+uy2λv21-uxvc22+uy2λv21-uxvc22

Multiply by γv2in the ux'part to simplify the above equation,

role="math" localid="1659332643154" γu'=11-1c2γv2ux-v2γv21-ux-vc22+uy2γv21-ux-vc22+uz2γv21-ux-vc22γu'=11-1c2γv2ux-v2+uy2+uz2γv21-uxvc22γu'=11-γv2ux-v2+uy2+uz2c2γv21-uxvc22γu'=1c2γv21-uxvc22-γv2ux-v2+uy2+uz2c2γv21-uxvc22

Solve further as,

γu'=11γv1-uxvc2c2γv21-uxvc22γv2ux-v2+uy2+uz2c2γu'=γv1-uxvc2c2γv21-uxvc22-γv2ux-v2+uy2+uz2c2γu'=γv1-uxvc2c2γv21+u2xv2c4-2uxvc2-γv2u2x+v2-2uxv+uy2+uz2c2γu'=γv1-uxvc2γv2c21+u2xv2c4-2uxvc-u2x+v2-2uxvc2

Solve further as,

γu'=γu1-uxvc2γv2c2+ux2v2c2-2uxv-ux2-v2+2uxv-uy2-uz2c2γu'=γu1-uxvc2γv2c2+ux2v2c2-u2xv2-uy2-uz2c2γu'=γu1-uxvc2γv2c2-v2+ux2v2c2-1-uy2-uz2c2γu'=γv1-uxvc2γv2c2-v2-yv2ux21-v2c2-uy2-uz2c2

Solve further as,

γu'=γv1-uxvc2c2yv21-v2c2-yv2ux21-v2c2uy2-uz2c2

Substitute 11-v/c2for γvinto above equation.

γu'=γv1-uxvc2c211-vc221-v2c2-11-vc22ux21-v2c2-uy2-uz2c2γu'=γv1-uxvc2c21-v2c2-ux21-v2c21-vc2-uy2-uz2c2γu'=γv1-uxvc2c2-ux2+uy2+uz2c2γu'=γv1-uxvc2c2-ux2+uy2+uz2c2

Substituteux2+uy2+uz2for u2into above equation.

γu'=γv1-uxvc2c2-u2c2γu'=γv1-uxvc21-u2c2

The root mean is equal to Lorentz factor for the velocityu through,

γu'=γv1-uxvc2γuγu'=1-uxvc2γuγv

Hence the required equationγu'=1-uxvc2γuγv is obtained.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

A projectile is a distance r from the center of a heavenly body and is heading directly away. Classically, if the sum of its kinetic and potential energies is positive, it will escape the gravitational pull of the body, but if negative, it cannot escape. Now imagine that the projectile is a pulse of light energy E. Since light has no internal energy ,E is also the kinetic energy of the light pulse. Suppose that the gravitational potential energy of the light pulse is given by Newton’s classical formula U=-(GMm/r), where M is the mass of the heavenly body and m is an “effective mass” of the light pulse. Assume that this effective mass is given by m=E/c2.

Show that the critical radius for which light could not escape the gravitational pull of a heavenly body is within a factor of 2 of the Schwarzschild radius given in the chapter. (This kind of “semiclassical” approach to general relativity is sometimes useful but always vague. To be reliable, predictions must be based from beginning to end on the logical, but unfortunately complex, fundamental equations of general relativity.)

Explain to your friend, who is willing to accept that light moves at the same speed in any frame, why clocks on a passing train are not synchronized. If it helps, assume that Anna is at the middle of the train.

Exercise 117 Gives the speed u of an object accelerated under a constant force. Show that the distance it travels is given byx=mc2F1+Ftmc2-1.

For reasons having to do with quantum mechanics. a given kind of atom can emit only certain wavelengths of light. These spectral lines serve as a " fingerprint." For instance, hydrogen's only visible spectral lines are656, 486,434,and410nm . If spectra/ lines were ofabsolutely precise wavelength. they would be very difficult to discern. Fortunately, two factors broaden them: the uncertainty principle (discussed in Chapter 4) and Doppler broadening. Atoms in a gas are in motion, so some light will arrive that was emitted by atoms moving toward the observer and some from atoms moving away. Thus. the light reaching the observer will Cover a range ofwavelengths. (a) Making the assumption that atoms move no foster than their rms speed-given by ,vrms=2KBT/m whereKB is the Boltzmann constant. Obtain a formula for the range of wavelengths in terms of the wavelengthλ of the spectral line, the atomic massm , and the temperatureT. (Note: .vrms<<c) (b) Evaluate this range for the656nm hydrogen spectral line, assuming a temperature of5×104K .

In Example 2.5, we noted that Anna could go wherever she wished in as little time as desired by going fast enough to length-contract the distance to an arbitrarily small value. This overlooks a physiological limitation. Accelerations greater than about 30g are fatal, and there are serious concerns about the effects of prolonged accelerations greater than 1g. Here we see how far a person could go under a constant acceleration of 1g, producing a comfortable artificial gravity.

(a) Though traveller Anna accelerates, Bob, being on near-inertial Earth, is a reliable observer and will see less time go by on Anna's clock (dt') than on his own (dt). Thus,, whereuis Anna's instantaneous speed relative to Bob. Using the result of Exercise 117(c), withgreplacingF/m, substitute for u, then integrate to show that

(b) How much time goes by for observers on Earth as they “see” Anna age 20 years?

(c) Using the result of Exercise 119, show that when Anna has aged a timet’, she is a distance from Earth (according to Earth observers) of

(d) If Anna accelerates away from Earth while aging 20 years and then slows to a stop while aging another 20. How far away from Earth will she end up and how much time will have passed on Earth?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free