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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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204 Chapter 6<br />

The field-strength tensor contains six independent degrees of freedom,<br />

the E and B fields. The redundancy imposed by the constraint of<br />

the homogeneous equations w<strong>as</strong> removed by introducing the vector potential.<br />

There still remains one redundant degree of freedom related to<br />

a constraint imposed by current conservation. The Maxwell equations<br />

remain invariant under a “gauge trans<strong>for</strong>mation” A → A − ∂α where α<br />

is an arbitrary scalar function. The modified A yields the same fields<br />

E and B which are the physically me<strong>as</strong>urable quantities.<br />

The relationship to current conservation is e<strong>as</strong>iest recognized if one<br />

recalls that Maxwell’s equations can be derived from a Lagrangian<br />

− 1 4 F 2 − J · A where F 2 = F µν F µν . A gauge trans<strong>for</strong>mation introduces<br />

an additional term J ·∂α which is identical to a total divergence ∂ ·(αJ)<br />

if ∂ · J = 0 and thus leaves the Euler-Langrange equations unchanged.<br />

Indeed, current conservation is a necessary and sufficient condition <strong>for</strong><br />

the gauge invariance of the theory (Itzykson and Zuber 1983).<br />

A judicious choice of gauge can simplify the equations enormously.<br />

Two important possibilities are the Lorentz gauge and the Coulomb,<br />

transverse, or radiation gauge, b<strong>as</strong>ed on the conditions<br />

∂ · A = 0,<br />

Lorentz gauge,<br />

∇ · A = 0, Coulomb gauge. (6.20)<br />

Maxwell’s equations are then found to be (Jackson 1975)<br />

Φ = ρ, A = J, Lorentz gauge,<br />

−∇ 2 Φ = ρ, A = J T , Coulomb gauge, (6.21)<br />

where J T is the transverse part of J characterized by ∇ · J T = 0.<br />

In the absence of sources (ρ = 0 and J = 0) the potential Φ vanishes<br />

in the Coulomb gauge while A obeys a wave equation. A Fourier trans<strong>for</strong>mation<br />

leads to (−k 2 + ω 2 )A = 0 whence the propagating modes<br />

have the dispersion relation k 2 = ω 2 corresponding to m<strong>as</strong>sless particles.<br />

Because of the transversality condition k · A = 0 there are only<br />

two polarizations, the usual transverse electromagnetic waves. They<br />

are characterized by an electric field E transverse to k and a magnetic<br />

field of the same magnitude transverse to both.<br />

6.3.2 Linear Response of the Medium<br />

Maxwell’s equations allow one to calculate the electromagnetic fields<br />

in the presence of prescribed external currents. However, the charged

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