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 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 ...
Contents
1 | 1 |
BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
Copyright | |
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4-vector Ampère's law angle angular distribution antenna approximation atomic axis B₁ Babinet's principle behavior boundary conditions calculate cavity Chapter charged particle coefficients collisions component conducting conductor consider constant coordinate cross section cylinder d³x dielectric diffraction dimensions dipole direction discussed E₁ electric field electromagnetic fields electrons electrostatic energy loss factor force equation 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 parallel perpendicular phase velocity plane wave plasma polarization power radiated Poynting's vector problem propagation radius region relativistic result S₁ 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