Classical Electrodynamics |
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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 448
... energy loss for ultrarelativistic particles pro- vided their densities are such that the density of electrons is the same in each . Since there are numerous calculated curves of energy loss based on Bethe's formula ( 13.44 ) , it is ...
... energy loss for ultrarelativistic particles pro- vided their densities are such that the density of electrons is the same in each . Since there are numerous calculated curves of energy loss based on Bethe's formula ( 13.44 ) , it is ...
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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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