Classical ElectrodynamicsProblems after each chapter |
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Page 22
... energy . There is perhaps one puzzling thing about ( 1.55 ) . The energy density is positive definite . Consequently its volume integral is necessarily non- negative . This seems to contradict our impression from ( 1.51 ) that the ...
... energy . There is perhaps one puzzling thing about ( 1.55 ) . The energy density is positive definite . Consequently its volume integral is necessarily non- negative . This seems to contradict our impression from ( 1.51 ) that the ...
Page 439
... energy transfers , and ( 2 ) limitations due to the wave nature of the particles and the uncertainty principle . The problem of the discrete nature of the energy transfer can be illus- trated by calculating the classical energy transfer ...
... energy transfers , and ( 2 ) limitations due to the wave nature of the particles and the uncertainty principle . The problem of the discrete nature of the energy transfer can be illus- trated by calculating the classical energy transfer ...
Page 537
... energy transfer per collision is much smaller . Show that the energy loss is divided approximately equally between the two kinds of collisions , and verify that your total energy loss is in essential agreement with Bethe's result ...
... energy transfer per collision is much smaller . Show that the energy loss is divided approximately equally between the two kinds of collisions , and verify that your total energy loss is in essential agreement with Bethe's result ...
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Common terms and phrases
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