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Formula sheet · PU-305

Classical Electrodynamics — formula sheet

Every boxed result from the 12 derivations of this unit on one page, for revision. Each title links to the full derivation, with its assumptions and where the formula breaks down. Constants: physical constants table.

D-283

Laplacian of 1/r as a Delta Function

\[ \nabla^2\!\left(\frac{1}{r}\right) = -4\pi\,\delta^3(\mathbf{r}) \]

The Newtonian kernel \( 1/r \) is harmonic everywhere except at the origin, where it hides a point source of strength \( -4\pi \). Applied to \( -\frac{1}{4\pi r} \), the Laplacian returns exactly \( \delta^3(\mathbf{r}) \), which is why \( G(\mathbf{r}) = -\frac{1}{4\pi r} \) is the Green's function of \( \nabla^2 \). Physically, the flux of the Coulomb field through any closed surface enclosing the charge is the same — Gauss's law in miniature.

D-285

Electrostatic Potential and Irrotational E

\[ \nabla\times\mathbf{E}=\mathbf{0}\ \Longleftrightarrow\ \mathbf{E}=-\nabla\phi,\qquad \nabla^2\phi=-\frac{\rho}{\varepsilon_0} \]

A static electric field is irrotational, so it is the gradient of a single scalar potential. Feeding that potential into Gauss's law yields Poisson's equation, a single linear second-order PDE for \( \phi \). Given \( \phi \) or its normal derivative on the boundary, the solution is unique: electrostatics is completely determined by charge in the volume plus data on the surface.

D-047

Multipole Expansion of the Potential

\[ V(\vec r)=\frac{1}{4\pi\epsilon_0}\left[\frac{Q}{r}+\frac{\hat r\cdot\vec p}{r^{2}}+\frac{1}{2r^{3}}\sum_{i,j}\hat r_i\hat r_j\,Q_{ij}+\cdots\right] \]

Far from any bounded static source the potential is an ordered sum: a Coulomb tail set by the net charge \(Q\); if \(Q=0\), a dipole field set by \(\vec p=\int\vec r'\rho\,d^3r'\); if \(\vec p=0\) too, a quadrupole field set by the tensor \(Q_{ij}\); and so on. The leading non-vanishing moment controls the far field and, uniquely, is independent of where the origin is placed.

D-052

Ampère's Circuital Law from Biot–Savart

\[ \nabla\times\vec{B} = \mu_0\,\vec{J} \qquad\Longleftrightarrow\qquad \oint_C\vec{B}\cdot d\vec{l} = \mu_0 I_{\text{enc}} \]

The magnetostatic field circulates around current: its curl at a point is set entirely by the local current density there, and the net circulation around any loop counts only the current piercing that loop, weighted by \(\mu_0\). Regions with no current carry a curl-free (but not necessarily zero) field.

D-288

Vector Potential and Bound Currents

\[ \mathbf{J}_b=\nabla\times\mathbf{M},\qquad \mathbf{K}_b=\mathbf{M}\times\hat{\mathbf n},\qquad \mathbf{H}=\frac{1}{\mu_0}\mathbf{B}-\mathbf{M},\qquad \nabla\times\mathbf{H}=\mathbf{J}_f \]

A magnetized body produces exactly the field of a current \(\nabla\times\mathbf{M}\) threading its interior plus a sheet current \(\mathbf{M}\times\hat{\mathbf n}\) wrapping its surface — no more, no less. The field \(\mathbf{H}\) is engineered so that only the currents you drive through wires appear as its source; the material's own response is hidden inside \(\mathbf{H}\)'s definition through \(\mathbf{M}\).

D-289

Faraday's Law and the Induced Field

\[ \nabla\times\vec{E} = -\frac{\partial \vec{B}}{\partial t} \]

The circulation density of the electric field at a point equals minus the rate at which the magnetic field there is changing. A magnetic field growing out of the page ( \(\partial\vec{B}/\partial t\) out of the page) drives \(\vec{E}\) to circulate clockwise, so the induced electric field opposes the change that created it, this is Lenz's law written locally. The field is genuinely non-conservative: \(\oint\vec{E}\cdot d\vec{\ell}\neq 0\).

