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Page 213
... origin , such that at t = 0 they coalesced into the shape given by ( 7.38 ) . Clearly at later times we expect each pulse to re - emerge on the other side of the origin . Consequently the initial distribution ( 7.38 ) may be expected to ...
... origin , such that at t = 0 they coalesced into the shape given by ( 7.38 ) . Clearly at later times we expect each pulse to re - emerge on the other side of the origin . Consequently the initial distribution ( 7.38 ) may be expected to ...
Page 436
... origin O. Using the Fourier representations ( 13.16 ) and ( 13.17 ) , as well as that for a delta function ( 2.52 ) ... origin O at an impact parameter b with a velocity v , the electromagnetic fields at the origin are given by ( 11.118 ) ...
... origin O. Using the Fourier representations ( 13.16 ) and ( 13.17 ) , as well as that for a delta function ( 2.52 ) ... origin O at an impact parameter b with a velocity v , the electromagnetic fields at the origin are given by ( 11.118 ) ...
Page 482
... origin of time is chosen so that at t = 0 the particle is at the origin of coordinates . The vector part of the integrand in ( 14.67 ) can be written n x ( n x B ) = -- -El sin vt vt + € 1 cos sin 0 ( 14.75 ) = where = € , is a unit ...
... origin of time is chosen so that at t = 0 the particle is at the origin of coordinates . The vector part of the integrand in ( 14.67 ) can be written n x ( n x B ) = -- -El sin vt vt + € 1 cos sin 0 ( 14.75 ) = where = € , is a unit ...
Contents
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BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
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4-vector acceleration Ampère's law angle angular distribution antenna approximation atomic axis B₁ Babinet's principle behavior boundary conditions calculate cavity Chapter charge q charged particle coefficients collisions component conducting conductor constant coordinate cross section cylinder d³x dielectric diffraction dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss energy transfer factor force equation frame 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 P₂ parallel perpendicular plasma polarization power radiated problem radius region relativistic result S₁ scalar scattering screen shown in Fig shows sin² solid angle solution sphere spherical surface transverse unit V₁ vanishes vector potential velocity wave guide wave number wavelength ΦΩ