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Special Relativity and Electromagnetism

Maxwell’s equations in covariant form using the field tensor FμνF^{\mu\nu}:

μFμν=μ0Jν(inhomogeneous)\partial_\mu F^{\mu\nu} = \mu_0 J^\nu \quad \text{(inhomogeneous)}

λFμν+μFνλ+νFλμ=0(homogeneous / Bianchi identity)\partial_\lambda F_{\mu\nu} + \partial_\mu F_{\nu\lambda} + \partial_\nu F_{\lambda\mu} = 0 \quad \text{(homogeneous / Bianchi identity)}

The electromagnetic field tensor:

Fμν=(0Ex/cEy/cEz/cEx/c0BzByEy/cBz0BxEz/cByBx0)F^{\mu\nu} = \begin{pmatrix} 0 & -E_x/c & -E_y/c & -E_z/c \\ E_x/c & 0 & -B_z & B_y \\ E_y/c & B_z & 0 & -B_x \\ E_z/c & -B_y & B_x & 0 \end{pmatrix}

The dual tensor: F~μν=12ϵμνρσFρσ\tilde{F}^{\mu\nu} = \frac{1}{2}\epsilon^{\mu\nu\rho\sigma}F_{\rho\sigma}.

The Lorentz force: fμ=qFμνuνf^\mu = qF^{\mu\nu}u_\nu where uν=γ(c,v)u^\nu = \gamma(c, \mathbf{v}) is the four-velocity.

Under a boost with velocity vv along the xx-axis:

Ex=Ex,Bx=BxE'_x = E_x, \quad B'_x = B_x

Ey=γ(EyvBz),By=γ ⁣(By+vc2Ez)E'_y = \gamma(E_y - vB_z), \quad B'_y = \gamma\!\left(B_y + \frac{v}{c^2}E_z\right)

Ez=γ(Ez+vBy),Bz=γ ⁣(Bzvc2Ey)E'_z = \gamma(E_z + vB_y), \quad B'_z = \gamma\!\left(B_z - \frac{v}{c^2}E_y\right)

Key insight: E\mathbf{E} and B\mathbf{B} mix under Lorentz transformations. What appears as a pure electric field in one frame becomes a mixture of electric and magnetic fields in another. There is no frame-independent distinction between E\mathbf{E} and B\mathbf{B}.

Invariants: E2c2B2E^2 - c^2B^2 and EB\mathbf{E}\cdot\mathbf{B} are Lorentz invariants. A pure radiation field (E=cBE = cB, EB\mathbf{E}\perp\mathbf{B}) satisfies both invariants being zero.

12.3 Electromagnetic Field Momentum and Angular Momentum

Section titled “12.3 Electromagnetic Field Momentum and Angular Momentum”

Field momentum density:

g=Sc2=ε0E×B\mathbf{g} = \frac{\mathbf{S}}{c^2} = \varepsilon_0\mathbf{E} \times \mathbf{B}

Field angular momentum: L=r×gd3r\mathbf{L} = \int \mathbf{r} \times \mathbf{g}\, d^3r.

Conservation: \frac{d}{dt}\left(\mathbf{p}_{\text{mech} + \mathbf{p}_{\text{field}\right) = 0}}.

For a charge and a magnetic monopole (if they exist), the field angular momentum L=qgr^/(4π)\mathbf{L} = -qg\hat{\mathbf{r}}/(4\pi) is quantised in units of /2\hbar/2Leading to the Dirac charge quantisation condition eg=n/2eg = n\hbar/2.

Quantity3-vector form4-vector / tensor form
Potentialϕ\phi, A\mathbf{A}Aμ=(ϕ/c,A)A^\mu = (\phi/c, \mathbf{A})
FieldsE\mathbf{E}, B\mathbf{B}Fμν=μAννAμF^{\mu\nu} = \partial^\mu A^\nu - \partial^\nu A^\mu
Charge-currentρ\rho, J\mathbf{J}Jμ=(cρ,J)J^\mu = (c\rho, \mathbf{J})
Force densityρE+J×B\rho\mathbf{E} + \mathbf{J}\times\mathbf{B}fμ=FμνJνf^\mu = F^{\mu\nu}J_\nu
Energy-momentumu=12(ε0E2+B2/μ0)u = \frac{1}{2}(\varepsilon_0 E^2 + B^2/\mu_0), S\mathbf{S}TμνT^{\mu\nu}
flowchart TD
A[12_Special Relativity And Electromagnetism 12] --> B[Key Concepts]
A --> C[Core Principles]
A --> D[Practical Applications]
B --> E[Fundamental definitions]
C --> F[Design patterns]
D --> G[Real-world usage]

Special relativity and electromagnetism are inseparable: Maxwell’s equations are already relativistically correct, and the electric and magnetic fields are merely different aspects of a single electromagnetic field tensor. What one observer calls a pure electric field, a moving observer sees as a mixture of electric and magnetic components. The field tensor FμνF^{\mu\nu} packages all six field components into a single mathematical object that transforms cleanly under Lorentz boosts. The Lorentz force law becomes a compact four-vector equation, and the conservation of energy-momentum extends to include field contributions. The key physical picture is that electricity and magnetism are not separate forces but different faces of the same relativistic coin, unified by the geometry of spacetime.

