Electromagnetic Waves
Light as travelling electric and magnetic fields.
Displacement Current
A changing electric field makes a magnetic field.
A changing magnetic field makes an electric field. Maxwell realised the reverse must also hold, and adding that one term to Ampère’s law turned electricity and magnetism into a theory of light.
Where Ampère’s law fails
Ampère’s law, ∮B⃗·dl⃗ = μ₀i, holds only while the electric field through the loop is steady. Charge a capacitor with circular plates and put a compass between the plates: it deflects, so there is a magnetic field there. Take a loop γ lying between the plates, parallel to them. Its circulation of B is not zero, yet no charge crosses the flat surface it bounds: i = 0. And the field due to the currents in the wires alone, worked out from Biot–Savart, would give zero circulation. Something else between the plates makes magnetic field: the changing electric field.
The displacement current
Just as Faraday’s law says ∮E⃗·dl⃗ = −dΦB/dt, a changing electric flux makes a magnetic circulation:
With both a current and a changing electric field present, Maxwell’s generalised Ampère’s law is:
Show that while a parallel-plate capacitor is charging, the displacement current through the whole region between the plates equals the current in the wires.
A capacitor of plate area A is charged by a steady current i. What displacement current passes through an area A/3 between the plates, parallel to them?
Circular plates of radius 5.0 cm are charged at 0.50 A. Find B between them 3.0 cm from the axis, and outside the plates 10 cm from the axis.
Current is always continuous
If charge piles up inside a closed surface, conduction current i₁ in exceeds i₂ out: d(qinside)/dt = i₁ − i₂. By Gauss’s law ΦE = qinside/ε₀, so ε₀ dΦE/dt = d(qinside)/dt, i.e. id = i₁ − i₂.
Counting displacement current, as much current flows out of any closed surface as flows in.
- 1Ampère's law ∮B⃗·dl⃗ = μ₀i fails when E changes (charging capacitor).
- 2A changing electric flux makes B: displacement current i_d = ε₀ dΦ_E/dt.
- 3∮B⃗·dl⃗ = μ₀(i_c + i_d) (40.3).
- 4Total current (conduction + displacement) is continuous.
Check yourself
Videos, simulations & further reading (3)
Maxwell's Equations & EM Waves
Four equations, and light falls out.
Four equations sum up all of electricity and magnetism. In empty space they have a remarkable solution: a wave of electric and magnetic fields that travels at exactly the speed of light.
Maxwell’s equations
| Law | Equation | Says |
|---|---|---|
| Gauss (electricity) | ∮E⃗·dS⃗ = q/ε₀ | charges are sources of E |
| Gauss (magnetism) | ∮B⃗·dS⃗ = 0 | no magnetic poles |
| Faraday | ∮E⃗·dl⃗ = −dΦ_B/dt | changing B makes E |
| Ampère–Maxwell | ∮B⃗·dl⃗ = μ₀i + μ₀ε₀ dΦ_E/dt | currents and changing E make B |
In vacuum there are no charges or currents, leaving
A plane wave
Try a wave travelling along x, with E along y and B along z:
Faraday’s law on a rectangle in the x–y plane (sides at x₁ and x₂, height l): the circulation of E is E₀l[sin ω(t − x₂/c) − sin ω(t − x₁/c)], and −dΦB/dt works out to cB₀l times the same bracket. They agree if
Ampère–Maxwell law on a rectangle in the x–z plane does the same job for B and gives B₀ = μ₀ε₀cE₀. Together with E₀ = cB₀:
With μ₀ and ε₀ measured in purely electrical and magnetic experiments, this gave c = 2.99793 × 10⁸ m/s: the measured speed of light. That was the proof that light is an electromagnetic wave. (Today c and μ₀ are fixed by definition and ε₀ is defined through this equation.)
A plane wave travelling along x has its electric field along y with a maximum of 450 N/C. Find the maximum magnetic field and its direction.
A wave along x has wavelength 3.0 cm and its electric field along y with amplitude 60 V/m. Write E and B as functions of x and t.
- 1Maxwell's four equations describe all of electromagnetism.
- 2In vacuum they allow plane waves with E ⊥ B ⊥ direction of travel, in phase.
- 3E₀ = cB₀ (40.5); c = 1/√(μ₀ε₀) (40.6): light is an electromagnetic wave.
