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... relativistic radiation patterns , regardless of the vectorial relation between ẞ and B. The total power radiated can ... relativistic peaking at forward angles is present . In the relativistic limit ( y > 1 ) , the angular 9/9 -1.0 0 1.0 ...
... relativistic radiation patterns , regardless of the vectorial relation between ẞ and B. The total power radiated can ... relativistic peaking at forward angles is present . In the relativistic limit ( y > 1 ) , the angular 9/9 -1.0 0 1.0 ...
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... relativistic bremsstrahlung calculation can be done nonrelativistically . There are two aspects . First of all , we know that radiation emitted by a highly relativistic particle is confined to a narrow cone of half - angle of the order ...
... relativistic bremsstrahlung calculation can be done nonrelativistically . There are two aspects . First of all , we know that radiation emitted by a highly relativistic particle is confined to a narrow cone of half - angle of the order ...
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... Relativistic notation , 377 Relativistic transformation , and Thomas precession , 367 from CM system to laboratory , 400 f . of acceleration , 388 of charge and current densities , 378 of coordinates , 357 of electromagnetic fields ...
... Relativistic notation , 377 Relativistic transformation , and Thomas precession , 367 from CM system to laboratory , 400 f . of acceleration , 388 of charge and current densities , 378 of coordinates , 357 of electromagnetic fields ...
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