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Page 102
... consequently ( length ) 2 . Unless the circum- stances are exceptional ( e.g. , nuclei in atoms with completely closed electronic shells ) , nuclei are subjected to internal fields which possess field gradients in the neighborhood of ...
... consequently ( length ) 2 . Unless the circum- stances are exceptional ( e.g. , nuclei in atoms with completely closed electronic shells ) , nuclei are subjected to internal fields which possess field gradients in the neighborhood of ...
Page 120
... Consequently the induced dipole moment is e2 Pmolex = E 2 mwo ( 4.77 ) This means that the polarizability is y e2 / m2 . If there are Z electrons per molecule , f , having a restoring force constant mo , 2 ( Σf ; = Z ) , then the ...
... Consequently the induced dipole moment is e2 Pmolex = E 2 mwo ( 4.77 ) This means that the polarizability is y e2 / m2 . If there are Z electrons per molecule , f , having a restoring force constant mo , 2 ( Σf ; = Z ) , then the ...
Page 324
... Consequently each particle colliding with the plasma surface receives a momentum transfer 2MR . The number colliding with unit area of the surface per unit time is NŔ , where N is the initial number of particles per unit volume ...
... Consequently each particle colliding with the plasma surface receives a momentum transfer 2MR . The number colliding with unit area of the surface per unit time is NŔ , where N is the initial number of particles per unit volume ...
Contents
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BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
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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