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Videos, simulations & further reading (7)
Energy, Intensity & Radiation Pressure
Light carries energy and pushes.
Sunlight warms your face and pushes on solar sails. An electromagnetic wave carries both energy and momentum, shared equally between its electric and magnetic fields.
Energy density
In a small volume of the wave the energy is ½ε₀E² dV (electric) plus B²dV/2μ₀ (magnetic). With E = E₀ sin ω(t − x/c) and B = B₀ sin ω(t − x/c), and sin² averaging to ½:
Using E₀ = cB₀ and μ₀ε₀ = 1/c², the two terms are equal: on average the electric and magnetic fields carry the same energy.
A wave has E = (80 N/C) sin ω(t − x/c). How much energy is in a cylinder of cross-section 20 cm² and length 1.0 m along x?
Intensity
Intensity is the energy crossing unit area per unit time, perpendicular to the direction of travel. The energy in a cylinder of area A and length cΔt (uavcΔtA) crosses A in time Δt, so
Find the intensity of the wave above.
Momentum and radiation pressure
A portion of the wave carrying energy U also carries momentum
- Fully absorbed: the surface receives momentum U/c; the pressure is I/c.
- Fully reflected: the momentum reverses (p → −p), the surface receives 2U/c; the pressure is 2I/c.
Sunlight of intensity 1.36 kW/m² falls on a perfectly reflecting sail 100 m × 100 m, square-on. Find the force. Also find the peak electric field of sunlight.
- 1u_av = ½ε₀E₀² = B₀²/2μ₀ (40.7–40.8); electric and magnetic shares are equal.
- 2Intensity I = u_av c = ½ε₀E₀²c (40.9).
- 3Momentum p = U/c (40.10); pressure I/c absorbed, 2I/c reflected.
Check yourself
The EM Spectrum & the Atmosphere
One kind of wave over a vast range of wavelengths.
Maxwell’s equations don’t pick a wavelength. Radio waves, microwaves, light and gamma rays are the same phenomenon over an enormous range of scales.
The electromagnetic spectrum
Visible light spans only about 380–780 nm. Known electromagnetic waves stretch from about 30 fm (30 × 10⁻¹⁵ m) to 30 km. All travel at c in vacuum, so frequency and wavelength are tied by ν = c/λ. The boundaries between named regions are not sharp; gamma rays and X-rays overlap a good deal, and it is only on average that gamma rays are shorter.
Sources and uses
Every electromagnetic wave comes ultimately from accelerated charges, whose changing fields make up the wave.
- Radio waves: charges oscillating in LC circuits; radio and TV broadcasting.
- Microwaves: oscillating currents in electric circuits; radar, cooking, communication.
- Infrared: emitted by atoms and molecules of hot bodies; used in physiotherapy.
- Visible light: emitted by atoms, linked to the acceleration of their electrons.
- Ultraviolet: produced the same way; the Sun emits a lot, harmful in large doses.
- X-rays: most commonly from fast electrons slowing down in a metal target; medical diagnosis, harmful to tissue.
- Gamma rays: emitted by atomic nuclei; the shortest wavelengths we usually meet.
Find the wavelength of an FM station at 100 MHz and of a microwave oven at 2.45 GHz, and the frequency of 0.10 nm X-rays.
Radiation and the atmosphere
The atmosphere reaches about 300 km up, in rough layers without sharp boundaries:
- Troposphere, up to about 12 km: almost all clouds, water vapour and ice. Air at its top is about a tenth as dense as at the ground.
- Stratosphere, 12–50 km, with the ozone layer in its upper part; air at its top is about 10⁻³ times as dense as at the ground.
- Mesosphere, about 50–80 km; above it, the ionosphere.
The Sun is the main source of radiation reaching us, and much of it is absorbed on the way down. Visible light is only weakly absorbed. Much of the infrared is absorbed and heats the air. The ozone layer absorbs most of the ultraviolet and shorter wavelengths, converting it to infrared that heats the atmosphere and ground, and so protects living things.
- 1One spectrum from ≈ 30 fm to 30 km: gamma, X-ray, UV, visible (380–780 nm), IR, microwave, radio; ν = c/λ.
- 2All are produced by accelerated charges.
- 3Atmosphere: troposphere, stratosphere (ozone), mesosphere, ionosphere.
- 4Ozone absorbs UV; IR is largely absorbed low down; visible light mostly gets through.