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Page 512
... photon emitted . With this average velocity in place of v in ( 15.18 ) , we obtain Xq ( w ) ~ 16 Z2e2 ( z2 3 с Mc2 ... photon emission with dimensions of area / unit photon energy . Thus hwobrems ( hw ) d ( ħw ) = x ( w ) dw ( 15.23 ) ...
... photon emitted . With this average velocity in place of v in ( 15.18 ) , we obtain Xq ( w ) ~ 16 Z2e2 ( z2 3 с Mc2 ... photon emission with dimensions of area / unit photon energy . Thus hwobrems ( hw ) d ( ħw ) = x ( w ) dw ( 15.23 ) ...
Page 532
... photon is emitted , the neutrino has the full decay energy E , E. But when a photon of energy ho accompanies it , the neutrino's energy is reduced to E , E。 ho . Then the probability of neutrino emission is reduced by a factor , = E ...
... photon is emitted , the neutrino has the full decay energy E , E. But when a photon of energy ho accompanies it , the neutrino's energy is reduced to E , E。 ho . Then the probability of neutrino emission is reduced by a factor , = E ...
Page 549
... photon . If the z component of angular momen- tum of a single photon is known precisely , the uncertainty principle requires that the other components be uncertain , with mean square values such that ( 16.67 ) holds . On the other hand ...
... photon . If the z component of angular momen- tum of a single photon is known precisely , the uncertainty principle requires that the other components be uncertain , with mean square values such that ( 16.67 ) holds . On the other hand ...
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