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Free Physics Study Material for CSIR NET, IIT JAM, GATE, JEST & TIFR

by Pravegaa Education

Maxwell's Equations

Theory, worked examples and 28 previous-year questions with full solutions — IIT JAM, GATE, CSIR NET-JRF and JEST, 2020 onwards.

Theory
The greatest unification in physics

In 1865, James Clerk Maxwell assembled four equations that unified electricity, magnetism, and optics into a single theory. These equations predict electromagnetic waves, determine how fields behave at boundaries, encode energy flow, momentum, and radiation pressure, and remain exact even in special relativity. Every topic in this book after this chapter is a consequence of Maxwell's equations.

The Continuity Equation

Before Maxwell's correction, Ampère's law read \(\nabla\times\vec{B}=\muz\vec{J}\). Taking the divergence of both sides: \[ \nabla\cdot(\nabla\times\vec{B}) = \muz\,\nabla\cdot\vec{J}. \] The left side is identically zero (div of curl), but \(\nabla\cdot\vec{J}\neq 0\) in general. The continuity equation states:

Continuity Equation — Charge Conservation

\begin{equation} \nabla\cdot\vec{J} = -\frac{\partial\rho}{\partial t} \end{equation} Integral form: \(\oint_\mathcal{S}\vec{J}\cdot d\vec{a} = -\dfrac{d}{dt}\!\int_\mathcal{V}\rho\,d\tau\) (current flowing out = rate of decrease of enclosed charge).

The old Ampère's law is inconsistent unless \(\partial\rho/\partial t=0\). Maxwell fixed this with the displacement current.

Maxwell's Correction: The Displacement Current

From Gauss's law \(\rho=\eps\,\nabla\cdot\vec{E}\); substituting: \[ \nabla\cdot\vec{J} = -\eps\,\nabla\cdot\frac{\partial\vec{E}}{\partial t} \implies \nabla\cdot\!\left(\vec{J}+\eps\frac{\partial\vec{E}}{\partial t}\right)=0. \] Maxwell added \(\eps\,\partial\vec{E}/\partial t\) to Ampère's law:

Displacement Current and Modified Ampère's Law

\begin{equation} \vec{J}_d \equiv \eps\frac{\partial\vec{E}}{\partial t}, \qquad \nabla\times\vec{B} = \muz\vec{J} + \muz\eps\frac{\partial\vec{E}}{\partial t} \end{equation} \(\vec{J}_d\) is not a real current (no charge flows) but generates \(\vec{B}\) exactly like a real current density.

Physical significance of \(J_d\)
  1. Capacitor in AC circuit: \(J_d\) between the plates equals the conduction current in the wires — no discontinuity in \(\vec{B}\).

  2. Electromagnetic waves: changing \(\vec{E}\) creates \(\vec{B}\) (via \(J_d\)), and changing \(\vec{B}\) creates \(\vec{E}\) (Faraday), sustaining a self-propagating wave in vacuum.

Example 3.1   Displacement current in a capacitor

A parallel-plate capacitor (area \(A\)) is charged by current \(I\). Find \(I_d\) and \(\vec{B}\) at radius \(s\) from the axis (\(s<\sqrt{A/\pi}\)).

Step 1: \(E=Q/(\eps A)\), so \(\partial E/\partial t = I/(\eps A)\).

Step 2: \(J_d = \eps\,\partial E/\partial t = I/A\); total \(I_d = J_d\cdot A = I\).

Step 3 (Ampère–Maxwell): \(B(2\pi s) = \muz J_d\pi s^2 = \muz I s^2/A\).

\[\boxed{I_d = I,\qquad \vec{B}=\frac{\muz I s}{2\pi(A/\pi)}\,\phihat}\] The displacement current exactly equals \(I\), ensuring \(\vec{B}\) is the same regardless of which surface is chosen.

Example 3.2   Inconsistency of old Ampère's law

Show explicitly the contradiction in \(\nabla\times\vec{B}=\muz\vec{J}\) for a charging capacitor.

Surface 1 (disk through wire): \(\oint\vec{B}\cdot d\vec{l} = \muz I\).

Surface 2 (balloon between plates): No real current pierces it, so \(\oint\vec{B}\cdot d\vec{l} = 0\).

Same loop, two answers: contradiction.

