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Page 513
... photon energy , the main dependence of the cross section on photon energy is as ( ħw ) -1 , known as the typical bremsstrahlung spectrum . The radiation cross section ( w ) depends on the properties of the particles involved in the ...
... photon energy , the main dependence of the cross section on photon energy is as ( ħw ) -1 , known as the typical bremsstrahlung spectrum . The radiation cross section ( w ) depends on the properties of the particles involved in the ...
Page 520
... photon interaction . The table lists a few typical correspondences and specifies the incident particle and Correspondences between charged particle interactions and photon interactions Particle Process Incident Particle Struck System ...
... photon interaction . The table lists a few typical correspondences and specifies the incident particle and Correspondences between charged particle interactions and photon interactions Particle Process Incident Particle Struck System ...
Page 530
... photon spectrum is shown in Fig . 15.11 . The singularity at w = ∞。 may seem alarming , but it is really quite natural and expected . If the electron were to keep orbiting forever , the radiation spectrum would be a sharp line at ww ...
... photon spectrum is shown in Fig . 15.11 . The singularity at w = ∞。 may seem alarming , but it is really quite natural and expected . If the electron were to keep orbiting forever , the radiation spectrum would be a sharp line at ww ...
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4-vector Ampère's law angle angular distribution approximation atomic axis boundary conditions calculate Chapter charge density charge q charged particle coefficients collisions component conductor consider coordinates cross section current density cylinder d³x delta function dielectric constant diffraction dimensions dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss expansion expression factor frequency given Green's function impact parameter incident particle inside integral inversion Laplace's equation linear Lorentz transformation macroscopic magnetic field magnetic induction magnetic moment magnitude Maxwell's equations meson modes molecules momentum motion multipole nonrelativistic normal obtain oscillations P₁ parallel plasma point charge Poisson's equation polarization problem radiation radius region relativistic result scalar scalar potential scattering shown in Fig shows solution spherical surface surface-charge density theorem transverse unit V₁ vanishes vector potential velocity volume wave equation wave number wavelength written zero ΦΩ