Electromagnetic theory
1. Basic Laws of Electromagnetic Theory
电荷在电场、磁场中受力 \[\vec{F} = q \left( \vec{E} + \vec{v}\times \vec{B} \right)\]
- Maxwell Equations
- \begin{cases} &\nabla\cdot \vec{E} = \dfrac{\rho}{\varepsilon_0}\\ &\nabla\cdot \vec{B} = 0\\ &\nabla\times \vec{E} = - \dfrac{\partial \vec{B}}{\partial t}\\ &\nabla\times \vec{B} = \mu_0 \vec{\jmath} + \mu_0\epsilon_0 \dfrac{\partial \vec{E}}{\partial t}\\ \end{cases}
- Constitutive equation (本构方程)
- \begin{cases} &\vec{D} = \varepsilon_0 \vec{E} + \vec{P} = \varepsilon_0\varepsilon_r \vec{E}\\ &\vec{B} = \mu_0 \left( \vec{H} + \vec{M} \right) = \mu_0\mu_r \vec{H}\\ &\vec{P} = \varepsilon_0\chi_e \vec{E};\;\vec{M} = \chi_m \vec{H};\;\vec{J}_f = \sigma \vec{E} \end{cases}
2. Electromagnetic wave
假设介质均匀, 且无源电荷源电流 \(\vec{J} = \mathbf{0}\), 此时
\begin{cases} &\nabla\cdot \vec{E} = 0\\ &\nabla\cdot \vec{B} = 0\\ &\nabla\times \vec{E} = - \dfrac{\partial \vec{B}}{\partial t}\\ &\nabla\times \vec{B} = \mu_0 \varepsilon_0\mu_r\varepsilon_r \frac{\partial \vec{E}}{\partial t}\\ \end{cases}由矢量分析可知: \[\nabla\times \left( \nabla\times \vec{E} \right) = \nabla \left( \nabla\cdot \vec{E} \right) - \nabla^2 \vec{E} = - \nabla^2 \vec{E}\] \[\nabla\times \left( - \frac{\partial \vec{B}}{\partial t} \right) = \frac{\partial}{\partial t} \left( \nabla\times \vec{B} \right) =- \mu_0\varepsilon_0\mu_r\varepsilon_r \frac{\partial^2 \vec{E}}{\partial t^2}\] 故有:\[\nabla^2 \vec{E} = \mu_0\varepsilon_0\mu_r\varepsilon_r \frac{\partial^2\vec{E}}{\partial t^2}\] \[\nabla^2\vec{B} = \mu_0\varepsilon_0\mu_r\varepsilon_r \frac{\partial^2\vec{B}}{\partial t^2}\] \[v = \frac{1}{\sqrt{\mu_0\varepsilon_0\mu_r\varepsilon_r}} = \frac{c}{\sqrt{\mu_r\varepsilon_r}} = \frac{c}{n}\] 其中 \(n = \sqrt{\mu_r\varepsilon_r}\), 为材料折射率.
2.1. 平面波解
设平面光波沿着 \(x\) 方向传播, \(\vec{E}\) 不依赖 \(y, z\) \[\nabla\cdot \vec{E} = 0\Rightarrow \frac{\partial E_x}{\partial x} = 0\] 故
- 电场只有 \(y, z\) 分量, 振动方向垂直于传播方向 (横波)
- 电场振动方向可以用两个正交的分量叠加-两个线偏振光组合.
设电场为沿 y 方向振动的线偏振光 \(\vec{E} = \hat{\jmath}E_y(x, t)\) \[\nabla\times \vec{E} = -\frac{\partial \vec{B}}{\partial t} \Rightarrow \frac{\partial E_y}{\partial x} = -\frac{\partial B_z}{\partial t}, \;\frac{\partial B_x}{\partial t} = \frac{\partial B_y}{\partial t} = 0\] \[\Rightarrow \vec{B} = \frac{1}{\omega}\vec{k}\times \vec{E} \Rightarrow E_y = vB_z\] 在 均匀、线性、各向同性 的电介质传播的电磁波是电场与磁场传播方向互为正交的横波.
