Part I, Chapter 4

The Electromagnetic Field

Vector fields, gauge invariance, and Maxwell's equations from the Lagrangian

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Video Lecture

Electromagnetic Field - MIT QFT Lecture

Classical electromagnetic field theory from the Lagrangian formulation

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4.1 The Electromagnetic Lagrangian

The electromagnetic field is described by a 4-vector potential Aμ(x) = (φ, A), where φ is the scalar potential and A is the vector potential.

💡Why a 4-Vector Potential?

In special relativity, space and time must be treated on equal footing. The electric potential φ and magnetic vector potential A naturally combine into a 4-vector Aμ = (φ, A1, A2, A3).

This ensures the theory is Lorentz invariant - different observers will agree on the physics despite measuring different E and B fields!

The Lagrangian density for the free electromagnetic field is:

$$\mathcal{L} = -\frac{1}{4}F_{\mu\nu}F^{\mu\nu}$$

where the field strength tensor is defined as:

$$F^{\mu\nu} = \partial^\mu A^\nu - \partial^\nu A^\mu$$

This is antisymmetric: Fμν = -Fνμ, giving us 6 independent components corresponding to the 3 components of E and 3 components of B.

4.2 The Field Strength Tensor

In matrix form, the field strength tensor is:

$$F^{\mu\nu} = \begin{pmatrix} 0 & -E_x & -E_y & -E_z \\ E_x & 0 & -B_z & B_y \\ E_y & B_z & 0 & -B_x \\ E_z & -B_y & B_x & 0 \end{pmatrix}$$

The electric and magnetic fields are extracted as:

\begin{align*} E^i &= F^{0i} = -\partial_0 A^i + \partial^i A^0 \\ B^i &= \frac{1}{2}\epsilon^{ijk}F_{jk} \end{align*}

4.3 Maxwell's Equations from the Lagrangian

The Euler-Lagrange equation for Aμ is:

$$\partial_\mu \frac{\partial \mathcal{L}}{\partial(\partial_\mu A_\nu)} - \frac{\partial \mathcal{L}}{\partial A_\nu} = 0$$

For our Lagrangian ℒ = -¼FμνFμν, this yields:

$$\partial_\mu F^{\mu\nu} = 0$$

These are Maxwell's equations in vacuum (in the absence of sources)!

Maxwell's Equations (source-free):

  • • ∂μFμν = 0 → Gauss's law: ∇·E = 0
  • • ∂μFμν = 0 → Ampère-Maxwell: ∇×B - ∂tE = 0
  • • ∂μμν = 0 → No magnetic monopoles: ∇·B = 0
  • • ∂μμν = 0 → Faraday's law: ∇×E + ∂tB = 0

4.4 Gauge Invariance

A crucial property of electromagnetism is gauge invariance. The Lagrangian and physics are unchanged under the transformation:

$$A^\mu(x) \to A^\mu(x) + \partial^\mu \alpha(x)$$

where α(x) is an arbitrary scalar function. This is because:

\begin{align*} F'^{\mu\nu} &= \partial^\mu(A^\nu + \partial^\nu\alpha) - \partial^\nu(A^\mu + \partial^\mu\alpha) \\ &= \partial^\mu A^\nu - \partial^\nu A^\mu + \partial^\mu\partial^\nu\alpha - \partial^\nu\partial^\mu\alpha \\ &= F^{\mu\nu} \quad \text{(partial derivatives commute)} \end{align*}

💡Physical Meaning of Gauge Invariance

Gauge invariance reflects a deep truth: potentials are not directly observable. Only the field strengths E and B (or Fμν) are physical.

We have freedom to choose different potentials Aμ that give the same E and B. This "gauge freedom" is actually a symmetry of nature, and by Noether's theorem, it leads to charge conservation!

4.5 Gauge Fixing

While gauge invariance is a physical symmetry, it causes problems for quantization (redundant degrees of freedom). We must "fix the gauge" by imposing a constraint:

Common Gauge Choices:

  • Lorenz Gauge:μAμ = 0
    Manifestly Lorentz covariant, good for relativistic calculations
  • Coulomb Gauge: ∇·A = 0
    A0 = 0, transverse polarizations only, good for non-relativistic QED
  • Temporal Gauge: A0 = 0
    Simplifies time evolution but breaks manifest Lorentz invariance
  • Axial Gauge: nμAμ = 0
    Useful in specific calculations, nμ is a constant 4-vector

