## Classical electrodynamics |

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Page 472

For relativistic motion the

14.14) the radial component of Poynting's vector can be calculated to be [S - n]re

...

For relativistic motion the

**acceleration**fields depend on the velocity as well as the**acceleration**. Consequently the angular distribution is more complicated. From (14.14) the radial component of Poynting's vector can be calculated to be [S - n]re

...

Page 475

The total power radiated can be found by integrating (14.44) over all angles or

from (14.26): P(f') = -!£-/ (14.46) It is instructive to compare the power radiated for

...

The total power radiated can be found by integrating (14.44) over all angles or

from (14.26): P(f') = -!£-/ (14.46) It is instructive to compare the power radiated for

**acceleration**parallel to the velocity (14.43) or (14.27) with the power radiated for...

Page 506

The sudden creation of a fast electron in nuclear beta decay, for example, can be

viewed for our purposes as the violent

at rest to some final velocity in a very short time interval, or, alternatively, as the ...

The sudden creation of a fast electron in nuclear beta decay, for example, can be

viewed for our purposes as the violent

**acceleration**of a charged particle initiallyat rest to some final velocity in a very short time interval, or, alternatively, as the ...

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### Contents

Introduction to Electrostatics | 1 |

Scalar potential | 7 |

Greens theorem | 14 |

Copyright | |

18 other sections not shown

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### Common terms and phrases

4-vector acceleration angular distribution approximation assumed atomic axis behavior Bessel functions boundary conditions bremsstrahlung calculate Chapter charge density charge q charged particle classical coefficients collisions component conductor Consequently consider coordinates cross section current density cylinder defined delta function dielectric constant diffraction dimensions dipole direction discussed effects electric field electromagnetic fields electron electrostatic emitted energy loss expansion expression factor force equation frequency given Green's function impact parameter incident particle inside integral Laplace's equation limit linear Lorentz invariant Lorentz transformation macroscopic magnetic field magnetic induction magnitude Maxwell's equations meson molecules momentum multipole multipole expansion nonrelativistic obtain orbit oscillations parallel perpendicular plane wave plasma point charge polarization power radiated problem quantum quantum-mechanical radiative radius region relativistic result scalar scattering shown in Fig shows solid angle solution spectrum spherical surface theorem transverse vanishes vector potential wave equation wave number wavelength written zero