Consider a particle in hyperbolic motion,

x(t)=b2+(ct)2,y=z=0

(a) Find the proper time role="math" localid="1654682576730" τas a function of τ, assuming the clocks are set so thatτ=0 whenτ=0 . [Hint: Integrate Eq. 12.37.]

(b) Find x and v (ordinary velocity) as functions ofτ .

(c) Findημ (proper velocity) as a function of τ.

Short Answer

Expert verified

(a) The proper time as a function of tis τ=bcInc+b2c2t2b.

(b) The x and v (ordinary velocity) as a function of τis role="math" localid="1654683130022" x=bcoshcτbandrole="math" localid="1654683078037" v=ctanhcτb respectively.

(c) The x and v (ordinary velocity) as a function of τis x=bcoshcτband v=ctanhcτbrespectively.

Step by step solution

01

Expression for the Lorentz contraction:

Write the expression for the Lorentz contraction.

Y=11-v2c2 …… (1)

Here, v is the velocity, and c is the speed of light.

02

Determine the proper time τ as a function of t:

(a)

Write the expression for the velocity of a particle.

v=dx(t)dt

Substitute b2+c2t2for x(t)in the above expression.

localid="1654683753767" v=ddtb2+c2t2v=12b2+c2t2ddtb2+c2t2v=12b2+c2t22c2tv=c2tb2+c2t2

Squaring on both sides in equation (1).

γ2=11-v2c22γ2=11-v2c2

Substitute c2tb2+c2t2 for v in the above expression.

localid="1654687319733" γ2=11-c2tb2+c2t22c2γ2=11-c4t2b2+c2t2×1c2γ2=11-c2t2b2+c2t2γ2=b2+c2t2b2

Write the relation between proper time and the time interval.

dτ=1-v2c2dt

Integrate the proper time dτ.

localid="1654685358421" dτ=τ=1-v2c2dtτ=1-v2c2dt

Substitute 1-v2c2=1γ2and γ2=b2+c2t2b2in the above expression.

localid="1654685793217" τ=1γ2dt=1b2+c2t2b2dt=b2b2+c2t2dt=bb2+c2t2dt

To further solve the integration,

τ=bcInct+b2+c2t2+k …… (2)

It is given that:

τ=0then t=0

Solve as,

τ=bcInc0+b2+c202+k0=bcInb+kk=-bcInb

Substitute -bcInb fork in equation (2).

τ=bcInct+b2+c2t2-bcIn(b)τ=bcInc+b2+c2t2b

Therefore, the proper time as a function of tis τ=bcInc+b2+c2t2b.

03

Determine the x and v (ordinary velocity) as a function of τ:

(b)

Write the equation for the x ordinary velocity as a function of τ.

x2-b2+x=becτbx2-b2=becτb-x

Squaring on both sides in the above expression.

x2-b22=becτb-x2x2-b2=b2e2cτb+x2-2xbe2cτb2xbe2cτb=b21+e2cτbx=b221+e2cτbbe2cτb

On further solving,

x=b21+e2cτbe2cτbx=be-cτb+ecτb2x=bcoshcτb

As it is kown that:

v=c2tb2+c2t2v=cxx2-b2

Substitute bcoshcτbfor x in the above expression.

v=cbcoshcτbbcoshcτb2-b2=ccosh2cτb-1coshcτb=csinhcτbcoshcτb=ctanhcτb

Therefore, the x and v (ordinary velocity) as a function of τis x=bcoshcτband v=ctanhcτbrepectively.

04

Determine ημ (proper velocity) as a function of τ:

(c)

It is known that:

ημ=γc,v,0,0

Substitute b2+c2t2bfor γand ctanhcτbfor v in the above equation.

ημ=b2+c2t2bc,ctanhcτb,0,0ημ=xbc,ctanhcτb,0,0ημ=bcoshcτbbc,ctanhcτb,0,0ημ=ccoshcτb,sincτb,0,0

Therefore, the proper velocity ημas a function of τis

ημ=ccoshcτb,sincτb,0,0.

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

In the past, most experiments in particle physics involved stationary targets: one particle (usually a proton or an electron) was accelerated to a high energy E, and collided with a target particle at rest (Fig. 12.29a). Far higher relative energies are obtainable (with the same accelerator) if you accelerate both particles to energy E, and fire them at each other (Fig. 12.29b). Classically, the energy E¯of one particle, relative to the other, is just 4E(why?) . . . not much of a gain (only a factor of 4). But relativistically the gain can be enormous. Assuming the two particles have the same mass, m, show that

E=2E2mc2=mc2 (12.58)

FIGURE 12.29

Suppose you use protons (mc2=1GeV)with E=30GeV. What Edo you get? What multiple of E does this amount to? (1GeV=109electronvolts)[Because of this relativistic enhancement, most modern elementary particle experiments involve colliding beams, instead of fixed targets.]

(a) Show that (EB)is relativistically invariant.

(b) Show that (E2-c2B2)is relativistically invariant.

(c) Suppose that in one inertial systemB=0but E0(at some point P). Is it possible to find another system in which the electric field is zero atP?

An ideal magnetic dipole moment m is located at the origin of an inertial system S¯ that moves with speed v in the x direction with respect to inertial system S. InS¯ the vector potential is

A¯=μ04πm¯×r^¯r¯2

(Eq. 5.85), and the scalar potentialV¯ is zero.

(a) Find the scalar potential V in S.

(b) In the nonrelativistic limit, show that the scalar potential in S is that of an ideal electric dipole of magnitude

p=v×mc2

located atO¯ .

A particle of mass m collides elastically with an identical particle at rest. Classically, the outgoing trajectories always make an angle of 90°. Calculate this angle relativistically, in terms ofϕ , the scattering angle, and v, the speed, in the center-of-momentum frame.

Show that the potential representation (Eq. 12.133) automatically satisfies [Suggestion: Use Prob. 12.54.]

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