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... orbit coupling by a factor of ( sometimes called the Thomas factor ) , yielding e U = - S.B + mc 1 2m2c2 S.L 1 dV r dr ( 11.56 ) as the correct spin - orbit interaction energy for an atomic electron . In atomic nuclei the nucleons ...
... orbit coupling by a factor of ( sometimes called the Thomas factor ) , yielding e U = - S.B + mc 1 2m2c2 S.L 1 dV r dr ( 11.56 ) as the correct spin - orbit interaction energy for an atomic electron . In atomic nuclei the nucleons ...
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... orbit . If the particle moves through regions where the magnetic field strength varies slowly in space or time , the adiabatic invariance of J means that the flux linked by the particle's orbit remains constant . If B increases , the ...
... orbit . If the particle moves through regions where the magnetic field strength varies slowly in space or time , the adiabatic invariance of J means that the flux linked by the particle's orbit remains constant . If B increases , the ...
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... orbit of very large quantum number around a nucleus down to the low - lying orbits . Over most of the time interval the quantum numbers are sufficiently large that the classical description of continuous motion is an adequate ...
... orbit of very large quantum number around a nucleus down to the low - lying orbits . Over most of the time interval the quantum numbers are sufficiently large that the classical description of continuous motion is an adequate ...
Contents
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Greens theorem | 14 |
BoundaryValue Problems in Electrostatics I | 26 |
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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