D-167

Maxwell Stress Tensor and Field Momentum

\[ \frac{d}{dt}\left(\mathbf{p}_{\text{mech}} + \mathbf{p}_{\text{field}}\right)_i = \oint_{\mathcal{S}} T_{ij}\,da_j, \qquad T_{ij} = \varepsilon_0\!\left(E_iE_j - \tfrac{1}{2}\delta_{ij}E^2\right) + \tfrac{1}{\mu_0}\!\left(B_iB_j - \tfrac{1}{2}\delta_{ij}B^2\right), \qquad \mathbf{g} = \varepsilon_0\,\mathbf{E}\times\mathbf{B} = \frac{\mathbf{S}}{c^2} \]

Momentum is conserved locally in electrodynamics, but only if the field is credited with momentum of density \(\mathbf{g} = \mathbf{S}/c^2\). The rate of change of (mechanical + field) momentum inside any closed surface equals the stress-tensor flux through that surface: \(T_{ij}\,da_j\) is the \(i\)-th component of force transmitted across the area element \(d\mathbf{a}\). Equivalently, \(-T_{ij}\) is the flux density of the \(i\)-component of momentum in the \(j\)-direction. The diagonal elements are pressures/tensions: along a field line the field pulls with tension \(\tfrac{1}{2}\varepsilon_0E^2 + \tfrac{1}{2}B^2/\mu_0\) per unit area; transverse to the lines it pushes with the same magnitude of pressure.

D-164

Electromagnetic Wave Equation in Vacuum

∇2E = μ0ε0 ∂2E/∂t2     ∇2B = μ0ε0 ∂2B/∂t2     c = 1/√(μ0ε0)

Each Cartesian component of E and of B obeys the same three-dimensional wave equation. A disturbance in the fields propagates without a medium at the fixed speed c, determined solely by the two vacuum constants. The two fields are not independent: they are locked together through the original first-order equations (which force E ⊥ B ⊥ propagation direction and E = cB in magnitude), but each separately satisfies the second-order wave equation.

D-293

Retarded Potentials in Lorenz Gauge

\[ V(\vec r,t)=\frac{1}{4\pi\varepsilon_0}\int\frac{[\rho]}{|\vec r-\vec r\,{}'|}\,d^3r',\qquad \vec A(\vec r,t)=\frac{\mu_0}{4\pi}\int\frac{[\vec J]}{|\vec r-\vec r\,{}'|}\,d^3r',\qquad [\,\cdot\,]\equiv \text{evaluated at }t_r=t-\frac{|\vec r-\vec r\,{}'|}{c} \]

The potential here-and-now is the Coulomb/Biot–Savart-like sum over all source elements, but each element speaks to us from the moment its light-cone reaches us. Information about a source point a distance \(R\) away is always old by \(R/c\). The functional form is identical to the static case except that "now" is replaced by "then." When the sources change slowly (or not at all), \(t_r\to t\) and the static expressions are recovered.

D-170

Larmor Formula for Radiated Power

\[ P = \frac{q^2 a^2}{6\pi\varepsilon_0 c^3} = \frac{\mu_0 q^2 a^2}{6\pi c} \]

An accelerating charge sheds energy as light at a rate fixed by the square of its acceleration. Doubling the acceleration quadruples the radiated power; the sign of the charge and the direction of the acceleration are irrelevant to the total. The emission is beamed sideways — a \( \sin^2\theta \) doughnut with its dead axis along \( \vec{a} \), maximal in the plane perpendicular to the acceleration.

D-294

Covariant Formulation of Electrodynamics

\[ \boxed{\ \partial_{\mu}F^{\mu\nu}=\mu_{0}J^{\nu}\ ,\qquad \partial_{\lambda}F_{\mu\nu}+\partial_{\mu}F_{\nu\lambda}+\partial_{\nu}F_{\lambda\mu}=0\ } \]

The first equation is Gauss's law (\(\nu=0\)) and the Ampère–Maxwell law (\(\nu=1,2,3\)) fused into one four-component tensor equation; the source is the four-current. The second is the homogeneous pair (\(\nabla\cdot\vec{B}=0\) and Faraday's law), which holds automatically because the field is derived from a potential. Every symbol carries spacetime indices, so both equations keep their form under any Lorentz transformation — covariance is manifest, not something to be verified frame by frame. \(\vec{E}\) and \(\vec{B}\) are not independent fields but components of the single object \(F^{\mu\nu}\).

D-295

Transformation of E and B under Boosts

\[ \vec E'_\parallel=\vec E_\parallel,\quad \vec B'_\parallel=\vec B_\parallel,\quad \vec E'_\perp=\gamma\!\left(\vec E+\vec v\times\vec B\right)_\perp,\quad \vec B'_\perp=\gamma\!\left(\vec B-\tfrac{1}{c^2}\vec v\times\vec E\right)_\perp \]

Components of the field along the boost survive untouched; components perpendicular to the boost are amplified by \(\gamma\) and, crucially, mixed — the perpendicular electric field in \(S'\) picks up a \(\vec v\times\vec B\) contribution and the perpendicular magnetic field picks up a \(-\vec v\times\vec E/c^2\) contribution. There is no frame-independent way to say "this is an electric field": \(\vec E\) and \(\vec B\) are the time-space and space-space parts of the single antisymmetric tensor \(F^{\mu\nu}\), and a boost simply re-slices that tensor. The combinations \(\vec E\cdot\vec B\) and \(B^2-E^2/c^2\) are the two quantities the slicing leaves fixed.

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