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

Short Answer

Expert verified

The potential representation is automatically satisfiedGμνxv=0

Step by step solution

01

Expression for the field tensor equation:

Using equation 12.130, write the equation for the field tensor.

Fμν=Fμνxλ+Fνλxμ+Fλμxν .........(1)

Itisalsoknowthat:x2=λxμ=μxν=νAlso,thevalueofFμν,FμλandFνλisgivenby:Fμν=μAν-νAμFμλ=νAλ-λAνFνμ=λAμ-μAλ

02

Show that :

λμAV=μλλAV

SubstituteλforXλ,μforXμ,VforXV,μAV-VAμforFμv,VAλ-λ-AVforFandλAμ-μAλFiμinequation(1)FμVX2+FXμ+FλμXV=λFμV+μF+VFλμFμVX2+FXμ+FλμXV=λμAV-V+μVAλ-λAV+VλAμ-μAλFμVX2+FXμ+FλμXV=λμAV-λVAμ+λVAλ-μλAV+VλAμ-VμAλOnfurthersolving,FμVX2+FXμ+FλμXV=λμAV-λVAμ+λVAλ-μλAV+VλAμ-VμAλFμVX2+FXμ+FλμXV=λμAν-μλAν+-λVAμ+νλAμ+μλAλ-νμAλFμVX2+FXμ+FλμXV=0Hence,theaboveequationsatisfiesGμνxν=0Therefore,thepotentialrepresentattionisautomaticallysatisfiedGμνxν=0

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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) Equation 12.40 defines proper velocity in terms of ordinary velocity. Invert that equation to get the formula for u in terms of η.

(b) What is the relation between proper velocity and rapidity (Eq. 12.34)? Assume the velocity is along the x direction, and find as a function of θ.

Check Eq. 12.29, using Eq. 12.27. [This only proves the invariance of the scalar product for transformations along the x direction. But the scalar product is also invariant under rotations, since the first term is not affected at all, and the last three constitute the three-dimensional dot product a-b . By a suitable rotation, the x direction can be aimed any way you please, so the four-dimensional scalar product is actually invariant under arbitrary Lorentz transformations.]

A car is traveling along the 45° line in S (Fig. 12.25), at (ordinary) speed(2/5)c .

(a) Find the componentsux anduy of the (ordinary) velocity.

(b) Find the componentsrole="math" localid="1658247416805" ηx andηy of the proper velocity.

(c) Find the zeroth component of the 4-velocity,η0 .

SystemS¯ is moving in the x direction with (ordinary) speed 2/5c, relative to S. By using the appropriate transformation laws:

(d) Find the (ordinary) velocity componentsu¯x and u¯yin S¯.

(e) Find the proper velocity components η¯x andη¯y in S¯.

(f) As a consistency check, verify that

η¯=u¯1-u¯2c2

As an illustration of the principle of relativity in classical mechanics, consider the following generic collision: In inertial frame S, particle A (massmA, velocityuB ) hits particle B (massmB, velocity uB). In the course of the collision some mass rubs off A and onto B, and we are left with particles C (massmc, velocityuc ) and D (mass mD, velocityuD ). Assume that momentum (p=mu)is conserved in S.

(a) Prove that momentum is also conserved in inertial frames¯, which moves with velocity relative to S. [Use Galileo’s velocity addition rule—this is an entirely classical calculation. What must you assume about mass?]

(b) Suppose the collision is elastic in S; show that it is also elastic in S¯.

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