Classical ElectrodynamicsProblems after each chapter |
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Page 439
... energy transfers , and ( 2 ) limitations due to the wave nature of the particles and the uncertainty principle . The problem of the discrete nature of the energy transfer can be illus- trated by calculating the classical energy transfer ...
... energy transfers , and ( 2 ) limitations due to the wave nature of the particles and the uncertainty principle . The problem of the discrete nature of the energy transfer can be illus- trated by calculating the classical energy transfer ...
Page 448
... energy loss for ultrarelativistic particles pro- vided their densities are such that the density of electrons is the same in each . Since there are numerous calculated curves of energy loss based on Bethe's formula ( 13.44 ) , it is ...
... energy loss for ultrarelativistic particles pro- vided their densities are such that the density of electrons is the same in each . Since there are numerous calculated curves of energy loss based on Bethe's formula ( 13.44 ) , it is ...
Page 537
... energy transfer per collision is much smaller . Show that the energy loss is divided approximately equally between the two kinds of collisions , and verify that your total energy loss is in essential agreement with Bethe's result ...
... energy transfer per collision is much smaller . Show that the energy loss is divided approximately equally between the two kinds of collisions , and verify that your total energy loss is in essential agreement with Bethe's result ...
Contents
1 | 1 |
BoundaryValue Problems in Electrostatics I | 26 |
Dielectrics | 98 |
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4-vector acceleration Ampère's law angular distribution approximation atomic axis behavior boundary conditions bremsstrahlung calculation Chapter charge q charged particle Cherenkov radiation classical coefficients collisions component conducting conductor consider constant coordinate cross section cylinder d³x dielectric diffraction dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic emitted energy loss energy transfer equation of motion factor force equation frame frequency given Green's function impact parameter incident particle integral Lagrangian limit Lorentz force Lorentz invariant Lorentz transformation m₁ magnetic field magnetic induction magnitude Maxwell's equations meson modes momentum multipole nonrelativistic obtain orbit oscillations P₁ P₂ parallel perpendicular photon plane plasma polarization power radiated problem quantum quantum-mechanical radius region relativistic result scalar scattering screen shown in Fig shows sin² solid angle solution spectrum sphere spherical surface transverse V₁ vanishes vector potential wave number wavelength ΦΩ