Unit 1: Electromagnetic Theory
1. Vector Calculus and Differential Field Operators
Electromagnetic theory describes the behavior of electric charges, currents, and electromagnetic radiation through spatial vector and scalar fields. A scalar field maps a scalar value to every coordinate in space (e.g., electric potential or temperature ), whereas a vector field assigns a directed magnitude (e.g., electric field intensity ec{E}(x, y, z) or magnetic flux density ec{B}(x, y, z)).
CODEVector Field Classification: ├── Irrotational / Conservative: ∇ × A = 0 (Can be expressed as A = -∇V) ├── Solenoidal / Divergence-free: ∇ · A = 0 (Can be expressed as A = ∇ × Ψ) └── General Helmholtz Vector: A = -∇V + ∇ × Ψ (Superposition of irrotational & solenoidal)
1.1 The Gradient of a Scalar Field ($
abla \phi
abla\phi(x,y,z)\phi$. Its magnitude equals that maximal directional rate of increase:
abla \cdot ec{A} = \lim_{\Delta V o 0} rac{1}{\Delta V} \oiint_S ec{A} \cdot dec{S} = rac{\partial A_x}{\partial x} + rac{\partial A_y}{\partial y} + rac{\partial A_z}{\partial z}$$
- Physical Significance:
- abla \cdot ec{A} > 0: The point acts as a net positive source (e.g., positive electric charge creating diverging ec{E}).
- abla \cdot ec{A} < 0: The point acts as a net negative sink (e.g., negative electric charge absorbing ec{E}).
- abla \cdot ec{A} = 0: The vector field is solenoidal (no isolated sources or sinks; field lines form closed, continuous loops, as in ec{B}).
1.3 The Curl of a Vector Field ($
abla imes ec{A}$)
The curl evaluates the circulation density or rotational vorticity of a vector field per unit area around an infinitesimal closed loop:
abla imes ec{A} = egin{vmatrix} \hat{i} & \hat{j} & \hat{k} \ rac{\partial}{\partial x} & rac{\partial}{\partial y} & rac{\partial}{\partial z} \ A_x & A_y & A_z \end{vmatrix} = \left(rac{\partial A_z}{\partial y} - rac{\partial A_y}{\partial z}
ight)\hat{i} + \left(rac{\partial A_x}{\partial z} - rac{\partial A_z}{\partial x}
ight)\hat{j} + \left(rac{\partial A_y}{\partial x} - rac{\partial A_x}{\partial y}
ight)\hat{k}$$
- Physical Significance:
- abla imes ec{A} e 0: The field contains rotational circulation (e.g., magnetic field circling an electric current).
- abla imes ec{A} = 0: The field is irrotational or conservative (e.g., static electrostatic field).
1.4 Fundamental Vector Identities and the Laplacian Operator
Two foundational null identities underpin classical electromagnetic gauge theory:
- The Curl of a Gradient is Identically Zero:
abla \cdot (
abla imes ec{A}) = 0$$
Physical Consequence: Any solenoidal vector field ec{B} ( abla \cdot ec{B} = 0) can be represented as the curl of a magnetic vector potential: ec{B} = abla imes ec{A}.
- The Laplacian Operator ():
- For a scalar field: abla^2 \phi = abla \cdot ( abla \phi) = rac{\partial^2 \phi}{\partial x^2} + rac{\partial^2 \phi}{\partial y^2} + rac{\partial^2 \phi}{\partial z^2}
- Vector Laplacian identity: abla^2 ec{A} = abla( abla \cdot ec{A}) - abla imes ( abla imes ec{A})
1.5 Integral Calculus: Gauss's Divergence Theorem and Stokes' Theorem
CODE[Gauss's Divergence Theorem] Closed Surface Integral ◄───► Volume Integral ∬_S A · dS = ∭_V (∇ · A) dV ▲ │ [Stokes' Curl Theorem] Closed Line Integral ◄───► Open Surface Integral ∮_C A · dr = ∬_S (∇ × A) · dS
- Gauss's Divergence Theorem: Transforms a flux integral over a closed boundary surface enclosing volume into an integral of the divergence over the enclosed volume:
abla \cdot ec{E} = rac{
ho}{arepsilon_0} \quad \implies \quad
abla \cdot ec{D} =
ho_f$$
Where ec{D} = arepsilon ec{E} = arepsilon_0 ec{E} + ec{P} is the electric displacement vector, ec{P} is the electric polarization vector, and is the volume density of free charges.