Resolution: \(J_d=\eps\,\partial E/\partial t\) threads Surface 2 and restores \(\oint\vec{B}\cdot d\vec{l}=\muz I\) for both surfaces. \[\boxed{\text{Inconsistency resolved by }\vec{J}_d=\eps\,\partial\vec{E}/\partial t}\]

Maxwell's Equations — Complete Set

Maxwell's Equations in Vacuum — Differential Form

\begin{align} \nabla\cdot\vec{E} &= \frac{\rho}{\eps} \tag{M1 — Gauss} \\[4pt] \nabla\cdot\vec{B} &= 0 \tag{M2 — No monopoles} \\[4pt] \nabla\times\vec{E} &= -\frac{\partial\vec{B}}{\partial t} \tag{M3 — Faraday} \\[4pt] \nabla\times\vec{B} &= \muz\vec{J} + \muz\eps\frac{\partial\vec{E}}{\partial t} \tag{M4 — Ampère--Maxwell} \end{align}

Maxwell's Equations — Integral Form

\begin{align} \oint_\mathcal{S}\vec{E}\cdot d\vec{a} &= Q_\text{enc}/\eps \tag{M1}\\[4pt] \oint_\mathcal{S}\vec{B}\cdot d\vec{a} &= 0 \tag{M2}\\[4pt] \oint_\mathcal{C}\vec{E}\cdot d\vec{l} &= -d\Phi_B/dt \tag{M3}\\[4pt] \oint_\mathcal{C}\vec{B}\cdot d\vec{l} &= \muz I_\text{enc} + \muz\eps\,d\Phi_E/dt \tag{M4} \end{align}

Maxwell's Equations in Matter

Using \(\vec{D}=\eps\vec{E}+\vec{P}\) and \(\vec{H}=\vec{B}/\muz-\vec{M}\): \begin{align} \nabla\cdot\vec{D} &= \rho_f \tag{M1$'$} \\[4pt] \nabla\cdot\vec{B} &= 0 \tag{M2$'$} \\[4pt] \nabla\times\vec{E} &= -\partial\vec{B}/\partial t \tag{M3$'$} \\[4pt] \nabla\times\vec{H} &= \vec{J}_f + \partial\vec{D}/\partial t \tag{M4$'$} \end{align} Linear media: \(\vec{D}=\eps\varepsilon_r\vec{E}\), \(\vec{B}=\muz\mu_r\vec{H}\).

Physical meaning of each equation

Eq.

Source

Physics

M1

Electric charge \(\rho\)

Charges are sources of \(\vec{E}\) field lines

M2

No magnetic charge

\(\vec{B}\) field lines never start or end

M3

Changing \(\vec{B}\)

Time-varying \(\vec{B}\) curls \(\vec{E}\) (Faraday)

M4

Current + changing \(\vec{E}\)

Both create circulating \(\vec{B}\)

Concept Checks — Maxwell's Equations & Displacement Current

Concept check.

Electric field \(\vec{E}=E_0(3\hat{x}+4\hat{y})e^{i(kz-\omega t)}\). Conclude: (a) Has non-uniform charge distribution   (b) Has no charge   (c) Has time-dependent \(\vec{B}\)   (d) Energy flux zero everywhere

Show answer

(b) and (c). \(\nabla\cdot\vec{E}=0\) (the components do not depend on \(x\) or \(y\)), so \(\rho=0\); and \(\nabla\times\vec{E}\neq0\) with harmonic time dependence, so \(\partial\vec{B}/\partial t\neq0\). The wave carries energy along \(z\), so (d) is false.

Concept check.

Circular loop (radius \(r=0.1\) m) in time-varying \(\vec{B}=10t\,\hat{z}\) T. Magnitude of induced \(E\) (in V/m):

Show answer

\(E(2\pi r)=-d\Phi/dt=-\pi r^2\cdot 10\); \(E=10r/2=0.5\) V/m.

Faraday's Law and Motional EMF

Faraday's Law

\begin{equation} \mathcal{E} = \oint_\mathcal{C}\vec{E}\cdot d\vec{l} = -\frac{d\Phi_B}{dt}, \qquad \Phi_B = \int_\mathcal{S}\vec{B}\cdot d\vec{a}. \end{equation}

Lenz's Law

The induced EMF opposes the change in flux (minus sign). This is a consequence of energy conservation.

Motional EMF

A rod of length \(L\) moving at velocity \(\vec{v}\perp\vec{B}\): \begin{equation} \boxed{\mathcal{E} = \int_\text{rod}(\vec{v}\times\vec{B})\cdot d\vec{l} = vBL} \end{equation}

Universal Flux Rule

Whether EMF arises from a changing \(\vec{B}\) (transformer EMF) or from motion (motional EMF): \[\mathcal{E} = -\frac{d\Phi_B}{dt}\] always holds for any combination of moving loops and changing fields.

