Mathematical Principles of Theoretical Physics

(Rick Simeone) #1

54 CHAPTER 2. FUNDAMENTAL PRINCIPLES OF PHYSICS


whereP= (P^1 ,P^2 ,P^3 )is as in (2.2.28). Thus, it follows that the relativistic motion law is
given by


(2.2.32)


d
dt

Pk=


1 −v^2 /c^2 Fk, Pk=

mvk

1 −v^2 /c^2

fork= 1 , 2 , 3.

2.2.5 Lorentz invariance of electromagnetism


2.6.3 PHD for Maxwell electromagnetic fields


curlE=−

1


c

∂H


∂t

(2.2.33) ,


(2.2.34) divH= 0 ,


curlH=

1


c

∂E


∂t

+


4 π
c

(2.2.35) J,


(2.2.36) divE= 4 π ρ,


whereE,Hare the electric and magnetic fields, andJis the current density, andρthe charge
density.
To show the Lorentz invariance of the Maxwell equations (2.2.33)-(2.2.36), we need to
express them in the form of the 4-D electromagnetic potential and current density.
The electromagnetic potential and current density are briefly introduced in (2.2.16) and
(2.2.17):


(2.2.37)


Aμ= (A 0 ,A 1 ,A 2 ,A 3 ),
Jμ= (J 0 ,J 1 ,J 2 ,J 3 ), J 0 =−cρ.

Using the Lorentz tensor operator


∂μ=


∂xμ

=


(



∂x^0

,



∂x^1

,



∂x^2

,



∂x^3

)


,


we can construct two second-order Lorentz tensors:


(2.2.38)


Fμ ν=
∂Aν
∂xμ


∂Aμ
∂xν

,


Gμ ν=

1


2


εμ ν α βgα κgβ λFκ λ,

wheregα βis the Minkowski metric, and


εμ ν α β=








1 (μ,ν,α,β)is an even permutation of( 0123 ),
− 1 (μ,ν,α,β)is an odd permutation of( 0123 ),
0 otherwise,

is a 4-th order Lorentz tensor. Thanks to the relations:


H=curl~A, E=∇A 0 −

1


c

∂~A


∂t

, ~A= (A 1 ,A 2 ,A 3 ),

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