## Classical electrodynamics |

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Page 474

For such small angles the

approximately (14.41) d£l _ , 77 c3 (1 + y202)5 The natural angular unit is

evidently y~l. The

in these units.

For such small angles the

**angular distribution**(14.39) can be writtenapproximately (14.41) d£l _ , 77 c3 (1 + y202)5 The natural angular unit is

evidently y~l. The

**angular distribution**is shown in Fig. 14.5 with angles measuredin these units.

Page 575

Keeping only lowest-order terms in P and making the long-wavelength

approximation, calculate the nonvanishing multipole moments, the

density of ...

Keeping only lowest-order terms in P and making the long-wavelength

approximation, calculate the nonvanishing multipole moments, the

**angular****distribution**of radiation, and the total power radiated. 16.3 The uniform chargedensity of ...

Page 636

Power, radiated,

charged particle, 470, 472 radiated, by charged particle in accelerators, 471

radiated, by charge in arbitrary periodic motion, 501 radiated, by multipoles, 550 f

. radiated, ...

Power, radiated,

**angular distribution**of quadrupole, 275, 552 radiated, bycharged particle, 470, 472 radiated, by charged particle in accelerators, 471

radiated, by charge in arbitrary periodic motion, 501 radiated, by multipoles, 550 f

. radiated, ...

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### Contents

Introduction to Electrostatics | 1 |

Scalar potential | 7 |

Greens theorem | 14 |

Copyright | |

17 other sections not shown

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### Common terms and phrases

4-vector acceleration angular distribution approximation assumed atomic average 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 photon 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