Retarded potential

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In electromagnetism, the retarded potentials are the electromagnetic potentials for the electromagnetic field generated by time-varying electric current or charge distributions in the past. The fields propagate at the speed of light c, so the delay of the fields connecting cause and effect at earlier and later times is an important factor: the signal takes a finite time to propagate from a point in the charge or current distribution (the point of cause) to another point in space (where the effect is measured), see figure below.^[1]

Contents

1 Potentials in the Lorenz gauge
- 1.1 Retarded and advanced potentials for time-dependent fields
- 1.2 Comparison with static potentials for time-independent fields
2 Potentials in the coulomb gauge
3 Occurance and application
4 References

Potentials in the Lorenz gauge

Main articles: Maxwell's equations and Mathematical descriptions of the electromagnetic field

Figure of source distribution.

The starting point is Maxwell's equations in the potential formulation using the Lorenz gauge:

$\Box \varphi = - \dfrac{\rho}{\epsilon_0} \,,\quad \Box \mathbf{A} = -\mu_0\mathbf{J}$

where φ(r, t) is the electric potential and A(r, t) is the magnetic potential, for an arbitrary source of charge density ρ(r, t) and current density J(r, t), and $\Box$ is the D'Alembert operator. Solving these gives the retarded potentials below.

Retarded and advanced potentials for time-dependent fields

For time-dependent fields, the retarded potentials are:^[2]^[3]

$\mathrm\varphi (\mathbf r , t) = \frac{1}{4\pi\epsilon_0}\int \frac{\rho (\mathbf r' , t_r)}{|\mathbf r - \mathbf r'|}\, \mathrm{d}^3\mathbf r'$

$\mathbf A (\mathbf r , t) = \frac{\mu_0}{4\pi}\int \frac{\mathbf J (\mathbf r' , t_r)}{|\mathbf r - \mathbf r'|}\, \mathrm{d}^3\mathbf r'\,.$

where r is a point in space, t is time,

$t_r = t-\frac{|\mathbf r - \mathbf r'|}{c}$

is the retarded time, and d³r' is the integration measure using r'.

From φ(r,t) and A(r, t), the fields E(r, t) and B(r, t) can be calculated using the definitions of the potentials:

$-\mathbf{E} = \nabla\varphi +\frac{\partial\mathbf{A}}{\partial t}\,,\quad \mathbf{B}=\nabla\times\mathbf A\,.$

and this leads to Jefimenko's equations. The corresponding advanced potentials have an identical form, except the advanced time

$t_a = t+\frac{|\mathbf r - \mathbf r'|}{c}$

replaces the retarded time.

Comparison with static potentials for time-independent fields

In the case the fields are time-independent (electrostatic and magnetostatic fields), the time derivatives in the $\Box$ operators of the fields are zero, and Maxwell's equations reduce to

$\nabla^2 \varphi =-\dfrac{\rho}{\epsilon_0}\,,\quad \nabla^2 \mathbf{A} =- \mu_0 \mathbf{J}\,,$

where ∇² is the Laplacian, which take the form of Poisson's equation in four components (one for φ and three for A), and the solutions are:

$\mathrm\varphi (\mathbf{r}) = \frac{1}{4\pi\epsilon_0}\int \frac{\rho (\mathbf r' )}{|\mathbf r - \mathbf r'|}\, \mathrm{d}^3\mathbf r'$

$\mathbf A (\mathbf r , t) = \frac{\mu_0}{4\pi}\int \frac{\mathbf J (\mathbf r' )}{|\mathbf r - \mathbf r'|}\, \mathrm{d}^3\mathbf r'\,.$

These also follow directly from the retarded potentials.

Potentials in the coulomb gauge

In the coulomb gauge, Maxwell's equations are^[4]

$\nabla^2 \varphi =-\dfrac{\rho}{\epsilon_0}$

$\nabla^2 \mathbf{A} - \dfrac{1}{c^2}\dfrac{\partial^2 \mathbf{A}}{\partial t^2}=- \mu_0 \mathbf{J} +\dfrac{1}{c^2}\nabla\left(\dfrac{\partial \varphi}{\partial t}\right)\,,$

although the solutions contrast the above, since A is a retarded potential yet φ changes instantly, given by:

$\varphi(\mathbf{r}, t) = \dfrac{1}{4\pi\epsilon_0}\int \dfrac{\rho(\mathbf{r})}{|\mathbf r - \mathbf r'|}\mathrm{d}^3\mathbf{r}'$

$\mathbf{A}(\mathbf{r},t) = \dfrac{1}{4\pi \varepsilon_0} \nabla\times\int \mathrm{d}^3\mathbf{r'} \int_0^{|\mathbf{r}-\mathbf{r}'|/c} \mathrm{d}t_r \dfrac{ t_r \mathbf{J}(\mathbf{r'}, t-t_r)}{|\mathbf{r}-\mathbf{r}'|^3}\times (\mathbf{r}-\mathbf{r}') \,.$

This is presents an advantage and a disadvantage of the coulomb gauge - φ is easy to calculate but A is not. While this appears to contradict special relativity in that the speed of light is the fastest speed of information transmission, the retardation of the A potential prevents E and B changing instantly, which can be measured by an observer (the potentials cannot be measured because infinitely many values of φ and A are simultaneously possible, due to the gauge freedom by their definition).

Occurance and application

A many-body theory which includes an average of retarded and advanced Liénard-Wiechert potentials is the Wheeler-Feynman absorber theory also known as the Wheeler-Feynman time-symmetric theory.

References

^ McGraw Hill Encyclopaedia of Physics (2nd Edition), C.B. Parker, 1994, ISBN 0-07-051400-3
^ Electromagnetism (2nd Edition), I.S. Grant, W.R. Phillips, Manchester Physics, John Wiley & Sons, 2008, ISBN 9-780471-927129
^ Introduction to Electrodynamics (3rd Edition), D.J. Griffiths, Pearson Education, Dorling Kindersley, 2007, ISBN 81-7758-293-3
^ Introduction to Electrodynamics (3rd Edition), D.J. Griffiths, Pearson Education, Dorling Kindersley, 2007, ISBN 81-7758-293-3

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