Example 3.3   AC generator

A rectangular loop (\(a\times b\)) rotates at \(\omega\) in field \(\vec{B}=B\zhat\).

Flux: \(\Phi_B = Bab\cos(\omega t)\).

EMF: \(\mathcal{E} = Bab\omega\sin(\omega t)\). \[\boxed{\mathcal{E}_0 = Bab\omega}\]

Example 3.4   Sliding rod — motional EMF

Rod of length \(L\), velocity \(v\), field \(B\), circuit resistance \(R\). Find EMF, current, and force needed to maintain constant \(v\).

\(\mathcal{E} = BLv\);   \(I = BLv/R\);   \(F_\text{brake} = BIL = B^2L^2v/R\). \[\boxed{F_\text{applied} = \frac{B^2L^2v}{R}}\] Power input \(= Fv = \mathcal{E}^2/R\) — all dissipated in \(R\). ✓

Example 3.5   Induced \(\vec{E}\) from a changing solenoid

Solenoid of radius \(R\), \(B(t)=B_0\cos(\omega t)\). Find \(\vec{E}\) everywhere.

Inside (\(s<R\)): \[\boxed{\vec{E} = \frac{B_0\omega s}{2}\sin(\omega t)\,\phihat}\]

Outside (\(s>R\)): \[\boxed{\vec{E} = \frac{B_0\omega R^2}{2s}\sin(\omega t)\,\phihat}\] Inside: linear in \(s\). Outside: falls as \(1/s\) — same form as \(B\) outside a wire (Ampère's law), by Faraday–Ampère duality.

Concept Checks — Faraday's Law & Motional EMF

Concept check.

Rectangular loop (\(l\times w\), resistance \(R\)), moving at constant \(v\) away from long wire (current \(I\)). Near side at distance \(d\). Current in loop: (a) \(\dfrac{\muz Ilwv}{2\pi Rd(d+l)}\)   (b) \(\dfrac{\muz Ilv}{2\pi Rd}\)   (c) \(\dfrac{\muz Iwv}{2\pi Rl}\)   (d) \(\dfrac{\muz Ilwv}{2\pi d(d+w)}\)

Show answer

(a). EMF \(= \frac{\muz I}{2\pi}\cdot v\cdot w\cdot\left(\frac{1}{d}-\frac{1}{d+l}\right) = \frac{\muz Ivwl}{2\pi d(d+l)}\). Current \(=\mathcal{E}/R\).

Self-Inductance and Mutual Inductance

Self-Inductance

\begin{equation} \Phi_B = LI,\qquad \boxed{\mathcal{E}_\text{back} = -L\frac{dI}{dt}} \end{equation}

Self-inductance of common geometries

Geometry

\(L\)

Solenoid (\(n\)/m, radius \(R\), length \(l\))

\(\muz n^2\pi R^2 l\)

Toroid (\(N\) turns, inner \(a\), outer \(b\), height \(h\))

\(\dfrac{\muz N^2 h}{2\pi}\ln\!\dfrac{b}{a}\)

Coaxial cable (inner \(a\), outer \(b\), length \(l\))

\(\dfrac{\muz l}{2\pi}\ln\!\dfrac{b}{a}\)

Mutual Inductance

\begin{equation} \Phi_{21} = MI_1,\quad \mathcal{E}_2 = -M\frac{dI_1}{dt},\quad M_{12}=M_{21}\text{ always.} \end{equation}

Neumann Formula

\begin{equation} M = \frac{\muz}{4\pi}\oint_1\oint_2 \frac{d\vec{l}_1\cdot d\vec{l}_2}{|\vec{r}_1-\vec{r}_2|} \end{equation}

Example 3.6   Self-inductance of a solenoid

Solenoid: radius \(R\), length \(l\), \(N\) turns total, \(n=N/l\) turns/m.

\(B=\muz nI\);   total flux linkage \(=N\cdot B\pi R^2 = \muz N^2\pi R^2 I/l\). \[\boxed{L = \muz n^2\pi R^2 l}\]

Example 3.7   Mutual inductance — coaxial solenoids

Short solenoid (length \(l_2\), \(N_2\) turns, radius \(R_2\)) inside a long solenoid (\(n_1\) turns/m, \(R_1>R_2\)).

