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by Pravegaa Education

Potential Formulation

Theory, worked examples and 5 previous-year questions with full solutions — IIT JAM, GATE, CSIR NET-JRF and JEST, 2020 onwards.

Theory
Physical motivation

Instead of working directly with six field components (\(\vec{E}\), \(\vec{B}\)), we encode electrodynamics in four potential components — scalar \(V\) and vector \(\vec{A}\). In the Lorenz gauge these satisfy wave equations with retarded solutions: changes in sources propagate outward at speed \(c\). Retarded potentials are the foundation for computing radiation fields.

Scalar and Vector Potentials

Since \(\nabla\cdot\vec{B}=0\) always, write \(\vec{B}=\nabla\times\vec{A}\). Faraday's law \(\nabla\times\vec{E}=-\partial\vec{B}/\partial t\) then gives: \(\nabla\times(\vec{E}+\partial\vec{A}/\partial t)=\mathbf{0}\), so:

Fields in terms of potentials

\begin{equation} \vec{E} = -\nabla V - \frac{\partial\vec{A}}{\partial t},\qquad \vec{B} = \nabla\times\vec{A} \end{equation} Only M2 and M3 are automatically satisfied. M1 and M4 give: \begin{align} \nabla^2V + \frac{\partial(\nabla\cdot\vec{A})}{\partial t} &= -\frac{\rho}{\eps} \\[4pt] \nabla^2\vec{A} - \muz\eps\frac{\partial^2\vec{A}}{\partial t^2} - \nabla\!\left(\nabla\cdot\vec{A}+\muz\eps\frac{\partial V}{\partial t}\right) &= -\muz\vec{J} \end{align}

Gauge Transformations

Gauge freedom

The transformation: \begin{equation} \vec{A} \to \vec{A}' = \vec{A}+\nabla\lambda,\qquad V \to V' = V-\frac{\partial\lambda}{\partial t} \end{equation} leaves \(\vec{E}\) and \(\vec{B}\) unchanged for any scalar \(\lambda(\vec{r},t)\). Physical observables are gauge invariant; \(V\) and \(\vec{A}\) individually are not unique.

Coulomb Gauge: \(\nabla\cdot\vec{A}=0\)

\begin{equation} \nabla^2 V = -\frac{\rho}{\eps} \quad\text{(instantaneous Poisson — no retardation)} \end{equation} Best for: static problems, quantum mechanics (canonical quantization).

Lorenz Gauge: \(\nabla\cdot\vec{A}+\muz\eps\,\partial V/\partial t=0\)

Symmetric, covariant wave equations: \begin{align} \Box^2 V \equiv \nabla^2 V - \muz\eps\frac{\partial^2 V}{\partial t^2} &= -\frac{\rho}{\eps} \\[4pt] \Box^2\vec{A} \equiv \nabla^2\vec{A} - \muz\eps\frac{\partial^2\vec{A}}{\partial t^2} &= -\muz\vec{J} \end{align} \(\Box^2\) = d'Alembertian. Relativistically covariant. Best for: radiation.

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