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Page 248
... gives the time - averaged flux of energy . For the two types of field we find , using ( 8.24 ) : wk S = 8пуя [ C [ GIVIN2 + 12 VON ] k - i k ( 8.48 ) where the upper ( lower ) line is for TM ( TE ) modes . Since y is generally real ...
... gives the time - averaged flux of energy . For the two types of field we find , using ( 8.24 ) : wk S = 8пуя [ C [ GIVIN2 + 12 VON ] k - i k ( 8.48 ) where the upper ( lower ) line is for TM ( TE ) modes . Since y is generally real ...
Page 366
... gives the anomalous Zeeman effect correctly , but has a spin - orbit interaction which is twice too large . The error in ( 11.45 ) can be traced to the incorrectness of ( 11.40 ) as an equation of motion for the electron spin . The left ...
... gives the anomalous Zeeman effect correctly , but has a spin - orbit interaction which is twice too large . The error in ( 11.45 ) can be traced to the incorrectness of ( 11.40 ) as an equation of motion for the electron spin . The left ...
Page 439
... gives an energy transfer large compared to typical atomic excitation energies would we expect it to be correct . This would set quite a different upper limit on the impact parameters . Fortunately the classical result can be applied in ...
... gives an energy transfer large compared to typical atomic excitation energies would we expect it to be correct . This would set quite a different upper limit on the impact parameters . Fortunately the classical result can be applied in ...
Contents
1 | 1 |
BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
Copyright | |
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4-vector acceleration Ampère's law angular distribution antenna approximation atomic axis B₁ Babinet's principle behavior boundary conditions calculate Chapter charge q charged particle coefficients collisions component conducting conductor consider constant coordinate cross section cylinder d³x dielectric diffraction dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss energy transfer 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 momentum multipole nonrelativistic obtain oscillations P₁ P₂ parallel perpendicular phase velocity plane wave plasma polarization power radiated problem radius region relativistic result S₁ scalar scattering screen shown in Fig shows sin² solid angle solution sphere spherical surface transverse unit V₁ vanishes vector potential velocity wave number wavelength ΦΩ