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# Maxwell's equations

Maxwell's equations are the set of four equations by James Clerk Maxwell that describe the behavior of both the electric and magnetic fields.

 Table of contents 1 Introduction 2 Summary 3 Detail 4 A Final Note on Unit Systems 5 Formulation of Maxwell's equations in special relativity 6 Maxwell's equations in terms of differential forms 7 References 8 External links

## Introduction

Maxwell's equations provided the basis for the unification of electric field and magnetic field, the electromagnetic description of light, and ultimately, Theodor Kaluza's unification (Kaluza-Klein theory) of electromagnetism with Albert Einstein's theory of relativity.

The modern mathematical formulation of Maxwell's equations is due to Oliver Heaviside and Willard Gibbs, who in 1884 reformulated Maxwell's original equations using vector calculus. (Maxwell's 1865 formulation was in terms of 20 equations in 20 variables, although he later attempted a quaternion formulation that proved awkward.) The change to the vector notation produced a symmetric mathematical representation that reinforced the perception of physical symmetries between the various fields.

In the late 19th century, because of the appearance of a velocity () in the equations, Maxwell's equations were only thought to express electromagnetism in the rest frame of the Luminiferous aether (the postulated medium for light, whose interpretation was considerably debated). When the Michelson-Morley experiment conducted by Edward Morley and Albert Abraham Michelson produced a null result for the change of the velocity of light due to the Earth's hypothesized motion through the aether, however, alternative explanations were sought by Lorentz and others. This culminated in Einstein's theory of special relativity, which postulated the absence of any absolute rest frame (or aether) and the invariance of Maxwell's equations in all frames of reference.

The electromagnetic field equations have an intimate link with special relativity: the magnetic field equations can be derived from consideration of the transformation of the electric field equations under relativistic transformations at low velocities. (In relativity, the equations are written in an even more compact, "manifestly covariant" form, in terms of the rank-2 antisymmetric field-strength 4-tensor.)

Kaluza and Klein showed in the 1920's that the Maxwell's equations can be derived by extending general relativity into five dimensions. This strategy of using higher dimensions to unify different forces is an active area of research in particle physics.

## Summary

### General Case

Note that the second equation is equivalent to the statement that magnetic monopoles do not exist.

### In Linear Media/Material

In linear media, the macroscopic field strengths D and H are related to the bare field strengths E and B by

In linear and isotropic media, ε and μ are constants, and Maxwell's equations reduce to

### In a Vacuum

The vacuum is such a medium, and the proportionality constants in the vacuum are denoted by ε0 and μ0. If there is no current or electric charge present in the vacuum, we obtain the Maxwell equation's in free space:

This equation has a simple solution in terms of travelling sinusoidal plane waves, with the elecric and magnetic field directions orthogonal to one another and the direction of travel, and with the two fields 90° out of phase, travelling at the speed

Maxwell discovered that this quantity c is simply the
speed of light in vacuum, and thus that light is a form of electromagnetic radiation.

## Detail

### Charge Density and the Electric Field

,

where is the free electric charge density (in units of C/m3), not including dipole charges bound in a material, and is the electric displacement field (in units of C/m2). This equation corresponds to Coulomb's law for stationary charges in vacuum.

The equivalent integral form (by the divergence theorem), also known as Gauss's Law, is:

where is the area of a differential square on the closed surface A with an outward facing surface normal defining its direction, and is the free charge enclosed by the surface.

In a linear material , is directly related to the electric field via a material-dependent constant called the permittivity, :

.

Any material can be treated as linear, as long as the electric field is not extremely strong. The permittivity of free space is referred to as , and appears in:

where, again, is the electric field (in units of V/m), is the total charge density (including bound charges), and (approximately 8.854 pFarads/m) is the permittivity of free space. can also be written as , where is the material's relative permittivity or its dielectric constant.

### The Structure of the Magnetic Field

```is the magnetic flux density (in units of tesla, T), also called the magnetic induction.
```
Equivalent integral form:

```is the area of a differential square on the surface  with an outward facing surface normal defining its direction.
```
Note: like the electric field's integral form, this equation only works if the integral is done over a closed surface.

### A Changing Magnetic Field and the Electric Field

Equivalent Integral Form:

where

ΦB is the magnetic flux through the area A described by the second equation, ε is the
electromotive force around the edge of the surface A.

Note: this equation only works of the surface A is not closed because the net magnetic flux through a closed surface will always be zero, as stated by the previous equation. That, and the electromotive force is measured along the edge of the surface; a closed surface has no edge. Some textbooks list the Integral form with an N (representing the number of coils of wire that are around the edge of A) in front of the flux derivative. The N can be taken care of in calculating A (multiple wire coils means multiple surfaces for the flux to go through), and it is an engineering detail so it has been omitted here.

Note the negative sign; it is necessary to maintain conservation of energy. It is so important that it even has its own name, Lenz's law.

This equation relates the electric and magnetic fields, but it also has a lot of practical applications, too. This equation describes how electric motors and electric generators work.

This law corresponds to the Faraday's law of electromagnetic induction.

Note: Maxwell's equations apply to a right-handed coordinate system. To apply them unmodified to a left handed system would mean a reversal of polarity of magnetic fields (not inconsistent, but confusingly against convention).

### The Source of the Magnetic Field

where H is the magnetic field strength (in units of A/m), related to the magnetic flux B by a constant called the permeability, μ (B = μH), and J is the current density, defined by: J = ∫ρqvdV where v is a vector field called the drift velocity that describes the velocities of that charge carriers which have a density described by the scalar function ρq.

In free space, the permeability μ is the permeability of free space, μ0, which is defined to be exactly 4π×10-7 W/Am. Thus, in free space, the equation becomes:

Equivalent integral form:

s is the edge of the open surface A (any surface with the curve s as its edge will do), and Iencircled is the current encircled by the curve s (the current through any surface is defined by the equation: Ithrough A = ∫AJ·dA).

Note: unless there is a capacitor or some other place where , the second term on the right hand side is generally negligable and ignored. Any time this applies, the integral form is known as Ampere's Law.

## A Final Note on Unit Systems

The above equations are all in a unit system called mks (short for meter, kilogram, second; also know as the International System of Units (or SI for short). This is more commonly known as the metric system. In a related unit system, called cgs (short for centimeter, gram, second), the equations take on a more symmetrical form, as follows:

Where c is the speed of light in a vacuum. The symmetry is more apparent when the electromagnetic field is considered in a vacuum. The equations take on the following, highly symmetric form:

Note: All variables that are in bold represent vector quantities; see also vector calculus.

## Formulation of Maxwell's equations in special relativity

to do: 4-vectors, and the d'Alembertian operator

## Maxwell's equations in terms of differential forms

In a vacuum, where ε and μ are constant everywhere, Maxwell's equations simplify considerably once you use the language of differential geometry and differential forms. Now, the electric and magnetic fields are jointly described by a 2-form in a 4-dimensional spacetime manifold which is usually called F. Maxwell's equations then reduce to the Bianchi identity

where d is the exterior derivative, and the source equation
where these are represented in natural units where ε0 is 1. Here, J is a 1-form called the "electric current" satisfying the continuity equation

See gauge theory for more details.