Classical ElectrodynamicsProblems after each chapter |
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Page 94
... determine exactly which coefficients are different from zero . For the nonvanishing terms , exhibit the coefficients as an integral over cos 0 . ( b ) For the special case of n = 1 ( two hemispheres ) determine explicitly the potential ...
... determine exactly which coefficients are different from zero . For the nonvanishing terms , exhibit the coefficients as an integral over cos 0 . ( b ) For the special case of n = 1 ( two hemispheres ) determine explicitly the potential ...
Page 129
... determine the fractional difference in radius ( a - b ) / R . 4.3 A localized distribution of charge has a charge density p ( r ) = 1 64π r2er sin2 0 = ( a ) Make a multipole expansion of the potential due to this charge density and ...
... determine the fractional difference in radius ( a - b ) / R . 4.3 A localized distribution of charge has a charge density p ( r ) = 1 64π r2er sin2 0 = ( a ) Make a multipole expansion of the potential due to this charge density and ...
Page 451
... determine the energy loss , whereas collisions with atoms determine the scattering . If the screening of the nuclear Coulomb field by the atomic electrons is neglected , a fast particle of momentum p = yMv and charge ze , [ Sect . 13.6 ] ...
... determine the energy loss , whereas collisions with atoms determine the scattering . If the screening of the nuclear Coulomb field by the atomic electrons is neglected , a fast particle of momentum p = yMv and charge ze , [ Sect . 13.6 ] ...
Contents
1 | 1 |
BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
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4-vector acceleration Ampère's law angular distribution approximation atomic axis behavior boundary conditions bremsstrahlung calculation Chapter charge q charged particle Cherenkov radiation classical coefficients collisions component conducting conductor consider constant coordinate cross section cylinder d³x dielectric diffraction dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic emitted energy loss energy transfer equation of motion factor force equation frame frequency given Green's function impact parameter incident particle integral Lagrangian limit Lorentz force Lorentz invariant Lorentz transformation m₁ magnetic field magnetic induction magnitude Maxwell's equations meson modes momentum multipole nonrelativistic obtain orbit oscillations P₁ P₂ parallel perpendicular photon plane plasma polarization power radiated problem quantum quantum-mechanical radius region relativistic result scalar scattering screen shown in Fig shows sin² solid angle solution spectrum sphere spherical surface transverse V₁ vanishes vector potential wave number wavelength ΦΩ