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... photon emitted . With this average velocity in place of v in ( 15.18 ) , we obtain 16 Z2e2 ( z2e2 2 2 2 2 Xq ( w ) ... photon emission with dimensions of area / unit photon energy . Thus hwobrems ( hw ) d ( hw ) = x ( w ) dw ( 15.23 ) The ...
... photon emitted . With this average velocity in place of v in ( 15.18 ) , we obtain 16 Z2e2 ( z2e2 2 2 2 2 Xq ( w ) ... photon emission with dimensions of area / unit photon energy . Thus hwobrems ( hw ) d ( hw ) = x ( w ) dw ( 15.23 ) The ...
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... 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 , = 2 ...
... 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 , = 2 ...
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... 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
1 | 1 |
Greens theorem | 14 |
BoundaryValue Problems in Electrostatics I | 26 |
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 classical coefficients collisions component conducting conductor constant coordinate cross section cylinder d³x dielectric diffraction dimensions dipole direction discussed E₁ effects electric field electromagnetic fields electrons electrostatic energy loss energy transfer factor force equation formula frequency given Green's function impact parameter incident particle integral Kirchhoff Lorentz invariant Lorentz transformation magnetic field magnetic induction magnitude Maxwell's equations meson modes momentum motion multipole nonrelativistic obtain oscillations P₁ parallel perpendicular plane wave plasma plasma oscillations polarization power radiated Poynting's vector problem propagation quantum quantum-mechanical radius region relativistic result 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