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Page 269
... dependence ( 9.1 ) , the solution for A becomes eik x - x ' A ( x ) == d3x ' | x − x ' - ( 9.3 ) where k = w / c is the wave number , and a sinusoidal time dependence is understood . The magnetic induction is given by B = V × A while ...
... dependence ( 9.1 ) , the solution for A becomes eik x - x ' A ( x ) == d3x ' | x − x ' - ( 9.3 ) where k = w / c is the wave number , and a sinusoidal time dependence is understood . The magnetic induction is given by B = V × A while ...
Page 296
... dependence on wave number . But the scalar result has no azimuthal dependence ( apart from that contained in § ) , whereas the vector expression does . The azimuthal variation comes from the polarization properties of the field , and ...
... dependence on wave number . But the scalar result has no azimuthal dependence ( apart from that contained in § ) , whereas the vector expression does . The azimuthal variation comes from the polarization properties of the field , and ...
Page 553
... dependence can be analyzed into its Fourier components , and we consider only harmonically varying sources , p ( x ) e - it , J ( x ) e - iot M ( x ) e -iwt ( 16.76 ) where it is understood that we take the real part of such complex ...
... dependence can be analyzed into its Fourier components , and we consider only harmonically varying sources , p ( x ) e - it , J ( x ) e - iot M ( x ) e -iwt ( 16.76 ) where it is understood that we take the real part of such complex ...
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4-vector Ampère's law angle angular distribution approximation atomic axis boundary conditions calculate Chapter charge density charge q charged particle coefficients collisions component conductor consider coordinates cross section current density cylinder d³x delta function dielectric constant diffraction dimensions dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss expansion expression factor frequency given Green's function impact parameter incident particle inside integral inversion Laplace's equation linear Lorentz transformation macroscopic magnetic field magnetic induction magnetic moment magnitude Maxwell's equations meson modes molecules momentum motion multipole nonrelativistic normal obtain oscillations P₁ parallel plasma point charge Poisson's equation polarization problem radiation radius region relativistic result scalar scalar potential scattering shown in Fig shows solution spherical surface surface-charge density theorem transverse unit V₁ vanishes vector potential velocity volume wave equation wave number wavelength written zero ΦΩ