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# Maxwell's equations

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Maxwell's equations are the set of four equations, attributed to James Clerk Maxwell, that describe the behavior of both the electric and magnetic fields, as well as their interactions with matter.

 Table of contents 1 Introduction 2 Historical developments of Maxwell's equations and relativity 3 Summary of the Equations 4 Detail 5 Maxwell's Equations in CGS units 6 Formulation of Maxwell's equations in special relativity 7 Maxwell's equations in terms of differential forms 8 See also 9 References

## Introduction

Maxwell's four equations express, respectively, how electric charges produce electric fields (Gauss's law), the experimental absence of magnetic chargess, how currentss produce magnetic fields (Ampere's law), and how changing magnetic fields produce electric fields (Faraday's law of induction). Maxwell, in 1864, was the first to put all four equations together and to notice that a correction was required to Ampere's law: changing electric fields act like currents, likewise producing magnetic fields.

Furthermore, Maxwell showed that the four equations, with his correction, predict wavess of oscillating electric and magnetic fields that travel through empty space at a speed that could be predicted from simple electrical experiments—using the data available at the time, Maxwell obtained a velocity of 310,740,000 m/s. Maxwell (1865) wrote:

This velocity is so nearly that of light, that it seems we have strong reason to conclude that light itself (including radiant heat, and other radiations if any) is an electromagnetic disturbance in the form of waves propagated through the electromagnetic field according to electromagnetic laws.

Maxwell was correct, and his quantitative explanation of light as an electromagnetic wave is considered one of the great triumphs of 19th-century physics. (Actually, Michael Faraday had postulated a similar picture of light in 1846, but had not been able to give a quantitative description or predict the velocity.) Moreover, it laid the foundation for many future developments in physics, such as special relativity and its unification of electric and magnetic fields as a single tensor quantity, and Kaluza and Klein's unification of electromagnetism with gravity and general relativity.

## Historical developments of Maxwell's equations and relativity

The modern mathematical formulation of Maxwell's equations is due to Oliver Heaviside and Willard Gibbs, who in 1884 reformulated Maxwell's original system of equations to a far simpler representation using vector calculus. (Maxwell's 1865 formulation was in terms of 20 equations in 20 variables, although in 1873 he attempted a quaternion formulation that ultimately proved unpopular.) The change to the vector notation produced a symmetric mathematical representation that reinforced the perception of physical symmetries between the various fields. This highly symmetric formulation would directly inspire later developments in fundamental physics.

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 that unifies the electric and magnetic fields into a single object.)

Kaluza and Klein showed in the 1920s that 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 of the Equations

### General Case (SI units)

 Name Partial Differential form Gauss's law: Gauss's law for magnetism: Faraday's law of induction: Ampere's law + Maxwell's extension:

where:

ρ is the free electric charge density (in units of C/m3), not including dipole charges bound in a material

B is the magnetic flux density (in units of tesla, T), also called the magnetic induction.

D is the electric displacement field (in units of C/m2).

E is the electric field (in units of V/m),

H is the magnetic field strength (in units of A/m)

J is the current density

∇× is the curl operator

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

It is important to note that Maxwell's equations are generally applied to macroscopic averages of the fields, which vary wildly on a microscopic scale in the vicinity of individual atoms (where they undergo quantum mechanical effects as well).  It is only in this averaged sense that one can define quantities such as the permittivity and permeability of a material, below.  (The microscopic Maxwell's equations, ignoring quantum effects, are simply those of vacuum — but one must include all atomic charges and so on, which is normally an intractable problem.)

### In Linear Materials

In linear materials, the D and H fields are related to E and B by:

where:

μ is the magnetic permeability

(This can actually be extended to handle nonlinear materials as well, by making ε and μ depend upon the field strength; see e.g. the Kerr and Pockels effects.)

In non-dispersive, isotropic media, ε and μ are time-independent scalars, and Maxwell's equations reduce to

In a uniform (homogeneous) medium, ε and μ are constants independent of position, and can thus be furthermore interchanged with the spatial derivatives.

More generally, ε and μ can be rank-2 tensors (3×3 matrices) describing birefringent (anisotropic) materials. Also, although for many purposes the time/frequency-dependence of these constants can be neglected, every real material exhibits some material dispersion by which ε and/or μ depend upon frequency (and causality constrains this dependence to obey the Kramers-Kronig relations).

### In Vacuum, Without Charges or Currents

The vacuum is a linear, isotropic, dispersionless medium, and the proportionality constants in the vacuum are denoted by ε0 and μ0 (neglecting very slight nonlinearities due to quantum effects). If there is no current or electric charge present in the vacuum, we obtain the Maxwell's equations in free space:

These equations have a simple solution in terms of travelling sinusoidal plane waves, with the electric and magnetic field directions orthogonal to one another and the direction of travel, and with the two fields in 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.

Compare Poisson's equation.

### 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 is only useful if 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. Furthermore, 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 negligible and ignored. Any time this applies, the integral form is known as Ampère's Law.

## Maxwell's Equations in CGS units

The above equations are given in the International System of Units, or SI for short. In a related unit system, called cgs (short for centimetre, 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.

## Formulation of Maxwell's equations in special relativity

In special relativity, in order to more clearly express the fact that Maxwell's equations (in vacuum) take the same form in any inertial coordinate system, the vacuum Maxwell's equations are written in terms of four-vectors and tensors in the "manifestly covariant" form:

,

and

where J is the 4-current density, F is the field strength
tensor (written as a 4 × 4 matrix), and is the 4-gradient (so that is the d'Alembertian operator). (The α in the first equation is implicitly summed over, according to Einstein notation.) The first tensor equation expresses the two inhomogenous Maxwell's equations: Gauss' law and Ampere's law with Maxwell's correction. The second equation expresses the other two, homogenous equations: Faraday's law of induction and the absence of magnetic monopoles.

More explicitly, J = (cρ, J), in terms of the charge density ρ and the current density J. In terms of the 4-potential A = (φ, A), where φ is the electric potential and A is the magnetic vector potential in the Lorentz gauge (), F can be expressed as:

which leads to the 4 × 4 matrix (rank-2 tensor):

The fact that both electric and magnetic fields are combined into a single tensor expresses the fact that, according to relativity, both of these are different aspects of the same thing—by changing frames of reference, what seemed to be an electric field in one frame can appear as a magnetic field in another frame, and vice versa.

Note that different authors sometimes employ different sign conventions for the above tensors and 4-vectors (which does not affect the physical interpretation). Note also that Fαβ and Fαβ are not the same...they are the contravariant and covariant forms of the tensor, related by the metric tensor g so that they have opposite signs in some of their components.

## 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