Classical ElectrodynamicsIntroduction to electrostatics. Boudary-value problems in electrostatics: I. Boundary-value problems in electrostatics: II. Multipoles, electrostatics of macroscopic media, dielectrics. Magnetostatics. Time-varying fields, maxwell equations, conservation laws. Plane electromagnetic waves and wave propagation. Wave guides and resonant cavities. Simple radiating systems, scattering, and diffraction. Magnetohydrodynamics and plasma physics. Special theory of relativity. Dynamics of relativistic particles and electromagnetic fields. Collisions between charged particles, energy loss, and scattering. Radiation by moving charges. Bremsstrahlung, method of virtual quanta, radiative beta processes. Multipole fields. Radiation damping, self-fields of a particle, scattering and absorption of radiation by a bound system. Units and dimensions, basic units and derived units. Electromagnetic units and equations. Various systems of electromagnetic units. Conversion of equations and amounts between Gaussian units and MKSA units. |
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Page 370
... given by ( 8.31 ) and ( 8.33 ) and E2 , H2 are the longitudinal fields . The wave number k 、 is given by ( 8.37 ) and is taken to be real and positive for propagating modes in lossless guides . A time dependence e it is , of course ...
... given by ( 8.31 ) and ( 8.33 ) and E2 , H2 are the longitudinal fields . The wave number k 、 is given by ( 8.37 ) and is taken to be real and positive for propagating modes in lossless guides . A time dependence e it is , of course ...
Page 496
... given by Im w -Wp 度(笑) e ̃ ( k2 / 2k2 ) ( 10.93 ) provided k <<< kD . To obtain ( 10.93 ) a Maxwellian distribution of velocities was assumed . For k≥k , the damping constant is larger than given by ( 10.93 ) and rapidly becomes much ...
... given by Im w -Wp 度(笑) e ̃ ( k2 / 2k2 ) ( 10.93 ) provided k <<< kD . To obtain ( 10.93 ) a Maxwellian distribution of velocities was assumed . For k≥k , the damping constant is larger than given by ( 10.93 ) and rapidly becomes much ...
Page 699
... given in milligauss and E in GeV . What is the half - life using the numbers from part ( a ) ? How does this compare with the known lifetime of the Crab nebula ? Must the energetic electrons be continually replenished ? From what source ...
... given in milligauss and E in GeV . What is the half - life using the numbers from part ( a ) ? How does this compare with the known lifetime of the Crab nebula ? Must the energetic electrons be continually replenished ? From what source ...
Contents
L2 The Inverse Square Law or the Mass of the Photon | 1 |
BoundaryValue Problems | 54 |
Multipoles Electrostatics | 136 |
Copyright | |
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4-vector Ampère's law amplitude angle angular distribution angular momentum approximation atomic axis behavior boundary conditions calculate Chapter charge density charge q charged particle classical coefficients collision components conducting conductor consider coordinates cross section current density cylinder d³x defined dielectric constant diffraction dimensions dipole direction discussed electric and magnetic electric field electromagnetic fields electrons electrostatic expansion expression factor force frame frequency given Green function incident integral limit linear Lorentz transformation macroscopic magnetic field magnetic induction magnetic monopole magnitude Maxwell equations medium modes molecules motion multipole multipole expansion multipole moments nonrelativistic normal obtained oscillations parallel parameter photon Phys plane wave plasma polarization problem propagation quantum quantum-mechanical radiation radius region relativistic result scattering shown in Fig sin² solution spectrum sphere spherical surface tensor theorem transverse unit vanishes vector potential velocity volume wave guide wave number wavelength written zero ΦΩ