Flux through inner due to outer current \(I_1\): \(\Phi_{21} = N_2\muz n_1 I_1\pi R_2^2\). \[\boxed{M = \muz n_1 N_2\pi R_2^2}\] Verify by reciprocity: compute flux through outer due to inner current — same result. ✓

Energy in the Electromagnetic Field

Electromagnetic energy storage

\begin{align} U_E &= \tfrac{1}{2}CV^2 = \tfrac{1}{2}\eps\int E^2\,d\tau \\[4pt] U_B &= \tfrac{1}{2}LI^2 = \tfrac{1}{2\muz}\int B^2\,d\tau \end{align} Energy densities: \begin{equation} u_E = \frac{\eps}{2}E^2,\quad u_B = \frac{B^2}{2\muz},\quad u = \frac{1}{2}\!\left(\eps E^2+\frac{B^2}{\muz}\right) \end{equation}

Poynting's Theorem — Derivation

Use M4 to eliminate \(\vec{J}\) from \(\vec{J}\cdot\vec{E}\), then apply the vector identity \(\vec{E}\cdot(\nabla\times\vec{B}) = \vec{B}\cdot(\nabla\times\vec{E}) - \nabla\cdot(\vec{E}\times\vec{B})\) and M3:

Poynting's Theorem

\begin{equation} \frac{\partial u}{\partial t} + \nabla\cdot\vec{S} = -\vec{J}\cdot\vec{E} \end{equation} Poynting vector (energy flux, W/m\(^2\)): \begin{equation} \boxed{\vec{S} = \frac{1}{\muz}\vec{E}\times\vec{B}} \end{equation} Integral form (energy conservation): \begin{equation} -\frac{dU_\text{em}}{dt} = \oint\vec{S}\cdot d\vec{a} + \int\vec{J}\cdot\vec{E}\,d\tau \end{equation}

What Poynting's theorem says

The rate of decrease of EM energy in a volume equals the power flowing out through its surface (via \(\vec{S}\)) plus the power delivered to charges (via \(\vec{J}\cdot\vec{E}\)). Energy propagates through the field, not along the wires.

Example 3.8   Poynting vector — resistive wire

Wire: radius \(a\), length \(L\), resistivity \(\eta\), current \(I\).

\(E_z = \eta I/\pi a^2\) (along wire);   \(B_\phi = \muz I/2\pi a\) (circumferential).

\(\vec{S} = (\vec{E}\times\vec{B})/\muz\) points radially inward.

Power into wire: \(P = |\vec{S}|\cdot 2\pi aL = I^2R\). \[\boxed{P = I^2R}\quad\checkmark\] Joule heating is supplied by energy flowing inward from the surrounding field.

Example 3.9   Energy in a solenoid

Solenoid: \(n\), \(R\), \(l\), current \(I\).

\(u_B = \muz n^2I^2/2\);   \(U = u_B\cdot\pi R^2 l = \frac{1}{2}LI^2\). ✓ \[\boxed{U_B = \frac{1}{2}LI^2}\]

Example 3.10   Poynting vector — charging capacitor

Circular capacitor (radius \(R\), separation \(d\)), voltage \(V(t)\).

\(E=V/d\);   \(B=(\muz\eps R/2d)\,dV/dt\) at edge (\(s=R\)).

Power flowing in: \(P = S\cdot 2\pi Rd = \frac{d}{dt}(\frac{1}{2}CV^2)\). \[\boxed{P = \frac{d}{dt}\!\left(\tfrac{1}{2}CV^2\right)}\quad\checkmark\]

Concept Checks — Energy, Poynting & Momentum

Concept check.

Rectangular loop (\(a\times b\), resistance \(R\)), rotating at \(\omega\) in field \(B\). Maximum induced current:

Show answer

\(\mathcal{E}_\text{max}=Bab\omega\); \(I_\text{max}=Bab\omega/R\).

Electromagnetic Momentum and Radiation Pressure

EM Momentum Density

\begin{equation} \vec{g} = \muz\eps\,\vec{S} = \eps(\vec{E}\times\vec{B}) \qquad[\text{kg/(m}^2\text{s)}] \end{equation}

Radiation Pressure

For EM wave with time-averaged intensity \(I\) (W/m\(^2\)): \begin{equation} P_\text{rad} = \frac{I}{c}\ \text{(absorbed)},\qquad P_\text{rad} = \frac{2I}{c}\ \text{(reflected)} \end{equation}