4.6 Classical vs. Quantum Electromagnetism

Classical EM vs. Quantum EM (QED)

How quantization changes our understanding of electromagnetic fields

AspectClassical EMQuantum EM (QED)
FieldsE(x,t) and B(x,t) - classical vectors
Sourcesρ(x,t) and j(x,t) - charge/current densities
PhotonsEmerge as wave packets
Gauge InvarianceA^μ → A^μ + ∂^μα
EquationsMaxwell equations

4.7 Coupling to Matter

To include charged particles (e.g., electrons), we add a coupling term to the Lagrangian:

$$\mathcal{L}_{\text{int}} = -j^\mu A_\mu = -(\rho A^0 - \mathbf{j} \cdot \mathbf{A})$$

where jμ = (ρ, j) is the 4-current density. For a Dirac fermion ψ:

$$j^\mu = -e\bar{\psi}\gamma^\mu\psi$$

This gives the complete QED Lagrangian:

$$\mathcal{L}_{\text{QED}} = -\frac{1}{4}F_{\mu\nu}F^{\mu\nu} + \bar{\psi}(i\gamma^\mu\partial_\mu - m)\psi - e\bar{\psi}\gamma^\mu\psi A_\mu$$

⚠️Common Mistakes to Avoid

Mistake:

Treating A^μ as a 4-vector without considering gauge freedom
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Why it's wrong:

The electromagnetic potential has gauge redundancy - different A^μ can describe the same physical E and B fields.

Correct approach:

Work with gauge-invariant quantities (F^μν, E, B) or fix a gauge (Lorenz gauge, Coulomb gauge, etc.) and stick to it consistently.

Mistake:

Forgetting the constraint equation ∂_μ A^μ = 0 in Lorenz gauge
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Why it's wrong:

The Lorenz gauge condition is not automatic - it's a choice that must be imposed as a constraint on the dynamics.

Correct approach:

Include the gauge condition explicitly. In canonical quantization, this leads to subtleties with negative-norm states that require gauge fixing.

Mistake:

Confusing the electric field E^i with ∂_0 A^i
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Why it's wrong:

In field theory, E^i = -∂_0 A^i - ∂^i A_0, not just the time derivative. The A_0 term is crucial.

Correct approach:

Use the proper definition: E^i = F^{0i} = ∂^0 A^i - ∂^i A^0 (with proper index raising/lowering).

📚 Supplementary Video Lectures

For a comprehensive treatment of classical electrodynamics that complements this field theory approach, see the Advanced Physics: Classical Electrodynamics playlist (62 lectures covering Maxwell's equations, wave propagation, boundary conditions, radiation, and transmission lines).

View All 62 Advanced Physics Videos →

Maxwell's Equations & Fundamentals (7 lectures)

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Video Lecture

Introduction and Equation of Continuity

Foundation of electromagnetic theory

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Video Lecture

Maxwell's Postulate: Displacement Current

The missing piece in Ampère's law

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Video Lecture

Physical Interpretation of Maxwell's Postulate

Understanding displacement current

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Video Lecture

Illustrations of Displacement Current

Examples and applications

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Video Lecture

Maxwell's Field Equations - Part 1

Integral and differential forms

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Video Lecture

Maxwell's Field Equations - Part 2

Derivations and symmetries

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Video Lecture

Maxwell's Field Equations - Part 3

Complete formulation

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Energy & Momentum in EM Fields (8 lectures)

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Video Lecture

Poynting Theorem - Part 1

Energy conservation in EM fields

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Video Lecture

Poynting Theorem - Part 2

Applications and examples

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Video Lecture

Poynting Vector - Part 1

Energy flux in EM waves

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Video Lecture

Poynting Vector - Part 2

Calculations and interpretations

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Video Lecture

Poynting Vector - Part 3

Advanced applications

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Video Lecture

Maxwell Stress Tensor - Part 1

Momentum in EM fields

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Video Lecture

Maxwell Stress Tensor - Part 2

Force and pressure

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Video Lecture

Maxwell Stress Tensor: Radiation Pressure

Pressure from EM waves

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Wave Propagation (10 lectures)

