Unit 5: Maxwell's Equations

14โ€“17% of AP Exam ยท 5 Subsections ยท ~8 Practice Questions

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5.1 Gauss's Law for Electric Fields

Maxwell Equation 1: Electric charges are sources of electric fields.

$$\oint \vec{E} \cdot d\vec{A} = \frac{Q_{\text{enc}}}{\varepsilon_0}$$

Electric field lines start on + charges and end on โˆ’ charges. Net flux through a closed surface is proportional to enclosed charge. Differential form: \(\nabla \cdot \vec{E} = \rho/\varepsilon_0\).

Exam Tip The AP exam may ask you to identify which Maxwell equation applies to a given situation. This one: "net electric flux through closed surface = enclosed charge over epsilon-zero."

5.2 Gauss's Law for Magnetic Fields

Maxwell Equation 2: No magnetic monopoles exist.

$$\oint \vec{B} \cdot d\vec{A} = 0$$

B-field lines are always closed loops โ€” they never start or end. Net B-flux through any closed surface = 0. Cut a bar magnet in half โ†’ two smaller magnets, each with N and S. Differential form: \(\nabla \cdot \vec{B} = 0\).

Common Mistake Through a closed surface, net B-flux = 0. Through an open surface, B-flux can be non-zero โ€” that's what Faraday's Law describes.

5.3 Faraday's Law

Maxwell Equation 3: Changing B creates a circulating E-field.

$$\oint \vec{E} \cdot d\vec{\ell} = -\frac{d\Phi_B}{dt}$$

Time-varying B induces a non-conservative E-field (\(\oint\vec{E}\cdot d\vec{\ell} \neq 0\)). This drives current in conductors โ€” the principle behind generators. Differential form: \(\nabla \times \vec{E} = -\partial\vec{B}/\partial t\).

Practice

Q5.1: Identity the Maxwell Equation

A time-varying B-field through a loop induces circulating E-field: \(\oint\vec{E}\cdot d\vec{\ell} = -d\Phi_B/dt\). Which Maxwell equation is this?

Show Solution
Faraday's Law (Maxwell Equation 3). Describes induction โ€” changing B produces curling E. Principle of transformers and generators.

5.4 The Ampere-Maxwell Law

Maxwell Equation 4: Currents AND changing E-fields create B-fields.

$$\oint \vec{B} \cdot d\vec{\ell} = \mu_0 I_{\text{enc}} + \mu_0\varepsilon_0 \frac{d\Phi_E}{dt}$$

Maxwell's crucial addition is the displacement current term: \(I_d = \varepsilon_0\frac{d\Phi_E}{dt}\). Even between capacitor plates (no moving charges), a changing E acts as an effective current producing B-field.

Without this term, Ampere's law is inconsistent for time-varying scenarios. Differential form: \(\nabla \times \vec{B} = \mu_0\vec{J} + \mu_0\varepsilon_0\frac{\partial\vec{E}}{\partial t}\).

Critical The displacement current was Maxwell's great theoretical contribution. It completes the symmetry: changing E โ†’ B (this), changing B โ†’ E (Faraday). Together they predict EM waves.
Practice

Q5.2: Displacement Current

Parallel-plate capacitor (radius 5.0 cm) charges with \(E(t)=1.0\times10^6t\ \text{V/mยทs}\). Find displacement current density and B at r=3.0 cm.

Show Solution
\(J_d = \varepsilon_0 dE/dt = 8.85\times10^{-6}\ \text{A/m}^2\). Total \(I_d = J_d\cdot\pi R^2 = 6.95\times10^{-8}\ \text{A}\).
Ampere-Maxwell for r

5.5 Electromagnetic Waves

Maxwell's equations predict self-sustaining EM waves โ€” propagating oscillations of E and B requiring no medium.

