Quantum Mechanics for Mathematicians

(lily) #1

Maxwell’s equations become just the standard massless wave equation. Since


∇×B−

∂E

∂t

=∇×∇×A+

∂^2 A

∂t^2



∂t

∇A 0

=∇(∇·A)−∇^2 A+

∂^2 A

∂t^2



∂t

∇A 0

=∇

(

∇·A−


∂t

A 0

)

−∇^2 A+

∂^2 A

∂t^2

=−∇^2 A+

∂^2 A

∂t^2

the Maxwell equation 46.3 is the massless Klein-Gordon equation for the spatial
components ofA.
Similarly,


∇·E=∇

(


∂A

∂t

+∇A 0

)

=−


∂t

∇·A+∇^2 A^20

=−

∂^2 A 0

∂t^2

+∇^2 A 0

so Gauss’s law becomes the massless Klein-Gordon equation forA 0.
Like the temporal gauge, the Lorenz gauge does not completely remove the
gauge freedom. Under a gauge transformation



∂A 0

∂t

+∇·A→−

∂A 0

∂t

+∇·A−

∂^2 φ
∂t^2

+∇^2 φ

soφthat satisfy the wave equation


∂^2 φ
∂t^2

=∇^2 φ (46.20)

will give gauge transformations that preserve the Lorenz gauge conditionχ(A) =
0.
The four components ofAμcan be treated as four separate solutions of the
massless Klein-Gordon equation, and the theory then quantized in a Lorentz
covariant manner. The field operators will be


Âμ(t,x) =^1
(2π)^3 /^2


R^3

(aμ(p)e−iωpteip·x+a†μ(p)eiωpte−ip·x)

d^3 p

2 ωp

using annihilation and creation operators that satisfy


[aμ(p),a†ν(p′)] =±δμνδ(p−p′) (46.21)

where±is +1 for spatial coordinates,−1 for the time coordinate.
Two sorts of problems however arise:

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