## Classical Electrodynamics |

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Page 472

14.3 Angular Distribution of Radiation Emitted by an

the

14.3 Angular Distribution of Radiation Emitted by an

**Accelerated**Charge For an**accelerated**charge in nonrelativistic motion the angular ... For relativistic motionthe

**acceleration**fields depend on the velocity as well as the**acceleration**.Page 475

(14.46) 3 co It is instructive to compare the power radiated for

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

perpendicular to the velocity (14.46) for the same magnitude of applied force.

(14.46) 3 co It is instructive to compare the power radiated for

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

**acceleration**perpendicular to the velocity (14.46) for the same magnitude of applied force.

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 |

BoundaryValue Problems in Electrostatics I | 26 |

BoundaryValue Problems in Electrostatics II | 54 |

Copyright | |

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acceleration angle angular applied approximation assumed atomic average axis becomes boundary conditions calculate called Chapter charge classical collisions compared component conducting Consequently consider constant coordinates cross section cylinder defined density dependence derivative determine dielectric dimensions dipole direction discussed distance distribution effects electric field electromagnetic electron electrostatic energy equal equation example expansion expression factor force frame frequency function given gives incident inside integral involved limit Lorentz loss magnetic magnetic field magnetic induction magnitude mass means modes momentum motion moving multipole normal observation obtain origin parallel particle physical plane plasma polarization position potential problem properties radiation radius region relation relative relativistic result satisfy scalar scattering shows side solution space sphere spherical surface transformation unit vanishes vector velocity volume wave written