2.2 Electrostatic Potential and Laplace/Poisson Equations
Because static electric fields are irrotational ( abla imes ec{E} = 0), the electric field can be expressed as the negative gradient of an electrostatic scalar potential :
abla V$$ Substituting this relation into Gauss's differential law yields **Poisson's Equation**:abla \cdot (-
abla V) = rac{
ho}{arepsilon} \implies
abla^2 V = -rac{
ho}{arepsilon}$$
In charge-free regions (), Poisson's equation reduces to Laplace's Equation:
abla^2 V = 0 \iff rac{\partial^2 V}{\partial x^2} + rac{\partial^2 V}{\partial y^2} + rac{\partial^2 V}{\partial z^2} = 0$$ - **Uniqueness Theorem:** A solution to Laplace's equation in a given volume $V$ is uniquely determined if the potential $V$ (Dirichlet boundary condition) or its normal derivative $\partial V / \partial n$ (Neumann boundary condition) is specified on the bounding surface. ### 2.3 Magnetostatics, Biot-Savart Law, and Ampère's Circuital Law The magnetic field generated by a steady current element $I dec{l}$ is governed by the Biot-Savart Law: $$dec{B} = rac{\mu_0}{4\pi} rac{I dec{l} imes \hat{r}}{r^2}$$ Ampère's Circuital Law states that the line integral of magnetic field $ec{B}$ around any closed closed loop $C$ is proportional to the net enclosed conduction current $I_{enc}$: $$\oint_C ec{B} \cdot dec{l} = \mu_0 I_{enc} = \mu_0 \iint_S ec{J} \cdot dec{S}$$ Applying Stokes' Theorem gives the differential form of Ampère's Law for static currents:abla imes ec{B} = \mu_0 ec{J} \quad \iff \quad
abla imes ec{H} = ec{J}_f$$
Because magnetic monopoles do not exist in nature, magnetic flux lines form continuous loops, establishing Gauss's Law for Magnetism:
abla \cdot ec{B} = 0$$ This identity implies that $ec{B}$ can always be written as the curl of a **Magnetic Vector Potential** $ec{A}$: $$ec{B} = abla imes ec{A}$$ Under the Coulomb gauge condition ($ abla \cdot ec{A} = 0$), magnetostatics satisfies a vector Poisson equation:abla^2 ec{A} = -\mu_0 ec{J}$$
3. Electrodynamics and Maxwell's Formulation
3.1 Faraday's Law of Electromagnetic Induction
Michael Faraday demonstrated that a time-varying magnetic flux induces an electromotive force (EMF) in a closed conductive circuit:
\mathcal{E} = -rac{d\Phi_B}{dt} = -rac{d}{dt} \iint_S ec{B} \cdot dec{S}
The negative sign embodies Lenz's Law (conservation of energy). Using Stokes' Theorem:
abla imes ec{E} = -rac{\partial ec{B}}{\partial t}$$ This differential equation proves that time-dependent magnetic fields generate non-conservative, rotational electric fields. ### 3.2 Inconsistency of Ampère's Law and Maxwell's Displacement Current Consider the divergence of the static Ampère's law:abla \cdot (
abla imes ec{H}) =
abla \cdot ec{J}$$
From vector calculus, the divergence of any curl is identically zero: abla \cdot ( abla imes ec{H}) \equiv 0. Consequently, static Ampère's law demands:
abla \cdot ec{J} = 0$$ However, the fundamental law of **Conservation of Electric Charge** is expressed by the **Continuity Equation**:abla \cdot ec{J} + rac{\partial
ho}{\partial t} = 0 \implies
abla \cdot ec{J} = -rac{\partial
ho}{\partial t}$$
In time-varying scenarios (such as charging a capacitor), , exposing a fatal mathematical contradiction in Ampère's static formulation.
