< User:John R. BrewsRevision as of 16:20, 23 April 2011 by imported>John R. Brews
Liénard–Wiechert potentials
Define β in terms of the velocity v of a point charge at time t as:

and unit vector û as

where R is the vector joining the observation point P to the moving charge q at the time of observation. Then the Liénard–Wiechert potentials consist of a scalar potential Φ and a vector potential A. The scalar potential is:[1]

where the tilde ‘ ~ ’ denotes evaluation at the retarded time ,

c being the speed of light, r the location of the observation point, and rO being the location of the particle on its trajectory.
The vector potential is:

With these potentials the electric field and the magnetic flux density are found to be (dots over symbols are time derivatives):[1]
![{\displaystyle {\boldsymbol {E}}({\boldsymbol {r}},\ t)=q\left[{\frac {(\mathbf {\hat {u}} -{\boldsymbol {\beta }})(1-\beta ^{2})}{(1-\mathbf {\hat {u}} \mathbf {\cdot } {\boldsymbol {\beta }})^{3}R^{2}}}+{\frac {\mathbf {{\hat {u}}\ \mathbf {\times } \ } [({\hat {\mathbf {u} }}-{\boldsymbol {\beta }})\ \mathbf {\times } \ {\boldsymbol {\dot {\beta }}}]}{c(1-\mathbf {{\hat {u}}\cdot } {\boldsymbol {\beta }})^{3}R}}\right]_{\tilde {t}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/e3f2d2bbbe117c7de23a92eb7703619906ff7a5e)

Notes
Feynman
Belušević
Gould
Schwartz
Schwartz
Oughstun
Eichler
Müller-Kirsten
Panat
Palit
Camara
Smith
classical distributed charge
Florian Scheck
Radiation reaction
Fulvio Melia
Radiative reaction Fulvio Melia
Barut Radiative reaction
Distributed charges: history
Lorentz-Dirac equation Gould
Fourier space description