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Find x as a function of t for motion starting from rest at the origin under the influence of a constant Minkowski force in the x direction. Leave your answer in implicit form (t as a function of x).[Answer:

2ktmc=[Zz2+1Inz+z2+1],where2kxmc2

Short Answer

Expert verified

The value of x as a function of t is 2ktmc=[(Z)z2+1In[z+z2+1]]

Step by step solution

01

Expression for the momentum:

Write the expression for the momentum

p=mu1-u2c2

Here, m is the mass, u is the velocity, and c is the speed of light.

02

Determine the relationship between angular frequency and mass:

As the force is always equal to the rate of change of momentum, write the required equation.

dpdt=kdpdtdt=k......(1)Here,dt=11-u2c2substitute11-u2c2fordtandmu1-u2c2forpinequation(1).ddt11-u2c2mu1-u2c2ddtu1-u2c2=k1-u2c2mmultiplyby1ufordtdxonL.H.Sintheaboveequation.dtdxddtu1-u2c2=k1-u2c2mddxu1-u2c2=k1-u2c2m.......(2)Letω=u1-u2c2substituteu1-u2c2forωinequation(2).ddxω=kuωmωdx=km122dx=km2dx=2kmonfuthersolving,2=2kmdx2=2kmdxω2=2kmx+constant.........(3)

03

Determine the value of x as a function of t:

At the time t = 0, as the constant value is zero, the equation (3).

w2=2Kmx

On further solving the above equation,

u21-u2c2=2Kmxu2=2Kmx-2Kxu2mc2u21+2Kxmc2=2Kxmu2=2Kxm1+2Kxmc2

Again on further solving,

u2=c21+mc22Kxu=c1+mc22Kx

It is known that:

dxdt=c1+mc22Kx

Integrate the above equation.

dxdt=c1+mc22Kxct=1+mc22Kxdx

Let mc2K=b2

Hence, the above equation becomes,

ct=1+b2xdx …… (4)

Let’s assume,

ct=1+b2xdx

Substitute 2ydy for dx and y2for x in equation (4).

ct=1+b2y22ydyct=y2+b2y2ydyct=2y2+b2dyct=yy2+b2+b2lny+y2+b2+constant …… (5)

ct=b2zz2+1lnz+z2+1actmc2K=zz2+1lnz+z2+12Ktmc=zz2+1lnz+z2+1

Therefore, the value of x as a function of tis .2Ktmc=zz2+1lnz+z2+1

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Most popular questions from this chapter

(a) Repeat Prob. 12.2 (a) using the (incorrect) definition p=mu, but with the (correct) Einstein velocity addition rule. Notice that if momentum (so defined) is conserved in S, it is not conserved inlocalid="1654750932476" S. Assume all motion is along the x axis.

(b) Now do the same using the correct definition,localid="1654750939709" p=mη . Notice that if momentum (so defined) is conserved in S, it is automatically also conserved inlocalid="1654750943454" S. [Hint: Use Eq. 12.43 to transform the proper velocity.] What must you assume about relativistic energy?

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) Construct a tensor Dμυ(analogous to Fμυ) out of Dand H. Use it to express Maxwell's equations inside matter in terms of the free current density Jfμ.

(b) Construct the dual tensor Hμυ(analogous to Gμυ)

(c) Minkowski proposed the relativistic constitutive relations for linear media:

Dμυηυ=c2εFμυηυ andHμυηυ=1μGμυηυ

Where εis the proper permittivity, μis the proper permeability, andηυ is the 4-velocity of the material. Show that Minkowski's formulas reproduce Eqs. 4.32 and 6.31, when the material is at rest.

(d) Work out the formulas relating D and H to E and B for a medium moving with (ordinary) velocity u.

Recall that a covariant 4-vector is obtained from a contravariant one by changing the sign of the zeroth component. The same goes for tensors: When you “lower an index” to make it covariant, you change the sign if that index is zero. Compute the tensor invariants

FμvFμv,GμvGμvandFμvGμv

in terms of E and B. Compare Prob. 12.47.

12.46 Two charges, ±q, are on parallel trajectories a distance apart, moving with equal speeds in opposite directions. We’re interested in the force on+q due to-q at the instant they cross (Fig. 12.42). Fill in the following table, doing all the consistency checks you can think of as you go alon

System

(Fig. 12.42)

System

( at rest)

System

( at rest)

Eat +qdue to -q

localid="1658130749562" Bat+qdue to -q

Fat +qdue to-q

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