注意: 平面波并非麦克斯韦方程的唯一解.
3. Energy and Momentum
\[u_E = \frac{\varepsilon_0}{2}E^2,\;u_B = \frac{1}{2\mu_0}B^2\] \[E = cB, c = \frac{1}{\sqrt{\varepsilon_0\mu_0}}\Rightarrow u_E = u_B\] \[\therefore u = u_E + u_B = \varepsilon_0 E^2 = \frac{1}{\mu_0}B^2\]
- 能流密度
- 波携带能量传播,单位时间流过单位面积的功率. \[S = uc = \frac{1}{\mu_0}EB = EH\]
- 波印廷矢量
- 考虑到能量传播的方向,定义 Poynting Vector: \[\vec{S} = \vec{E}\times \vec{H} = \frac{1}{\mu_0}\vec{E}\times \vec{B} = c^2\varepsilon_0 \vec{E}\times \vec{B}\]
- 平均能流密度
- 若电磁波为简谐波,平均能流密度: \[\left\langle S \right\rangle_T = \frac{c^2\varepsilon_0}{2}\left| \vec{E}_0\times \vec{B}_0 \right|\]
4. Light in Bulk Matter
- 折射率
- 光在介质中的传播依赖折射率: \(v = \frac{c}{n}\) \[n = \sqrt{\mu_r\varepsilon_r}\] 折射率源自 Constitutive equation: (忽略磁场极化, \(\mu_r\approx 0\)) \[\therefore \varepsilon_r = n^2 = 1 +\chi,\; \vec{P} = \varepsilon_0\chi \vec{E}\]
4.1. Simple harmonic oscillation 简谐振动
任何稳定平衡点附近的振动可以近似为简谐振动.
4.1.1. Forced vibratiom 受迫振动
- 策动力: \(f(t) = F\cos\omega t\)
- 稳态解: \(x = A\cos \left( \omega t+\varphi_0 \right)\)
4.2. Origin of refractive index
分子或介质置于外电场中, 发生极化, 诱导出偶极 \(q \vec{x}\), 方向为 \(-q\) 指向 \(+q\).
在光场(高频交变电磁场)驱动下, 分子中偏移电荷在平衡位置附近做受迫运动:(忽略磁场力) \[m \frac{\mathrm{d}^2x}{\mathrm{d}t^2} + m\omega_0^2 x = qE_0\cos(\omega t)\] \[\Rightarrow x(t) = \frac{q/m}{\left(\omega_0^2 - \omega^2\right)^2} E_0\cos(\omega t) = \frac{q/m}{\left(\omega 0^2 - \omega^2\right)^2} E(t)\] 设单位体积中有 \(N\) 个光电场诱导的偶极子,则电极化强度为: \[P = qxN = \frac{q^2NE/m}{\left(\omega 0^2 - \omega^2\right)^2} = \varepsilon_0\chi E\] \[\Rightarrow\chi = \frac{q^2N/m}{\left(\omega 0^2 - \omega^2\right)^2\varepsilon_0}\] \[\therefore n^2(\omega) = 1 + \frac{Nq^2}{\varepsilon_0m} \left( \frac{1}{\omega_0^2 - \omega^2} \right)\]
4.3. Cauchy relation
当光频率 \(\omega \ll \omega_0\), 折射率可近似表示为:
\begin{aligned} n^2(\omega) &= 1+ \frac{Nq^2}{\varepsilon_0m\omega_0^2} \left( 1+ \frac{\omega^2}{\omega_0^2} \right)\\ &= 1 + \frac{Nq^2}{\varepsilon_0m\omega_0^2} + \frac{Nq^24\pi^2c^2}{\varepsilon_0m\omega_0^4} \frac{1}{\lambda^2} \end{aligned}\[\therefore \left( n^2 - 1 \right)^{-1} = -C\lambda^{-2} + C\lambda_0^{-2}\]
- \(\lambda_0 = \frac{2\pi c}{\omega_0}\)
- \(C = \frac{4\pi^2c^2\varepsilon_0 m}{Nq^2}\)
- \(\lambda_0^2\ll\lambda^2\) 时上式成立.
