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Page 504
... spectrum N ( E ) dE ~ E TM ” dE , show that the synchrotron radiation has the power spectrum where a = ( n − 1 ) / 2 . - ( P ( w ) ) dw ~ w - α dw ( d ) Observations on the radiofrequency and optical continuous spectrum from the Crab ...
... spectrum N ( E ) dE ~ E TM ” dE , show that the synchrotron radiation has the power spectrum where a = ( n − 1 ) / 2 . - ( P ( w ) ) dw ~ w - α dw ( d ) Observations on the radiofrequency and optical continuous spectrum from the Crab ...
Page 525
... spectrum of virtual quanta I ( w ' ) is given by ( 15.54 ) with q = Ze . The minimum impact parameter is ħ / Mv , so that the frequency spectrum extends up to ' ~ yMc2 / h . The virtual quanta are scattered by the incident particle ...
... spectrum of virtual quanta I ( w ' ) is given by ( 15.54 ) with q = Ze . The minimum impact parameter is ħ / Mv , so that the frequency spectrum extends up to ' ~ yMc2 / h . The virtual quanta are scattered by the incident particle ...
Page 530
... spectrum is a typical bremsstrahlung spectrum . But for w ~ wo the intensity is very large ( infinite in our approximation ) . The behavior of the photon spectrum is shown in Fig . 15.11 . The singularity at w = ∞。 may seem alarming ...
... spectrum is a typical bremsstrahlung spectrum . But for w ~ wo the intensity is very large ( infinite in our approximation ) . The behavior of the photon spectrum is shown in Fig . 15.11 . The singularity at w = ∞。 may seem alarming ...
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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