  • Assuming E\mathbf{E} and B\mathbf{B} transform independently. They do not; the field tensor transforms as a whole under Lorentz boosts. A pure electric field in one frame becomes a mixture in another.
  • Confusing the dual tensor F~μν\tilde{F}^{\mu\nu} with FμνF^{\mu\nu}. The dual swaps electric and magnetic fields (EcB\mathbf{E} \to c\mathbf{B}, BE/c\mathbf{B} \to -\mathbf{E}/c) and is used in the homogeneous Maxwell equation μF~μν=0\partial_\mu \tilde{F}^{\mu\nu} = 0.
  • Forgetting that FμνF^{\mu\nu} is antisymmetric. This antisymmetry encodes the fact that there are six independent field components (three for E\mathbf{E}, three for B\mathbf{B}).
  • Misapplying the Lorentz force formula. The relativistic Lorentz force fμ=qFμνuνf^\mu = qF^{\mu\nu}u_\nu gives the four-force, not the three-force. The spatial components reduce to dp/dt=q(E+v×B)d\mathbf{p}/dt = q(\mathbf{E} + \mathbf{v}\times\mathbf{B}) in the non-relativistic limit.

Problem 1. Show that EB\mathbf{E}\cdot\mathbf{B} is a Lorentz invariant.

Solution. EB\mathbf{E}\cdot\mathbf{B} is proportional to 14F~μνFμν\frac{1}{4}\tilde{F}^{\mu\nu}F_{\mu\nu}. Since this is a full contraction of two tensors, it is a scalar and thus invariant. Explicitly: F~μνFμν=4EB/c\tilde{F}^{\mu\nu}F_{\mu\nu} = -4\mathbf{E}\cdot\mathbf{B}/c. Under any Lorentz transformation, both FμνF^{\mu\nu} and F~μν\tilde{F}^{\mu\nu} transform as tensors, so their contraction is invariant. \blacksquare

Problem 2. Derive the transformation of the Poynting vector under a Lorentz boost.

Solution. S=E×B/μ0\mathbf{S} = \mathbf{E} \times \mathbf{B} / \mu_0 transforms as part of the energy-momentum tensor TμνT^{\mu\nu}. The components T0i=Si/cT^{0i} = S_i/c transform under a boost: Sx=SxS'_x = S_x, Sy=γ(Syvu)S'_y = \gamma(S_y - v u), Sz=γ(Sz+vu)S'_z = \gamma(S_z + v u) where uu is the energy density. This shows that energy flux in one frame contributes to energy density in another. \blacksquare

  • Particle physics: The covariant formulation is essential for quantum electrodynamics (QED), where FμνF^{\mu\nu} couples to the Dirac field via minimal coupling μDμ\partial^\mu \to D^\mu.
  • Plasma physics: Relativistic plasmas require the covariant formulation for correct treatment of high-energy particle motion in strong electromagnetic fields.
  • Astrophysics: Pulsar electrodynamics and magnetar fields involve enormous Lorentz factors where the field transformation laws govern radiation emission mechanisms.
  • Accelerator physics: The design of particle accelerators requires precise knowledge of how electromagnetic fields appear in the rest frame of relativistic particle bunches.
Worked Example 12.1: Fields of a Moving Point Charge

A point charge qq at rest at the origin has E=qr^/(4πε0r2)\mathbf{E} = q\hat{\mathbf{r}}/(4\pi\varepsilon_0 r^2), B=0\mathbf{B} = 0.

In a frame moving with velocity vv along the xx-axis, the fields at the boosted position are:

Ey=γqy4πε0(r2+γ2v2t2)3/2,Bz=vc2EyE'_y = \gamma\frac{qy'}{4\pi\varepsilon_0(r'^2 + \gamma^2 v^2 t'^2)^{3/2}}, \quad B'_z = -\frac{v}{c^2}E'_y

At t=0t' = 0: E\mathbf{E}' is still radial (from the instantaneous position) but with an enhanced transverse component by factor γ\gamma. The magnetic field is B=v×E/c2\mathbf{B}' = -\mathbf{v} \times \mathbf{E}'/c^2Circulating around the direction of motion.

The Poynting vector S=E×B/μ0\mathbf{S}' = \mathbf{E}' \times \mathbf{B}'/\mu_0 is nonzero even for a uniformly moving charge (it points outward and forward, indicating energy flow in the direction of motion).

For ultrarelativistic motion (γ1\gamma \gg 1): the fields are concentrated in a thin disk of angular width 1/γ\sim 1/\gamma around the plane perpendicular to the motion. This is the basis of synchrotron radiation patterns.

This section provides detailed coverage of advanced concepts, including full derivations, proofs, and extended examples.

Complete mathematical derivations and proofs are provided where appropriate. Each step is explained to ensure understanding of the underlying reasoning.

Advanced examples demonstrate the application of concepts to complex problems. These examples go beyond standard exam questions to develop deeper understanding.

This material connects to current research and advanced applications in the field. Understanding these connections provides context for the study material.

Ensure you have mastered the prerequisite material before attempting this advanced content.