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 r2er sin2 0 64π ( a ) Make a multipole expansion of the potential due to this charge density and determine ...
... determine the fractional difference in radius ( a — b ) / R . 4.3 A localized distribution of charge has a charge density p ( r ) = 1 r2er sin2 0 64π ( a ) Make a multipole expansion of the potential due to this charge density and determine ...
Page 576
... determine the transcendental equations for the characteristic frequencies win of the cavity for TE and TM modes . In ( b ) Calculate numerical values for the wavelength λn in units of the radius a for the four lowest modes for TE and TM ...
... determine the transcendental equations for the characteristic frequencies win of the cavity for TE and TM modes . In ( b ) Calculate numerical values for the wavelength λn in units of the radius a for the four lowest modes for TE and TM ...
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4-vector Ampère's law angle angular distribution approximation atomic axis boundary conditions calculate Chapter charge density charge q charged particle coefficients collisions component conductor consider coordinates cross section current density cylinder d³x delta function dielectric constant diffraction dimensions dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss expansion expression factor frequency given Green's function impact parameter incident particle inside integral inversion Laplace's equation linear Lorentz transformation macroscopic magnetic field magnetic induction magnetic moment magnitude Maxwell's equations meson modes molecules momentum motion multipole nonrelativistic normal obtain oscillations P₁ parallel plasma point charge Poisson's equation polarization problem radiation radius region relativistic result scalar scalar potential scattering shown in Fig shows solution spherical surface surface-charge density theorem transverse unit V₁ vanishes vector potential velocity volume wave equation wave number wavelength written zero ΦΩ