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Page 20
... physical interchangeability of the source and the observation points . For Neumann boundary conditions the symmetry is not automatic , but can be imposed as a separate requirement . As a final , important remark we note the physical ...
... physical interchangeability of the source and the observation points . For Neumann boundary conditions the symmetry is not automatic , but can be imposed as a separate requirement . As a final , important remark we note the physical ...
Page 369
... physical con- sequences of the special theory of relativity and Lorentz transformations . In the next two sections we want now to discuss some of the more formal aspects and to introduce some notation and concepts which are very useful ...
... physical con- sequences of the special theory of relativity and Lorentz transformations . In the next two sections we want now to discuss some of the more formal aspects and to introduce some notation and concepts which are very useful ...
Page 607
... physical requirements that ( a ) the normal modes of oscil- lation of the system must decay in time ( even if very slowly ) because of ever - present resistive losses , and ( b ) at high frequencies binding effects are unimportant and ...
... physical requirements that ( a ) the normal modes of oscil- lation of the system must decay in time ( even if very slowly ) because of ever - present resistive losses , and ( b ) at high frequencies binding effects are unimportant and ...
Contents
1 | 1 |
BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
Copyright | |
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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