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'Classical electromagnetism' (or 'classical electrodynamics') is a theory of electromagnetism that was developed over the course of the 19th century, most prominently by James Clerk Maxwell. It provides an excellent description of electromagnetic phenomena whenever the relevant length scales and field strengths are large enough that quantum mechanical effects are negligible (see quantum electrodynamics).
Mathematically it follows from applying the Lorentz transformation to the Coulomb force of a point electric charge to find the force between moving charges.

Contents

Lorentz force

The electric field E

Electromagnetic waves

General field equations

See also

Lorentz force

The electromagnetic field exerts the following force (often called the Lorentz force) on charged particles:
:$$
mathbf{F} = qmathbf{E} + qmathbf{v} imes mathbf{B}

where all boldfaced quantities are vectors: 'F' is the force that a charge q experiences, 'E' is the electric field at q's location, 'v' is q's velocity, 'B' is the strength of the magnetic field at q's position.
This description of the force between charged particles, unlike Coulomb's force law, does not break down under relativity and in fact, the magnetic force is seen as part of the relativistic interaction of fast-moving charges that Coulomb's law neglects.

The electric field E

The electric field 'E' is defined such that, on a stationary charge:
:$$
mathbf{F} = q_0 mathbf{E}

where q₀ is what is known as a test charge. The size of the charge doesn't really matter, as long as it is small enough as to not influence the electric field by its mere presence. What is plain from this definition, though, is that the unit of 'E' is N/C, or newtons per coulomb. This unit is equal to V/m (volts per meter), see below.
The above definition seems a little bit circular but, in electrostatics, where charges are not moving, Coulomb's law works fine. So what we end up with is:
:$$
mathbf{E} = sum_{i=1}^{n} rac{q_i left( mathbf{r} - mathbf{r}_i
ight)} {4 pi epsilon_0 left| mathbf{r} - mathbf{r}_i
ight|^3}

where n is the number of charges, q_i is the amount of charge associated with the 'i'th charge, 'r'_i is the position of the 'i'th charge, 'r' is the position where the electric field is being determined, and ε₀ is a universal constant called the permittivity of free space.
Note: the above is just Coulomb's law, divided by q₁, adding up multiple charges.
Changing the summation to an integral yields the following:
:$$
mathbf{E} = int rac{
ho mathbf{r}_{unit}}{ 4 pi epsilon_0 r^2} mathrm{d}V

where ρ is the charge density as a function of position, 'r'_unit is the unit vector pointing from dV to the point in space 'E' is being calculated at, and r is the distance from the point 'E' is being calculated at to the point charge.
Both of the above equations are cumbersome, especially if one wants to calculate 'E' as a function of position. There is, however, a scalar function called the electrical potential that can help. Electric potential, also called voltage (the units for which are the volt), which is defined thus:
:$$
phi_mathbf{E} = - int_s mathbf{E} cdot mathrm{d}mathbf{s}

where φ_'E' is the electric potential, and s is the path over which the integral is being taken.
Unfortunately, this definition has a caveat. From Maxwell's equations, it is clear that $$
abla imes mathbf{E} is not always zero, and hence the scalar potential alone is insufficient to define the electric field exactly. As a result, one must resort to adding a correction factor, which is generally done by subtracting the time derivative of the 'A' vector potential described below. Whenever the charges are quasistatic, however, this condition will be essentially met, so there will be few problems. (As a side note, by using the appropriate gauge transformations, one can define V to be zero and define E entirely as the negative time derivative of 'A', however, this is rarely done because a) it's a hassle and more important, b) it no longer satisfies the requirements of the Lorenz gauge and hence is no longer relativistically invariant).
From the definition of charge, it is trivial to show that the electric potential of a point charge as a function of position is:
:$$
phi = rac{q}{ 4 pi epsilon_0 left| mathbf{r} - mathbf{r}_q
ight|}

where q is the point charge's charge, 'r' is the position, and 'r'_q is the position of the point charge. The potential for a general distribution of charge ends up being:
:$$
phi = rac{1}{4 pi epsilon_0}
int rac{
ho}{r}, mathrm{d}V

where ρ is the charge density as a function of position, and r is the distance from the volume element $mathrm\{d\}V$.
Note well that φ is a scalar, which means that it will add to other potential fields as a scalar. This makes it relatively easy to break complex problems down in to simple parts and add their potentials. Taking the definition of φ backwards, we see that the electric field is just the negative gradient (the del operator) of the potential. Or:
:$$
mathbf{E} = -
abla phi

From this formula it is clear that 'E' can be expressed in V/m (volts per meter).

Electromagnetic waves

A changing electromagnetic field propagates away from its origin in the form of a wave. These waves travel in vacuum at the speed of light and exist in a wide spectrum of wavelengths. Examples of the dynamic fields of electromagnetic radiation (in order of increasing frequency): radio waves, microwaves, light (infrared, visible light and ultraviolet), x-rays and gamma rays. In the field of particle physics this electromagnetic radiation is the manifestation of the electromagnetic interaction between charged particles.

General field equations

As simple and satisfying as Coulomb's equation may be, it is not entirely correct in the context of classical electromagnetism. Problems arise because changes in charge distributions require a non-zero amount of time to be "felt" elsewhere (required by special relativity). Disturbances of the electric field due to a charge propagate at the speed of light.
For the fields of general charge distributions, the retarded potentials can be computed and differentiated accordingly to yield Jefimenko's Equations.
Retarded potentials can also be derived for point charges, and the equations are known as the Liénard-Wiechert potentials. The scalar potential is:
$$
phi = rac{1}{4 pi epsilon_0} rac{q}{left| mathbf{r} - mathbf{r}_q(t_{ret})
ight|-rac{mathbf{v}(t_{ret})}{c} cdot mathbf{r}_q(t_{ret})}

where $q$ is the point charge's charge and $mathbf\{r\}$ is the position. $mathbf\{r\}\_q$ and $mathbf\{v\}$ are the position and velocity of the charge, respectively, as a function of retarded time. The vector potential is similar:
$$
mathbf{A} = rac{mu_0}{4 pi} rac{qmathbf{v}(t_{ret})}{left| mathbf{r} - mathbf{r}_q(t_{ret})
ight|-rac{mathbf{v}(t_{ret})}{c} cdot mathbf{r}_q(t_{ret})}

These can then be differentiated accordingly to obtain the complete field equations for a moving point particle. Although the equations are aesthetically unpleasant, they bring a satisfying closure to classical electrodynamics.

See also

★ Quantum electrodynamics