Classical Electrodynamics |
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Page 443
John David Jackson. 13.4 Density Effect in Collision Energy Loss For particles which are not too relativistic the observed energy loss is given accurately by ( 13.44 ) [ or by ( 13.36 ) if ŋ > 1 ] for all kinds of particles in all types ...
John David Jackson. 13.4 Density Effect in Collision Energy Loss For particles which are not too relativistic the observed energy loss is given accurately by ( 13.44 ) [ or by ( 13.36 ) if ŋ > 1 ] for all kinds of particles in all types ...
Page 448
... energy loss no longer depends on the details of atomic structure through ( w ) ( 13.38 ) , but only on the number of electrons per unit volume through o ,. Two substances having very different atomic struc- tures will produce the same ...
... energy loss no longer depends on the details of atomic structure through ( w ) ( 13.38 ) , but only on the number of electrons per unit volume through o ,. Two substances having very different atomic struc- tures will produce the same ...
Page 449
... Energy loss , including the density effect . The dotted curve is the total energy loss without density correction . The solid curves have the density effect incorporated , the upper one being the total energy loss and the lower one the ...
... Energy loss , including the density effect . The dotted curve is the total energy loss without density correction . The solid curves have the density effect incorporated , the upper one being the total energy loss and the lower one the ...
Common terms and phrases
4-vector acceleration Ampère's law angle angular distribution antenna approximation atomic axis 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 dielectric constant diffraction dipole direction discussed E₁ electric field electromagnetic fields electron electrostatic energy loss 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 phase velocity plane wave plasma polarization power radiated problem propagation radius region relativistic result scalar scattering screen shown in Fig shows sin² solution sphere spherical surface transverse unit V₁ vanishes vector potential velocity wave guide wave number wavelength ΦΩ