Classical Electrodynamics |
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Page 189
... electromagnetic energy into mechanical or thermal energy . It must be balanced by a corresponding rate of decrease of energy in the electromagnetic field within the volume V. In order to exhibit this conservation law explicitly , we ...
... electromagnetic energy into mechanical or thermal energy . It must be balanced by a corresponding rate of decrease of energy in the electromagnetic field within the volume V. In order to exhibit this conservation law explicitly , we ...
Page 590
... electromagnetic structures of the neutron and proton . These have been explored by high - energy electron scattering , assuming that the electrons are point particles with no structure and that no changes occur in electro- dynamics at ...
... electromagnetic structures of the neutron and proton . These have been explored by high - energy electron scattering , assuming that the electrons are point particles with no structure and that no changes occur in electro- dynamics at ...
Page 616
... Electromagnetic Units The various systems of electromagnetic units differ in their choices of the magnitudes and dimensions of the various constants above . Because of relations ( A.5 ) and ( A.11 ) there are only two constants ( e.g. ...
... Electromagnetic Units The various systems of electromagnetic units differ in their choices of the magnitudes and dimensions of the various constants above . Because of relations ( A.5 ) and ( A.11 ) there are only two constants ( e.g. ...
Common terms and phrases
4-vector acceleration Ampère's law angle angular distribution antenna approximation atomic axis Babinet's principle behavior boundary conditions calculate cavity Chapter charge q charged particle coefficients collisions component conducting conductor constant coordinate cross section cylinder d³x dielectric dielectric constant diffraction dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss factor force equation frame frequency given Green's function impact parameter incident particle integral Kirchhoff Lagrangian Laplace's equation Lorentz force Lorentz invariant Lorentz transformation m₁ magnetic field magnetic induction magnitude Maxwell's equations meson modes momentum multipole nonrelativistic obtain oscillations P₁ P₂ parallel perpendicular phase velocity plane wave plasma polarization power radiated problem propagation radius region relativistic result scalar scattering screen shown in Fig shows sin² solution sphere spherical surface transverse unit V₁ vanishes vector potential velocity wave guide wave number wavelength ΦΩ