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... nonrelativistic motion shows that λ = mc2 , yielding the free - particle Lagrangian ( 12.69 ) . The general requirement that yL be Lorentz invariant allows us to determine the Lagrangian for a relativistic charged particle in external ...
... nonrelativistic motion shows that λ = mc2 , yielding the free - particle Lagrangian ( 12.69 ) . The general requirement that yL be Lorentz invariant allows us to determine the Lagrangian for a relativistic charged particle in external ...
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... nonrelativistic and relativistic 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 ...
... nonrelativistic and relativistic 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 ...
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... nonrelativistic and relativistic charged particles in external fields were treated . The present chapter is devoted to problems of emission of electromagnetic radiation by charged particles in atomic and nuclear processes . Particles ...
... nonrelativistic and relativistic charged particles in external fields were treated . The present chapter is devoted to problems of emission of electromagnetic radiation by charged particles in atomic and nuclear processes . Particles ...
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