CODECharging Capacitor Circuit Dilemma: Plate +Q Plate -Q ─────────────| |───────────── Current I_c | | (Dielectric) Current I_c | | Conduction | | Displacement Conduction Current J_c | | Current J_d Current J_c
To resolve this inconsistency, James Clerk Maxwell recognized that Gauss's Law relates charge density to electric displacement:
ho = abla \cdot ec{D}$$ Differentiating with respect to time: $$rac{\partial ho}{\partial t} = rac{\partial}{\partial t}( abla \cdot ec{D}) = abla \cdot \left(rac{\partial ec{D}}{\partial t} ight)$$ Substituting into the continuity equation:abla \cdot ec{J} +
abla \cdot \left(rac{\partial ec{D}}{\partial t}
ight) = 0 \implies
abla \cdot \left( ec{J} + rac{\partial ec{D}}{\partial t}
ight) = 0$$
Maxwell postulated that total current density consists of conduction current density ec{J}_c and Displacement Current Density ec{J}_d:
ec{J}_d = rac{\partial ec{D}}{\partial t} = arepsilon_0 rac{\partial ec{E}}{\partial t} + rac{\partial ec{P}}{\partial t}
Displacement current represents a changing electric flux; it carries no physical charge carriers through space yet generates an identical surrounding magnetic field.
3.3 The Complete Set of Maxwell's Equations
| Law Name | Differential Form | Integral Form | Physical Significance |
|---|---|---|---|
| Gauss's Law for Electricity | $ | ||
| abla \cdot ec{D} = | |||
| ho_f$ | \oiint_S ec{D} \cdot dec{S} = Q_{f, ext{enc}} | Electric charges act as divergent sources and sinks of electric flux. | |
| Gauss's Law for Magnetism | $ | ||
| abla \cdot ec{B} = 0$ | \oiint_S ec{B} \cdot dec{S} = 0 | Magnetic monopoles do not exist; magnetic lines are continuous closed loops. | |
| Faraday's Law of Induction | $ | ||
| abla imes ec{E} = -rac{\partial ec{B}}{\partial t}$ | \oint_C ec{E} \cdot dec{l} = -rac{d}{dt}\iint_S ec{B} \cdot dec{S} | A time-varying magnetic field induces a rotational electric field. | |
| Ampère-Maxwell Law | $ | ||
| abla imes ec{H} = ec{J}_f + rac{\partial ec{D}}{\partial t}$ | \oint_C ec{H} \cdot dec{l} = I_{f} + \iint_S rac{\partial ec{D}}{\partial t} \cdot dec{S} | Magnetic fields are generated by conduction currents and changing electric fields. |
In isotropic, linear, and homogeneous media, the constitutive relations apply:
ec{D} = arepsilon ec{E} = arepsilon_r arepsilon_0 ec{E}, \quad ec{B} = \mu ec{H} = \mu_r \mu_0 ec{H}, \quad ec{J} = \sigma ec{E}
4. Electromagnetic Wave Equations and Propagation in Media
4.1 Derivation of the Electromagnetic Wave Equation in Free Space
In source-free, non-conducting vacuum ( ho = 0, ec{J} = 0, \sigma = 0, arepsilon = arepsilon_0, \mu = \mu_0), Maxwell's equations simplify to:
- abla \cdot ec{E} = 0
- abla \cdot ec{B} = 0
- abla imes ec{E} = -rac{\partial ec{B}}{\partial t}
- abla imes ec{B} = \mu_0 arepsilon_0 rac{\partial ec{E}}{\partial t}
Taking the curl of Faraday's Law:
abla imes ( abla imes ec{E}) = abla imes \left( -rac{\partial ec{B}}{\partial t} ight) = -rac{\partial}{\partial t}( abla imes ec{B})$$ Invoking the vector Laplacian identity $ abla imes ( abla imes ec{E}) = abla( abla \cdot ec{E}) - abla^2 ec{E}$, and noting that $ abla \cdot ec{E} = 0$: $$- abla^2 ec{E} = -rac{\partial}{\partial t}\left(\mu_0 arepsilon_0 rac{\partial ec{E}}{\partial t} ight) = -\mu_0 arepsilon_0 rac{\partial^2 ec{E}}{\partial t^2}$$abla^2 ec{E} - \mu_0 arepsilon_0 rac{\partial^2 ec{E}}{\partial t^2} = 0$$
