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Page 481
... emitted in orbital - electron capture by nuclei in Chapter 15 . 14.6 Frequency Spectrum of Radiation Emitted by a Relativistic Charged Particle in Instantaneously Circular Motion In Section 14.4 we saw that the radiation emitted by an ...
... emitted in orbital - electron capture by nuclei in Chapter 15 . 14.6 Frequency Spectrum of Radiation Emitted by a Relativistic Charged Particle in Instantaneously Circular Motion In Section 14.4 we saw that the radiation emitted by an ...
Page 506
... Emitted during Collisions If a charged particle makes a collision , it undergoes acceleration and emits radiation . If its collision partner is also a charged particle , they both emit radiation and a coherent superposition of the ...
... Emitted during Collisions If a charged particle makes a collision , it undergoes acceleration and emits radiation . If its collision partner is also a charged particle , they both emit radiation and a coherent superposition of the ...
Page 537
... emitted per unit energy interval because of the sudden creation of the moving mu meson . Assuming that the photons are emitted perpendicular to the direction of motion of the mu meson ( actually it is a sin2 0 distribu- tion ) , show ...
... emitted per unit energy interval because of the sudden creation of the moving mu meson . Assuming that the photons are emitted perpendicular to the direction of motion of the mu meson ( actually it is a sin2 0 distribu- tion ) , show ...
Contents
1 | 1 |
BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
Copyright | |
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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