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Page 15
... zero field and zero potential outside the volume V. ] - Two remarks are in order about result ( 1.36 ) . First , if the surface S goes to infinity and the electric field on S falls off faster than R - 1 , then the surface integral ...
... zero field and zero potential outside the volume V. ] - Two remarks are in order about result ( 1.36 ) . First , if the surface S goes to infinity and the electric field on S falls off faster than R - 1 , then the surface integral ...
Page 94
... zero . For the nonvanishing terms , exhibit the coefficients as an integral over cos 0 . ( b ) For the special case of n = 1 ( two hemispheres ) determine explicitly the potential up to and including all terms with 1 = 3. By a ...
... zero . For the nonvanishing terms , exhibit the coefficients as an integral over cos 0 . ( b ) For the special case of n = 1 ( two hemispheres ) determine explicitly the potential up to and including all terms with 1 = 3. By a ...
Page 236
... zero electric field inside the perfect conductor . Similarly , for time - varying magnetic fields , the surface charges move in response to the tangential magnetic field to produce always the correct surface current K : 4πT nx H = K ...
... zero electric field inside the perfect conductor . Similarly , for time - varying magnetic fields , the surface charges move in response to the tangential magnetic field to produce always the correct surface current K : 4πT nx H = K ...
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