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Page 438
... classical energy loss per unit length for a fast , heavy particle passing through matter . We suppose that there are N atoms per unit volume with Z electrons ... Classical Electrodynamics Classical and quantum-mechanical energy loss, 202 235.
... classical energy loss per unit length for a fast , heavy particle passing through matter . We suppose that there are N atoms per unit volume with Z electrons ... Classical Electrodynamics Classical and quantum-mechanical energy loss, 202 235.
Page 439
... classical result . The important quantum effects are ( 1 ) discreteness of the possible energy transfers , and ( 2 ) limitations due to the wave nature of the particles and the uncertainty principle . The problem of the discrete nature ...
... classical result . The important quantum effects are ( 1 ) discreteness of the possible energy transfers , and ( 2 ) limitations due to the wave nature of the particles and the uncertainty principle . The problem of the discrete nature ...
Page 440
... classical to quantum value of bmin is n = ze2 hv ( 13.42 ) If ŋ > 1 , the classical Bohr formula must be used . We see that this occurs for slow , highly charged , incident particles , in accord with observation . If < 1 , the quantum ...
... classical to quantum value of bmin is n = ze2 hv ( 13.42 ) If ŋ > 1 , the classical Bohr formula must be used . We see that this occurs for slow , highly charged , incident particles , in accord with observation . If < 1 , the quantum ...
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BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
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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