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MA3431/3432 Classical Field Theory and Classical Electrodynamics

Lecturer: Dr. Nigel Buttimore

Website: Link


Alternative Derivation of the EM field from the Liénard Potentials

Given the Liénard - Wiechert potentials

A^{\nu}=\frac{e V^{\nu}}{V_\sigma R^\sigma}

where the expression is to be evaluated at retarded time defined by

R^\sigma R_\sigma=0

and where

R^\mu=x^\mu-x_e^\mu(\tau)
V^\mu=\frac{\mathrm{d}x^\mu_e(\tau)}{\mathrm{d}\tau}=-\frac{\mathrm{d}R^\mu}{\mathrm{d}\tau}

We wish to find the electromagnetic fields F^{\mu\nu}.

We begin by taking finding how the retarded time is related to the change in the observation point

(\partial^{\mu} R^{\sigma})R_{\sigma}=0

now regarding R^{\sigma}=R^{\sigma}(x^\rho,\tau) and since the path of the charge e x_\mathrm{e}^\mu(\tau) intersects the past lightcone of the event x^\rho uniqely we can regard \tau=\tau(x^\rho). And so we find

\left(\frac{\partial R^\sigma}{\partial \tau}\partial^\mu \tau+g^{\mu \sigma}\right)R_\sigma=0
\left(-V^{\sigma} \partial^{\mu} \tau+g^{\mu \sigma}\right)R_{\sigma} =0
-V^{\sigma} R_{\sigma} \partial^\mu \tau+R^\mu=0
\partial^{\mu} \tau=\frac{R^\mu}{V^\sigma R_\sigma}

Now taking \partial^\mu of A^\nu, regarding \tau=\tau(x^\rho) and using the expression above we find

\partial^\mu A^\nu=\frac{e \partial^\mu V^\nu}{V^\sigma R_\sigma}-\frac{e V^\nu}{\left(V^\sigma R_\sigma\right)^2}\left( \left(\partial^\mu V^\rho\right)R_\rho+V^\rho \partial^\mu R_\rho\right)
=\frac{e \dot{V}^\nu}{V^\sigma R_\sigma}\frac{R^\mu}{V^\rho R_\rho}  -\frac{eV^\nu}{(V^\sigma R_\sigma)^2} \left( \dot{V}^\rho R_\rho \frac{R^\mu}{V^\lambda R_\lambda} +V^\rho \left(\dot{R}_\rho\frac{R^\mu}{V^\lambda R_\lambda}+\delta^\mu_\rho \right) \right)
=\frac{e }{(V^\sigma R_\sigma)^2}R^\mu \dot{V}^\nu-\frac{e \dot{V}^\rho R_\rho}{(V^\sigma R_\sigma)^3}R^\mu V^\nu  +\frac{e V^\rho V_\rho}{(V^\sigma R_\sigma)^3} R^\mu V^\nu -\frac{e}{(V^\sigma R_\sigma)^2}V^\mu V^\nu

where \dot{X} means \frac{\mathrm{d}}{\mathrm{d}\tau}X

Noting that

V^\sigma V_\sigma =\gamma^2(c^2-\overrightarrow{v}^2)
=\gamma^2 c^2 \gamma^{-2}
=c^2

and using our expression for \partial^\mu A^\nu we find

F^{\mu \nu}=\partial^\mu A^\nu-\partial^\nu A^\mu
=F_{acc}^{\mu \nu}+F_{vel}^{\mu \nu}

where

F_{acc}^{\mu \nu}=\frac{e}{(V^\sigma R_\sigma)^2}(R^\mu \dot{V}^\nu-R^\nu \dot{V}^\mu)-\frac{e \dot{V}^\rho R_\rho}{(V^\sigma R_\sigma)^3}(R^\mu V^\nu-R^\nu V^\mu)
F_{vel}^{\mu \nu}=\frac{e c^2}{(V^\sigma R_\sigma)^3}(R^\mu V^\nu - R^\nu V^\mu)