Similarly, taking the curl of the Ampère-Maxwell law yields the wave equation for the magnetic field:
abla^2 ec{B} - \mu_0 arepsilon_0 rac{\partial^2 ec{B}}{\partial t^2} = 0$$ Comparing this with the classical 3D d'Alembert wave equation $ abla^2 \psi - rac{1}{v^2}rac{\partial^2 \psi}{\partial t^2} = 0$, the propagation velocity $c$ is: $$c = rac{1}{\sqrt{\mu_0 arepsilon_0}} = rac{1}{\sqrt{(4\pi imes 10^{-7} ext{ H/m})(8.854 imes 10^{-12} ext{ F/m})}} pprox 2.998 imes 10^8 ext{ m/s}$$ This theoretical prediction confirmed that light is an electromagnetic wave. ### 4.2 Properties of Plane Electromagnetic Waves in Free Space For a monochromatic plane wave propagating along the $+z$ direction with angular frequency $\omega$ and wave number $k = \omega / c$: $$ec{E}(z, t) = E_0 \cos(kz - \omega t) \hat{i}$$ Substituting into Faraday's Law $ abla imes ec{E} = -rac{\partial ec{B}}{\partial t}$: $$rac{\partial E_x}{\partial z}\hat{j} = -k E_0 \sin(kz - \omega t)\hat{j} = -rac{\partial ec{B}}{\partial t}$$ Integrating with respect to time: $$ec{B}(z, t) = rac{k}{\omega} E_0 \cos(kz - \omega t) \hat{j} = rac{E_0}{c} \cos(kz - \omega t) \hat{j}$$ ``` Electromagnetic Plane Wave Architecture: E-field (x-axis) ▲ │ / B-field (y-axis) │ / │ / ─────────┼──/──────────► Propagation k (z-axis) /│ / │ / ▼ ``` - **Transverse Nature:** $ec{E} \cdot ec{k} = 0$ and $ec{B} \cdot ec{k} = 0$. Both electric and magnetic field vectors are mutually perpendicular to each other and perpendicular to the direction of propagation $ec{k}$. - **Phase Alignment:** In lossless media, $ec{E}$ and $ec{B}$ oscillate strictly in phase, reaching zero-crossings and extrema simultaneously. - **Intrinsic Impedance of Free Space ($\eta_0$):** The ratio of the electric field amplitude to the magnetic field intensity $H = B/\mu_0$: $$\eta_0 = rac{E_0}{H_0} = rac{E_0}{B_0 / \mu_0} = c \mu_0 = \sqrt{rac{\mu_0}{arepsilon_0}} pprox 376.73\ \Omega pprox 120\pi\ \Omega$$ ### 4.3 Wave Propagation in Conducting Media and Skin Depth In a conducting medium with conductivity $\sigma > 0$, Ohm's law $ec{J} = \sigma ec{E}$ introduces an attenuation term:abla^2 ec{E} - \mu \sigma rac{\partial ec{E}}{\partial t} - \mu arepsilon rac{\partial^2 ec{E}}{\partial t^2} = 0$$
Assuming time-harmonic solutions of the form , the complex propagation constant \gamma = lpha + ieta is:
\gamma^2 = -\omega^2 \mu arepsilon + i\omega \mu \sigma
Where:
- lpha: Attenuation constant (nepers/meter)
- eta: Phase propagation constant (radians/meter)
For a good conductor (rac{\sigma}{\omega arepsilon} \gg 1):
lpha pprox eta pprox \sqrt{rac{\omega \mu \sigma}{2}} = \sqrt{\pi f \mu \sigma}
The electric field decays exponentially as it penetrates the conductor:
ec{E}(z, t) = E_0 e^{-lpha z} \cos(eta z - \omega t) \hat{i}
- Skin Depth (): The penetration distance over which the wave amplitude attenuates to (pprox 36.8\%) of its initial surface value:
\delta = rac{1}{lpha} = \sqrt{rac{2}{\omega \mu \sigma}} = rac{1}{\sqrt{\pi f \mu \sigma}}
High-Frequency Implications: At microwave and radio frequencies, electrical conduction is confined exclusively to a microscopic outer layer of the conductor, increasing effective AC resistance.
