## Classical Electrodynamics |

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Page 501

14.5 14.6 14.7 14.8 more energy while near the equator, or while near its turning

points? Why? Make quantitative statements if you can. As in Problem 14.2a a

charge e moves in simple harmonic

14.5 14.6 14.7 14.8 more energy while near the equator, or while near its turning

points? Why? Make quantitative statements if you can. As in Problem 14.2a a

charge e moves in simple harmonic

**motion**along the z axis, z(t') = a cos (apot').Page 581

Since oo-" is a time appropriate to the mechanical

the relevant mechanical time interval is long compared to the characteristic time t

(17.3), radiative reaction effects on the

...

Since oo-" is a time appropriate to the mechanical

**motion**, again we see that, ifthe relevant mechanical time interval is long compared to the characteristic time t

(17.3), radiative reaction effects on the

**motion**will be unimportant. The examples...

Page 597

A discussion similar in some respects to that given here was presented by Wilson

.f 17.7 Integrodifferential Equation of

Section 17.2 the Abraham-Lorentz equation (17.9) was discussed qualitatively.

A discussion similar in some respects to that given here was presented by Wilson

.f 17.7 Integrodifferential Equation of

**Motion**, Including Radiation Damping InSection 17.2 the Abraham-Lorentz equation (17.9) was discussed qualitatively.

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### Contents

Introduction to Electrostatics | 1 |

BoundaryValue Problems in Electrostatics I | 26 |

Multipoles Electrostatics of Macroscopic Media | 98 |

Copyright | |

5 other sections not shown

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acceleration angle angular applied approximation assumed atomic average axis becomes boundary conditions calculate called Chapter charge charged particle 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 light limit Lorentz loss magnetic magnetic field magnetic induction magnitude mass means 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 shown in Fig shows side solution space sphere spherical surface transformation unit vanishes vector velocity volume wave written