Classical Electrodynamics |
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Page 519
... radiative loss is proportional to the particle's energy . The comparison of radiative loss to collision loss now becomes In dErad dEcoll 4 Zz2 m 3π 137 / M 1192M Zm γ In Ba ( 15.46 ) ~ The value of y for which this ratio is unity ...
... radiative loss is proportional to the particle's energy . The comparison of radiative loss to collision loss now becomes In dErad dEcoll 4 Zz2 m 3π 137 / M 1192M Zm γ In Ba ( 15.46 ) ~ The value of y for which this ratio is unity ...
Page 581
... radiative reaction effects on the motion will be unimportant . The examples of the last two paragraphs show that the reactive effects of radiation on the motion of a charged particle can be expected to be important if the external ...
... radiative reaction effects on the motion will be unimportant . The examples of the last two paragraphs show that the reactive effects of radiation on the motion of a charged particle can be expected to be important if the external ...
Page 630
... radiative reaction , 597 Equations of motion with radiative re- action , 582 , 583 Ether , 347 Ether drift , experiment on , 349 Expansion , of circularly polarized plane wave , 569 of eikR / R , 541 of retarded quantity , 586 of scalar ...
... radiative reaction , 597 Equations of motion with radiative re- action , 582 , 583 Ether , 347 Ether drift , experiment on , 349 Expansion , of circularly polarized plane wave , 569 of eikR / R , 541 of retarded quantity , 586 of scalar ...
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