User:John R. Brews/Sample: Difference between revisions
imported>John R. Brews |
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</ref> | </ref> | ||
:<math>\Phi(\boldsymbol r , \ t) | :<math>\Phi(\boldsymbol r , \ t) =\left. \frac{q}{(1-\mathbf{\hat u \cdot }\boldsymbol \beta )R}\right|_{\tilde t} \ , </math> | ||
where the tilde {{nowrap|‘ '''<sup>~</sup>''' ’}} denotes evaluation at the ''retarded time'' , | where the tilde {{nowrap|‘ '''<sup>~</sup>''' ’}} denotes evaluation at the ''retarded time'' , | ||
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The vector potential is: | The vector potential is: | ||
:<math>\boldsymbol A(\boldsymbol r , \ t) | :<math>\boldsymbol A(\boldsymbol r , \ t) =\left. \frac{q \boldsymbol \beta}{(1-\mathbf{\hat u \cdot }\boldsymbol \beta )R}\right|_{\tilde t} \ . </math> | ||
With these potentials the electric field and the magnetic flux density are found to be (dots over symbols are time derivatives):<ref name=Melia/> | With these potentials the electric field and the magnetic flux density are found to be (dots over symbols are time derivatives):<ref name=Melia/> |
Revision as of 16:19, 23 April 2011
Liénard–Wiechert potentials
Define β in terms of the velocity 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]
Notes
- ↑ 1.0 1.1 Fulvio Melia (2001). “§4.6.1 Point currents and Liénard-Wiechert potentials”, Electrodynamics. University of Chicago Press, pp. 101. ISBN 0226519570.
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