UY1: Energy & Momentum In Electromagnetic Waves

Why this matters + quick links

This page gives the UY1 working model/result for Energy & Momentum In Electromagnetic Waves. You reuse it when you build fields/potentials by symmetry or superposition, and when you connect fields to forces, energy, and circuits.

1) At a glance

  • EM waves transport both energy and momentum.
  • Vacuum energy density:
u = frac12ε₀E² + B²/2μ₀.
  • Energy flux (Poynting vector):
vec S = 1/μ₀vec E × vec B.
  • For a sinusoidal plane wave, the cycle-average intensity is
I = langle Srangle = frac12 ε₀ c E₀² = E₀B₀/2μ₀.
  • Radiation pressure for normal incidence:
pᵣₐd = I/c(absorption), pᵣₐd = 2I/c(perfect reflection).
  • Direction check: vec S points along the propagation direction (right-handed vec E,vec B,hatk).

Prerequisites: Electromagnetic Spectrum & Sinusoidal EM Plane Waves
Next uses: Standing Electromagnetic Waves

2) Setup

Consider a sinusoidal plane wave in vacuum.

  • vec Eperpvec B,
  • E = cB,
  • propagation direction along vec E × vec B.

Use cycle averages for practical power/intensity values.

Common traps (amplitudes vs averages)
  • Be clear whether you are using instantaneous fields or amplitudes (E₀,B₀) or RMS values. Intensity uses a cycle average.
  • Don’t drop the factor of 1/2 in I = tfrac12ε₀cE₀² for a sinusoid.
  • Pressure uses intensity: p = I/c for absorption and p = 2I/c for perfect reflection (because momentum change doubles).

3) Core derivation/explanation

In vacuum, electric and magnetic energy densities are equal on average:

langle uErangle = langlefrac12ε₀E²rangle, langle uBrangle = langleB²/2μ₀rangle, langle uErangle = langle uBrangle.

Instantaneous Poynting vector:

vec S = 1/μ₀vec E × vec B.

Its cycle average magnitude is intensity:

I = langle Srangle = E₀B₀/2μ₀ = frac12ε₀cE₀².

Momentum density:

vec g = vec S/c²,

so momentum flow causes measurable radiation pressure.

Units checks:

  • S in W m⁻²,
  • I/c in N m⁻² (Pa), matching pressure units.

Checks (sanity)

  • For a vacuum plane wave, langle uErangle = langle uBrangle and I = langle urangle c.
  • If you reverse the direction of propagation, vec S reverses because vec E × vec B reverses.

4) Worked example(s)

A plane wave has electric amplitude E₀ = 120 V m⁻¹.

Intensity:

I = frac12ε₀cE₀² = frac12(8.85 × 10⁻¹²)(3.00 × 10⁸)(120)² ≈ 19.1 W m⁻².

Radiation pressure:

  • perfect absorber:
pᵣₐd = I/c ≈ 6.4 × 10⁻⁸ Pa;
  • perfect reflector:
pᵣₐd = 2I/c ≈ 1.27 × 10⁻⁷ Pa.

5) Practice set (with hints + answers)

  1. If E₀ doubles, what happens to intensity? Hint: Ipropto E₀². Answer: it quadruples.

  2. A beam has I = 500 W m⁻². Find pressure for perfect absorption. Hint: divide by c. Answer: 1.67 × 10⁻⁶ Pa.

  3. Why is radiation pressure from reflection twice that from absorption at same intensity? Hint: compare momentum change signs. Answer: reflected photons reverse momentum, doubling transfer.

6) Summary + next steps

  • Poynting vector gives direction and rate of EM energy transport.
  • EM waves carry momentum with density vec S/c².
  • Radiation pressure is small but crucial in optics, astrophysics, and solar sails.

Next: Standing Electromagnetic Waves Previous: Electromagnetic Spectrum & Sinusoidal EM Plane Waves Back To Electromagnetism (UY1)

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