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Page ix
... classical electrodynamics . And even after almost 60 years , classical electrodynamics still impresses and delights as a beautiful example of the covariance of physical laws under Lorentz transformations . The special theory of ...
... classical electrodynamics . And even after almost 60 years , classical electrodynamics still impresses and delights as a beautiful example of the covariance of physical laws under Lorentz transformations . The special theory of ...
Page 511
... classical result holds only when ŋ > 1 , we see that 1 ( c ) @max ( a ) ( a ) @max @max η ( 15.20 ) This shows that the classical frequency spectrum is always confined to very low frequencies compared to the maximum allowed by ...
... classical result holds only when ŋ > 1 , we see that 1 ( c ) @max ( a ) ( a ) @max @max η ( 15.20 ) This shows that the classical frequency spectrum is always confined to very low frequencies compared to the maximum allowed by ...
Page 532
... classical spectra ( 15.83 ) and ( 15.84 ) must be corrected by multiplication with ( 15.85 ) to take into account the kinematics of the neutrino emission . The modified classical photon spectrum is N ( hw ) = e2 ho ( 1 2πhс ( mc2 ) 2 ...
... classical spectra ( 15.83 ) and ( 15.84 ) must be corrected by multiplication with ( 15.85 ) to take into account the kinematics of the neutrino emission . The modified classical photon spectrum is N ( hw ) = e2 ho ( 1 2πhс ( mc2 ) 2 ...
Contents
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BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
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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