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... motion as d ( ymv ) dt = 0 ( 12.67 ) - where y = [ 1 ( v2 / c2 ) ] . At the least sophisticated level we know that the Lagrangian L must be chosen strategically so that the Euler - Lagrange equations of motion , dt 4 ( 24 ) - 24 . = 0 ...
... motion as d ( ymv ) dt = 0 ( 12.67 ) - where y = [ 1 ( v2 / c2 ) ] . At the least sophisticated level we know that the Lagrangian L must be chosen strategically so that the Euler - Lagrange equations of motion , dt 4 ( 24 ) - 24 . = 0 ...
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... motion . 14.6 Show explicitly by use of the Poisson sum formula or other means that , if the motion of a radiating particle repeats itself with periodicity T , the continuous frequency spectrum becomes a discrete spectrum containing ...
... motion . 14.6 Show explicitly by use of the Poisson sum formula or other means that , if the motion of a radiating particle repeats itself with periodicity T , the continuous frequency spectrum becomes a discrete spectrum containing ...
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... motions of charged particles or currents are calculated . Antennas and radiation from multipole sources are examples of the first type of problem , while motion of charges in electric and magnetic fields and energy - loss phenomena are ...
... motions of charged particles or currents are calculated . Antennas and radiation from multipole sources are examples of the first type of problem , while motion of charges in electric and magnetic fields and energy - loss phenomena are ...
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