Speed of light:

$$c = \frac{1}{\sqrt{\mu_0\varepsilon_0}} = 3.00 \times 10^8\ \text{m/s}$$

Plane wave structure:

  • \(\vec{E} \perp \vec{B} \perp \vec{v}\) โ€” mutually perpendicular
  • E and B are in phase: \(E = E_0\sin(kx-\omega t)\), \(B = B_0\sin(kx-\omega t)\)
  • Amplitude: \(E_0 = cB_0\)
  • Propagation direction: \(\vec{E} \times \vec{B}\)

Poynting vector = energy flux (W/mยฒ): \(\vec{S} = \frac{1}{\mu_0}\vec{E} \times \vec{B}\)

Average intensity: \(I = \langle S \rangle = \frac{1}{2}c\varepsilon_0 E_0^2 = \frac{E_0^2}{2\mu_0 c}\)

Radiation pressure: \(p = I/c\) (perfect absorber), \(p = 2I/c\) (perfect reflector).

RMS Values: For sinusoidal waves: \(E_{\text{rms}} = E_0/\sqrt{2}\), \(B_{\text{rms}} = B_0/\sqrt{2}\). Average intensity: \(I = \frac{1}{2}c\varepsilon_0 E_0^2 = c\varepsilon_0 E_{\text{rms}}^2\).

Energy density in EM waves: \(u = \varepsilon_0 E^2 = B^2/\mu_0\) (instantaneous). Average: \(\langle u \rangle = \frac{1}{2}\varepsilon_0 E_0^2 = \varepsilon_0 E_{\text{rms}}^2\).

$$c = \lambda f = 3.00 \times 10^8\ \text{m/s}$$
Practice

Q5.3: EM Wave Direction

An EM wave has \(\vec{E}=100\sin(ky+\omega t)\hat{x}\ \text{V/m}\). Find propagation direction and \(\vec{B}(y,t)\).

Show Solution
Argument \((ky+\omega t)\) โ†’ plus sign between k and ฯ‰ means propagation in โˆ’y direction.
\(\vec{v} \propto \vec{E}\times\vec{B}\): (โˆ’ฤต) โˆ รฎ ร— Bฬ‚ โ†’ B must be along +kฬ‚ (รฎร—kฬ‚ = โˆ’ฤต โœ“).
\(B_0 = E_0/c = 100/(3\times10^8) = 3.33\times10^{-7}\ \text{T}\). \(\vec{B}=3.33\times10^{-7}\sin(ky+\omega t)\hat{z}\ \text{T}\).
Practice

Q5.4: Intensity and Radiation Pressure

EM wave: \(E_0=150\ \text{V/m}\). Find average intensity and radiation pressure on a perfect absorber.

Show Solution
\(I = \frac{1}{2}c\varepsilon_0 E_0^2 = 0.5(3\times10^8)(8.85\times10^{-12})(22500) = 29.9\ \text{W/m}^2\).
\(p = I/c = 29.9/(3\times10^8) = 1.0\times10^{-7}\ \text{Pa}\). Very small โ€” why solar sails need large area.
Practice

Q5.5: Maxwell Summary

Match each to its description:
(a) \(\oint\vec{E}\cdot d\vec{A}=Q_{\text{enc}}/\varepsilon_0\) โ€” (i) No magnetic monopoles
(b) \(\oint\vec{B}\cdot d\vec{A}=0\) โ€” (ii) Changing B makes E
(c) \(\oint\vec{E}\cdot d\vec{\ell}=-d\Phi_B/dt\) โ€” (iii) Charges make E
(d) \(\oint\vec{B}\cdot d\vec{\ell}=\mu_0 I+\mu_0\varepsilon_0 d\Phi_E/dt\) โ€” (iv) Current + changing E makes B

Show Solution
(a)โ†’(iii): Gauss's Law for E โ€” charges produce electric fields.
(b)โ†’(i): Gauss's Law for B โ€” no magnetic monopoles; B lines are closed loops.
(c)โ†’(ii): Faraday's Law โ€” changing magnetic flux induces circulating E-field.
(d)โ†’(iv): Ampere-Maxwell Law โ€” conduction current AND displacement current produce B-field.