Maxwell's Equations

Maxwell's Equations, formulated around 1861 by James Clerk Maxwell describe the interrelation between electric and magnetic fields.They were a synthesis of what was known about electricity and magnetism, particularly building on the work of Michael Faraday, Andre-Marie Ampere, and others. These equations predicted the existence of Electromagnetic waves, giving them properties that were recognized to be properties of light, leading to the (correct) realization that light is an electromagnetic wave. Other forms of electromagnetic waves, such as radio waves, were not known at the time, but were subsequently demonstrated by Heinrich Hertz in 1888. These equations are considered to be among the most elegant edifices of mathematical physics.

Maxwell's equations serve many purposes and take many forms. On the one hand, they are used in the solution of actual real-world problems of electromagnetic fields and radiation. On the other hand, they are the subject of admiration for their elegance. There are many T-shirts, typically obtainable on college campuses, sporting various forms of these equations.

What follows is a survey of the various forms that these equations take, beginning with the most utilitarian and progressing to the most elegant. Which form you prefer depends on your scientific outlook, and perhaps your taste in T-shirts. The various "<math>\nabla \cdot \mathbf{E}</math>" and "<math>\nabla \times \mathbf{E}</math>" symbols appearing in some of the equations are the divergence and curl operators, respectively.

Name	Partial Differential Equations	Integral Equations
Gauss's Law of Conservation:	<math>\nabla \cdot \mathbf{D} = \rho</math>	<math>\oint_S \mathbf{D} \cdot \mathrm{d}\mathbf{A} = \int_V \rho\, \mathrm{d}V</math>
Gauss' Law Of Magnetism:	<math>\nabla \cdot \mathbf{B} = 0</math>	<math>\oint_S \mathbf{B} \cdot \mathrm{d}\mathbf{A} = 0</math>
Faraday's Law of Induction:	<math>\nabla \times \mathbf{E} = -\frac{\partial \mathbf{B}} {\partial t}</math>	<math>\oint_C \mathbf{E} \cdot \mathrm{d}\mathbf{l} = - \int_S \frac{\partial\mathbf{B}}{\partial t} \cdot \mathrm{d} \mathbf{A}</math>
Ampère's Law of Circulation	<math>\nabla \times \mathbf{H} = \mathbf{J} + \frac{\partial \mathbf{D}} {\partial t}</math>	<math>\oint_C \mathbf{H} \cdot \mathrm{d}\mathbf{l} = \int_S \mathbf{J} \cdot \mathrm{d} \mathbf{A} + \int_S \frac{\partial\mathbf{D}}{\partial t} \cdot \mathrm{d} \mathbf{A}</math>

where B denotes the magnetic field, E denotes the electric field, H denotes the auxiliary magnetic field, J denotes the free current density, and <math>\rho</math> denotes the free electric charge density.

In the language of Exterior Calculus, Maxwell's equations can be rewritten much more compactly as:

<math>\mathrm{d}\bold{F}=0</math>

<math>\mathrm{d} * {\bold{F}}=\bold{J}</math>

where d is exterior derivative operator, * is the Hodge star operator, and F is the Faraday tensor.