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Video Lecture

Plane EM Waves in Free Space - Part 1

Wave equation solutions

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Video Lecture

Plane EM Waves in Free Space - Part 2

Polarization and properties

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Video Lecture

Waves in Isotropic Dielectric - Part 1

Material effects on propagation

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Video Lecture

Waves in Isotropic Dielectric - Part 2

Refractive index and dispersion

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Video Lecture

Waves in Anisotropic Dielectric - Part 1

Birefringence and crystals

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Video Lecture

Waves in Anisotropic Dielectric - Part 2

Double refraction

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Video Lecture

Waves in Conducting Medium - Part 1

Skin depth and attenuation

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Video Lecture

Waves in Conducting Medium - Part 2

Complex refractive index

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Video Lecture

Waves in Conducting Medium - Part 3

Applications to metals

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Video Lecture

Interaction of EM Waves with Matter

Absorption, scattering, dispersion

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Boundary Conditions & Optical Phenomena (7 lectures)

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Video Lecture

Boundary Conditions for D & B

Discontinuities at interfaces

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Video Lecture

Boundary Conditions for E & H

Tangential and normal components

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Video Lecture

Laws of Reflection and Refraction

Snell's law from Maxwell equations

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Video Lecture

Fresnel's Formulae - Part 1

Amplitude coefficients

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Video Lecture

Fresnel's Formulae - Part 2

Polarization effects

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Video Lecture

Reflection and Transmission Coefficients

Energy conservation at boundaries

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Video Lecture

Brewster's Law and Polarization

Polarization by reflection

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Video Lecture

Total Internal Reflection Polarization

Evanescent waves

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Scattering of EM Waves (3 lectures)

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Video Lecture

Differential Scattering Cross-section

Quantifying scattering processes

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Video Lecture

Thomson Scattering by Free Charge

Classical electron scattering

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Video Lecture

Thomson Scattering: Unpolarized Waves

Cross section calculations

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Electrodynamics of Moving Charges (16 lectures)

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Video Lecture

Electrodynamic Potentials - Part 1

Potentials for time-varying sources

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Video Lecture

Electrodynamic Potentials - Part 2

Gauge transformations

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Video Lecture

Retarded Potentials - Part 1

Causality and finite propagation speed

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Video Lecture

Retarded Potentials - Part 2

Green's functions

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Video Lecture

Liénard-Wiechert Potentials - Part 1

Potentials of moving point charge

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Video Lecture

Liénard-Wiechert Potentials - Part 2

Derivation and properties

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Video Lecture

Fields in Uniform Motion - Part 1

Lorentz contracted fields

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Video Lecture

Electric Field in Uniform Motion

Transformation of E field

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Video Lecture

Magnetic Field in Uniform Motion

Transformation of B field

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Video Lecture

Fields in Uniform Motion - Part 4

Complete field structure

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Video Lecture

Fields in Arbitrary Motion - Part 1

Acceleration effects

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Video Lecture

Fields in Arbitrary Motion - Part 2

Velocity and acceleration fields

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Video Lecture

Fields in Arbitrary Motion - Part 3

Radiation zones

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Video Lecture

Radiation from Accelerated Charge - Part 1

Larmor formula

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Video Lecture

Radiation from Accelerated Charge - Part 2

Angular distribution

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Dipole Radiation (6 lectures)

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Video Lecture

Oscillating Electric Dipole - Introduction

Antenna basics

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Video Lecture

Dipole: Vector and Scalar Potentials

Potential calculations

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Video Lecture

Dipole: Magnetic Field

Near and far field B

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Video Lecture

Dipole: Electric Field

Near and far field E

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Video Lecture

Dipole: Power Radiation

Radiated power and pattern

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Special Topics (5 lectures)

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Video Lecture

Lorentz Force and Potentials

Force in terms of A^μ

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Video Lecture

Potentials in Uniform Fields

Gauge choices for static fields

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Video Lecture

Transmission Line - Introduction

Distributed circuits

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Video Lecture

Transmission Line Equations

Telegrapher's equations

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Video Lecture

Reflection Coefficient

Impedance matching

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Video Lecture

Transmission Line (continued)

Applications

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Video Lecture

Standing Waves and SWR

Voltage standing wave ratio

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Full playlist: Advanced Physics - Classical Electrodynamics (62 lectures covering comprehensive EM theory)

🎯 Key Takeaways

  • The EM field is described by a 4-vector potential Aμ = (φ, A)
  • Physical fields E and B are encoded in the antisymmetric tensor Fμν
  • Maxwell's equations emerge from the Euler-Lagrange equations
  • Gauge invariance Aμ → Aμ + ∂μα is a fundamental symmetry
  • Gauge fixing is required for quantization (Lorenz, Coulomb, etc.)
  • Coupling to matter introduces the interaction term -jμAμ