5. Poynting Vector and Energy Conservation
5.1 Poynting's Theorem
Electromagnetic fields store potential and kinetic energy in space. The instantaneous volumetric energy density is the sum of electrostatic and magnetostatic energy densities:
u = u_E + u_B = rac{1}{2}arepsilon |ec{E}|^2 + rac{1}{2\mu}|ec{B}|^2 = rac{1}{2}(ec{E} \cdot ec{D} + ec{B} \cdot ec{H})
Differentiating with respect to time:
rac{\partial u}{\partial t} = ec{E} \cdot rac{\partial ec{D}}{\partial t} + ec{H} \cdot rac{\partial ec{B}}{\partial t}
Invoking Maxwell's curl equations (rac{\partial ec{D}}{\partial t} = abla imes ec{H} - ec{J} and rac{\partial ec{B}}{\partial t} = - abla imes ec{E}):
abla imes ec{H} - ec{J}) - ec{H} \cdot ( abla imes ec{E})$$ Using the vector identity $ abla \cdot (ec{E} imes ec{H}) = ec{H} \cdot ( abla imes ec{E}) - ec{E} \cdot ( abla imes ec{H})$: $$-rac{\partial u}{\partial t} = abla \cdot (ec{E} imes ec{H}) + ec{J} \cdot ec{E}$$ Defining the **Poynting Vector** $ec{S}$: $$ec{S} = ec{E} imes ec{H} = rac{1}{\mu_0}(ec{E} imes ec{B})$$ Integrating over a volume $V$ bounded by surface $S$: $$-rac{d}{dt}\iiint_V u dV = \oiint_S ec{S} \cdot dec{S} + \iiint_V (ec{J} \cdot ec{E}) dV$$ ``` Poynting Energy Flow Balance: [Rate of Energy Loss in Volume] = [Net EM Flux Leaving Boundary] + [Ohmic Joule Heating Work] ``` ### 5.2 Time-Average Poynting Flux (Radiation Intensity) For harmonic waves, the instantaneous Poynting vector oscillates at frequency $2\omega$. The observable physical energy transport is quantified by the **Time-Average Poynting Vector** $\langle ec{S} angle$: $$\langle ec{S} angle = rac{1}{T} \int_0^T ec{S}(t) dt = rac{1}{2} ext{Re}(ec{E} imes ec{H}^*)$$ For a plane wave in free space: $$\langle ec{S} angle = rac{E_0^2}{2\eta_0}\hat{k} = rac{1}{2} c arepsilon_0 E_0^2 \hat{k} \quad [ ext{Watts / m}^2]$$ - **Radiation Pressure ($P_{rad}$):** Electromagnetic waves carry linear momentum density $ec{p} = ec{S} / c^2$. When incident upon an absorbing surface: $$P_{rad} = rac{\langle S angle}{c} \quad ( ext{Complete Absorption}); \quad P_{rad} = rac{2\langle S angle}{c} \quad ( ext{Complete Reflection})$$ --- ## 6. Boundary Conditions at Material Interfaces When electromagnetic fields cross the interface between two differing physical media (Medium 1 with $arepsilon_1, \mu_1, \sigma_1$ and Medium 2 with $arepsilon_2, \mu_2, \sigma_2$), the field vectors must satisfy fundamental boundary conditions derived from Maxwell's integral equations. ``` Interface Geometry: Medium 1 (ε1, μ1) ──────────────────────────────── Interface (Surface charge σ_f, current K_f) Medium 2 (ε2, μ2) ``` ### 6.1 Derivation from Integral Equations 1. **Normal Component of Electric Displacement ($ec{D}$):** Applying Gauss's law over an infinitesimal pillbox cylinder spanning the interface: $$D_{1n} - D_{2n} = \sigma_f \iff arepsilon_1 E_{1n} - arepsilon_2 E_{2n} = \sigma_f$$ *Special Case:* At a boundary between two ideal dielectric media with zero free surface charge ($\sigma_f = 0$): $$D_{1n} = D_{2n} \implies arepsilon_1 E_{1n} = arepsilon_2 E_{2n}$$ 2. **Normal Component of Magnetic Flux Density ($ec{B}$):** Applying Gauss's law for magnetism ($\oiint ec{B} \cdot dec{S} = 0$) over a pillbox: $$B_{1n} = B_{2n} \implies \mu_1 H_{1n} = \mu_2 H_{2n}$$ *Consequence:* The normal component of $ec{B}$ is always strictly continuous across any interface. 3. **Tangential Component of Electric Field ($ec{E}$):** Applying Faraday's Law over an infinitesimal rectangular loop oriented perpendicular to the surface: $$E_{1t} = E_{2t}$$ *Consequence:* The tangential component of electric field is always continuous across any interface, regardless of surface charges or conductivity. 4. **Tangential Component of Magnetic Field Intensity ($ec{H}$):** Applying the Ampère-Maxwell law over an infinitesimal loop spanning the interface: $$\hat{n} imes (ec{H}_1 - ec{H}_2) = ec{K}_f \implies H_{1t} - H_{2t} = K_f$$ Where $ec{K}_f$ is the surface current density. For non-conducting media ($ec{K}_f = 0$): $$H_{1t} = H_{2t} \iff rac{B_{1t}}{\mu_1} = rac{B_{2t}}{\mu_2}$$ --- ## 7. Comparative Reference Table: Field Vector Characteristics | Vector Quantity | Symbol | SI Unit | Constitutive Formula | Free Space Constant | |---|---|---|---|---| | **Electric Field Intensity** | $ec{E}$ | $ ext{V/m}$ or $ ext{N/C}$ | $ec{F} = qec{E}$ | — | | **Electric Displacement** | $ec{D}$ | $ ext{C/m}^2$ | $ec{D} = arepsilon_0 ec{E} + ec{P}$ | $arepsilon_0 pprox 8.854 imes 10^{-12} ext{ F/m}$ | | **Magnetic Flux Density** | $ec{B}$ | $ ext{Tesla (T)}$ or $ ext{Wb/m}^2$ | $ec{F} = q(ec{v} imes ec{B})$ | $\mu_0 = 4\pi imes 10^{-7} ext{ H/m}$ | | **Magnetic Field Intensity** | $ec{H}$ | $ ext{A/m}$ | $ec{B} = \mu_0(ec{H} + ec{M})$ | — | | **Poynting Vector** | $ec{S}$ | $ ext{W/m}^2$ | $ec{S} = ec{E} imes ec{H}$ | $\eta_0 pprox 376.73\ \Omega$ | | **Electric Potential** | $V$ | $ ext{Volt (V)}$ | $ec{E} = - abla V$ | — | | **Magnetic Vector Potential** | $ec{A}$ | $ ext{Wb/m}$ or $ ext{T}\cdot ext{m}$ | $ec{B} = abla imes ec{A}$ | — |