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.

Short Answer

Expert verified

The tensor invariants are FμvFμv=2B2-E2c2GμvGμv=2E2c2-B2andFμvGμv=-4cE.B

Step by step solution

01

Expression for the Product of  and :

Write the expression for the product of FμvFμv

FμvFμv=F00F00-F01F01-F02F02-F03F03-F10F10-F20F20-F30F30+F11F11+F12F12+F13F13+F21F21+F22F22+F23F23+F31F31+F32F32+F33F33Here,F00=0,F01=Exc,F02=Eyc,F03=Ezc,F12=Bz,F31=ByandF23=Bx .......(1)

Write the expression for the product of GμvGμv

GμvGμv=G00G00-G01G01-G02G02-G03G03-G10G10-G20G20-G30G30+G11G11+G12G12+G13G13+G21G21+G22G22+G23G23+G31G31+G32G32+G33G33Here,G00=0,G01,G12=Bz,G31=By,G23=Bx,Exc,G02=EycandG03=Ezc ......(2)

02

Determine the Product of :

Substitute F00=0,F01=Exc,F02=Eyc,F03=Ezc,F12=Bz,F31=ByandF23=Bxin equation (1).

FμvFμv=0-Exc2--Eyc2-Ezc2-Exc2-Eyc2-Ezc2+0+Bz2+By2+Bx2+0+Bz2+By2+Bx2+0FμvFμv=-2Ex2c2-2Ey2c2-2Ez2c2+2Bx2+2By2+2Bz2Here,Bx+By+Bz=BandEx+Ex+Ex=E

So, the above equation becomes,

FμνFμν=-2Ex2c2-2Ey2c2-2Ez2c2+2Bx2+2By2+2Bz2FμνFμν=-2c2Ex2+Ey2+Ez2+2Bx2+By2+Bz2FμνFμν=-2E2c2+2B2FμνFμν=2B2E2c2

03

Determine the Product of :

Substitute G00=0,G01=Bx,G01=By,G01=Bz,G12=EZc,G31=EycandG31=Excin equation (2).

GμνGμν=0-Bx2-Bx2-Bx2-Bx2-Bx2-Bx2+0+-Ezc2+-Eyc+-Ezc+0+-Exc+-Eyc+-Exc+0GμνGμν=-2Bx2-2Bx2-2Bx2+Ez2c2+Ey2c2+Ez2c2+Ex2c2+Ez2c2+Ex2c2GμνGμν=-2Bx2+By2+Bz2+2c2Ex2+Ey2+Ez2

On further solving,

GμνGμν=-2B2+2c2E2GμνGμν=2E2c2-B2

04

Determine the Product of :

Write the expression for the product of FμνFμν

role="math" localid="1654678337382" FμνFμν=-2F01G01+F02G02+F03G03+2F12G12+F13G13+F23G23

Substitute, role="math" localid="1654679206876" F01=Exc,F02=Eyc,F03=Ezc,F12=Bz,F31=BzandF23=Bx

G01=Bx,G02=By,G03=BzG12=-Ezc,G31=-EzcandG23=-Ezcin the above expression.

FμνFμν=2ExcBx+EycBx+EzcBx+2BzEzc+ByEyc+BxExcFμνFμν=-2cExBx+EyBy+EzBz-2cExBx+EyBy+EzBzFμνFμν=-2cE.B-2cE.BFμνFμν=-4cE.B

Therefore, the tensor invariants areFμνFμν=2B2-E2c2GμνGμν=2E2c2-B2andFμνGμν=4cE.B.

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Most popular questions from this chapter

Why can’t the electric field in Fig 12.35 (b) have a, z component? After all, the magnetic field does.

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.]

In system S0, a static uniform line chargeλ coincides with thez axis.

(a) Write the electric fieldE0 in Cartesian coordinates, for the point (x0,y0,z0).

(b) Use Eq. 12.109 to find the electric in S, which moves with speedv in the x direction with respect to S0. The field is still in terms of (x0,y0,z0); express it instead in terms of the coordinates(x,y,z) in S. Finally, write E in terms of the vector S from the present location of the wire and the angleθ between S and x^. Does the field point away from the instantaneous location of the wire, like the field of a uniformly moving point charge?

(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?


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