如果分子有很多个简谐模式, 易得: (\(f_j\) 为跃迁几率) \[n^2(\omega) = 1+ \frac{Nq^2}{\varepsilon_0 m}\sum_j \frac{f_j}{\omega_{0j}^2 - \omega^2}\] 因为忽略阻尼, \(\omega\rightarrow\omega_0\), \(n\) 发散, 故引入阻尼, 得到复吸收率: \[n^2(\omega) = 1 + \frac{Nq^2}{\varepsilon_0 m} \sum_j \frac{f_j}{\omega_{0j}^2 - \omega^2 + \mathrm{i}\gamma_j\omega}\] \[n = \eta + \mathrm{i}\kappa \Rightarrow k = \frac{\omega}{v} = \frac{\omega}{c/n} = (\eta + \mathrm{i}\kappa)\frac{\omega}{c}\]
\begin{aligned} E &= E_0 \mathrm{e}^{\mathrm{i}(kz-\omega t)}\\ &= E_0\exp \left[ \mathrm{i}(\eta+\mathrm{i}\kappa)\frac{\omega}{c}z -\omega t \right]\\ &= E_0\exp \left[ \underbrace{-\mathrm{i}\omega \left( t-\frac{\eta z}{c} \right)}_{\text{transmission phase}} \;\underbrace{-\frac{\kappa\omega}{c}z}_{\text{damping}} \right] \end{aligned}transmission phase 为传输相位, damping 为衰减项.
4.4. Optical response of metal
\[n^2(\omega) = 1 - \frac{Nq^2}{\varepsilon_0m\omega^2} = 1 - \frac{\omega_p^2}{\omega^2}, \;\omega_p = q \sqrt{\frac{N}{\varepsilon_0 m}}\]
- \(\omega > \omega_p\) 折射率为小于 1 的实数, 透明
- \(\omega < \omega_p\) 折射率为虚数, 强吸收(强反射).
4.5. Correction on refractive index
Internal field (Lorentz local field) is different form the applied field due to polarization of the dielectric. \[E_{\text{tot}} = E + E_{\text{int}} = E + \frac{1}{3\varepsilon_0}P\] 可得
- Clausis-Mossotti relation
- \[\frac{n^2 - 1}{n^2 + 2} \frac{Nq_e^2}{\varepsilon_0 m_e} \sum_j \frac{f_j}{\omega_{0j}^2 - \omega^2 + \mathrm{i}\gamma_j\omega}\]
4.6. Kinds of dispersion
- Normal dispersion: \(n\) increases with frequency.
- Anomalous dispersion: \(n\) decreases with frequency.
5. Photon 光子
Electromanetic field itself is qunatized: \[\epsilon = h\nu\]
5.1. Radiation pressure and momentum
The radiation pressure equals the energy density of the electromagnetic wave. \[P = u = \frac{\varepsilon_0}{2}E^2 + \frac{1}{2\mu_0}B^2 = \frac{S(t)}{c}\] totally absorbed.
- Average radiation pressure
\[\left\langle P(t) \right\rangle = \frac{S(t)}{c} = \frac{I}{c}\]
5.2. 电磁动量体密度
电磁波的动量 \[p_V = \frac{u}{c} = \frac{S}{c^2}\]
5.3. 每个光子动量
\[p = \frac{\epsilon}{c} = \frac{h}{\lambda}\Rightarrow \vec{p} = \hbar \vec{k}\] 其中约化普朗克常量 \(\hbar = \frac{h}{2\pi}\)