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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 NŘ , 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 NŘ , where N is the initial number of particles per unit volume ...
Page 429
... Consequently the path is much less straight . After a short distance , electrons tend to diffuse into the material , rather than go in a rectilinear path . The subject of energy loss and scattering is an important one and is discussed ...
... Consequently the path is much less straight . After a short distance , electrons tend to diffuse into the material , rather than go in a rectilinear path . The subject of energy loss and scattering is an important one and is discussed ...
Page 470
... Consequently these radiative effects are largest for electrons . We will restrict our discussion to them . In a linear accelerator the motion is one dimensional . From ( 14.25 ) it is evident that in that case the radiated power is P ...
... Consequently these radiative effects are largest for electrons . We will restrict our discussion to them . In a linear accelerator the motion is one dimensional . From ( 14.25 ) it is evident that in that case the radiated power is P ...
Contents
1 | 1 |
BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
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 coefficients collisions component conducting conductor consider 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 momentum multipole nonrelativistic obtain oscillations P₁ P₂ parallel perpendicular phase velocity plane wave 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 number wavelength ΦΩ