Maxwell Equations

From TorontoMathWiki

Jump to: navigation, search

Contents

Differential Form

Maxwell's equations are,

\ \nabla \cdot \vec{D} = \rho

\ \nabla \cdot \vec{B} = 0

\ \nabla \times \vec{E} = \frac{- \partial \vec{B}}{\partial t}

\ \nabla \times \vec{H} = \frac{\partial \vec{D}}{\partial t} + \vec{J}.

Where the vectors are defined in the usual way. Also,

\ \vec{D} = \epsilon_0 \vec{E} + \vec{P} and,

\ \vec{B} = \mu_0 \vec{H} + \vec{M}.

Taking a Fourier transform with respect to the time variable, we have,


\ \nabla \cdot \vec{\hat{D}} = \rho

\ \nabla \cdot \vec{\hat{B}} = 0

\ \nabla \times \vec{\hat{E}} = -\dot{\imath} \omega \vec{\hat{B}}

\ \nabla \times \vec{\hat{H}} = \dot{\imath} \omega \vec{\hat{D}} + \vec{\hat{J}}.

See ``Electromagnetics" for more.

Integral Form

The integral form is also commonly given.

\ \oint \nabla \cdot \vec{D} dV = \oint \vec{D} \cdot d\vec{S} = Q_{enclosed}

\ \oint \nabla \cdot \vec{B} dV = \oint \vec{B} \cdot d\vec{S} = 0

\ \int \nabla \times \vec{E} \cdot d\vec{S} = \oint \vec{E} \cdot d\vec{l} =  \frac{- \partial }{\partial t} \int \vec{B}\cdot d\vec{S}

 \int \nabla \times \vec{H} \cdot d\vec{S}= \oint \vec{H} \cdot d\vec{l} =  \frac{\partial }{\partial t}\int \vec{D} \cdot \vec{S} + I

Energy of the Field

Power Flow into a Volume

The Poynting vector gives the direction of power flow. The Poynting vector is given by,

\ \vec{\mathcal{S}} = \vec{E} \times \vec{H} .

It has the units, watts per square meter.

The power flow through a differential area id given by \ -\vec{\mathcal{S}}\cdot d\vec{S} . The power flow through a volume is then given by summing up the power flow through the area enclosing that volume, thus:

\ P = -\oint \vec{\mathcal{S}} \cdot d\vec{S} = -\int \nabla \cdot \vec{\mathcal{S}} dV .

Expanding by Maxwell's equations,

\ P = -\int \nabla \cdot \vec{E} \times \vec{H} dV

\ = -\int \vec{H} \cdot (\nabla \cdot \vec{E}) - \vec{E} \cdot (\nabla \cdot \vec{H}) dV

\ = -\int \vec{H} \cdot \left(-\frac{\partial}{\partial t} (\mu_0 \vec{H} + \vec{M})\right) - \vec{E} \cdot \left(\frac{\partial}{\partial t} (\epsilon_0 \vec{E} + \vec{P}) + \vec{J}\right) dV

\ = \int \vec{H} \cdot \left(\frac{\partial \mu_0 \vec{H}}{\partial t} + \frac{\partial \vec{M}}{\partial t} \right) + \vec{E} \cdot \left(\frac{\partial\epsilon_0 \vec{E}}{\partial t}  + \frac{\partial \vec{P}}{\partial t}\right) + \vec{E} \cdot \vec{J} dV

\ = \int \frac{1}{2}\left(\mu_0 \frac{\partial  |\vec{H}|^2}{\partial t} + \epsilon_0  \frac{\partial\ |\vec{E}|^2}{\partial t}\right) + \vec{H} \cdot \frac{\partial \vec{M}}{\partial t} + \vec{E} \cdot \frac{\partial \vec{P}}{\partial t} + \vec{E} \cdot \vec{J} dV .

The first summand is the power density of the vacuum electromagnetic field; the second and third summands, when integrated, are the power dissipation by magnetic and electric dipoles; the fourth summand, when integrated is power dissipation by current.


Reference: ECE525 Lasers and Detectors. notes taken in class, 2010. Instructor: Joyce Poon.

Personal tools