Maxwell Stress Tensor

\begin{equation} T_{ij} = \eps\!\left(E_iE_j - \tfrac{1}{2}\delta_{ij}E^2\right) + \frac{1}{\muz}\!\left(B_iB_j - \tfrac{1}{2}\delta_{ij}B^2\right) \end{equation} Force on charges in \(\mathcal{V}\): \begin{equation} \vec{F} = \oint_\mathcal{S}\overleftrightarrow{T}\cdot d\vec{a} - \eps\muz\frac{d}{dt}\int_\mathcal{V}\vec{S}\,d\tau. \end{equation}

Maxwell stress tensor components

Uniform field \(\vec{E}=E\zhat\): \[ T_{zz} = +\frac{\eps E^2}{2}\ \text{(tension along field lines)},\quad T_{xx}=T_{yy} = -\frac{\eps E^2}{2}\ \text{(pressure transverse)}. \] Field lines behave like stretched elastic strings.

Example 3.11   EM momentum in crossed fields

\(\vec{E}=E\zhat\), \(\vec{B}=B\xhat\).

\(\vec{S} = EB\yhat/\muz\);   \(\vec{g} = \eps EB\,\yhat\). \[\boxed{\vec{g} = \eps(\vec{E}\times\vec{B}) = \eps EB\,\yhat}\] Even static crossed fields carry momentum — a famous counterintuitive result.

Example 3.12   Force on a capacitor plate via stress tensor

Parallel-plate capacitor, charge \(\pm Q\), area \(A\). Field between plates: \(E=Q/(\eps A)\); outside: \(E=0\).

\(T_{zz}^\text{inside} = -\eps E^2/2\) (pointing toward plate); \(T_{zz}^\text{outside} = 0\).

Force on \(+\) plate: \(F = (T_{zz}^\text{out}-T_{zz}^\text{in})\cdot A = \eps E^2 A/2\). \[\boxed{F = \frac{Q^2}{2\eps A} = \frac{\eps E^2 A}{2}}\] Factor of \(\frac{1}{2}\): plate only feels field on one side.

Boundary Conditions from Maxwell's Equations

Apply Maxwell's equations to a pillbox (for \(\nabla\cdot\)) and rectangular loop (for \(\nabla\times\)) straddling any interface:

General EM Boundary Conditions

\begin{align} D_1^\perp - D_2^\perp &= \sigma_f \\[4pt] B_1^\perp &= B_2^\perp \\[4pt] \vec{E}_1^\parallel &= \vec{E}_2^\parallel \\[4pt] \vec{H}_1^\parallel - \vec{H}_2^\parallel &= \vec{K}_f\times\hat{n}_{12} \end{align} \(\hat{n}_{12}\) points from medium 2 into medium 1.

At a perfect conductor surface

\(\vec{E}=\mathbf{0}\) and \(\vec{B}=\mathbf{0}\) inside. At surface: \(D^\perp=\sigma_f\); \(B^\perp=0\); \(E^\parallel=0\); \(H^\parallel=K_f\).

How to apply BCs — checklist
  1. Choose \(\hat{n}\) pointing from medium 2 to medium 1.

  2. Identify which field components are normal and tangential.

  3. Apply all four BCs above.

  4. Free \(\sigma_f\) and \(K_f\) appear only at conductors or when explicitly stated.

Example 3.13   Refraction of field lines at dielectric interface

Dielectrics with \(\varepsilon_{r1}=2\), \(\varepsilon_{r2}=5\). Field in medium 1 makes \(\theta_1=30\ensuremath{^\circ}\) with normal. No free surface charge. Find \(\theta_2\).

Normal BC: \(\varepsilon_{r1}E_1\cos\theta_1 = \varepsilon_{r2}E_2\cos\theta_2\).

Tangential BC: \(E_1\sin\theta_1 = E_2\sin\theta_2\).

Dividing: \(\tan\theta_2 = (\varepsilon_{r2}/\varepsilon_{r1})\tan\theta_1 = (5/2)\tan30\ensuremath{^\circ} = 5/(2\sqrt{3})\). \[\boxed{\theta_2 \approx 55.3\ensuremath{^\circ}}\] Field bends away from normal entering denser dielectric (\(\varepsilon_{r2}>\varepsilon_{r1}\)).

Gauge Transformations and Potentials

Since \(\nabla\cdot\vec{B}=0\), write \(\vec{B}=\nabla\times\vec{A}\). Faraday's law then gives \(\vec{E}=-\nabla V-\partial\vec{A}/\partial t\).

EM Potentials

\begin{equation} \vec{E} = -\nabla V - \frac{\partial\vec{A}}{\partial t},\qquad \vec{B} = \nabla\times\vec{A} \end{equation}

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