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... limits ( 3.103 ) . Then in the relativistic limit the Fermi expression ( 13.70 ) is dE 2 ( 20 ) 2 Re ( " too ( 1 ) пс2 X io [ In ( 1.123 ) -In ( 1- ( ) ] do ( 13.75 ) ωα € It is worth while right here to point out that the argument of ...
... limits ( 3.103 ) . Then in the relativistic limit the Fermi expression ( 13.70 ) is dE 2 ( 20 ) 2 Re ( " too ( 1 ) пс2 X io [ In ( 1.123 ) -In ( 1- ( ) ] do ( 13.75 ) ωα € It is worth while right here to point out that the argument of ...
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... limit qa < 1 holds , and a region of wider angles where the limit qa > 1 applies . For qa 1 , the arguments of exponents in ( 14.111 ) are all so small that the exponential factors can be approximated by unity . Then the differential ...
... limit qa < 1 holds , and a region of wider angles where the limit qa > 1 applies . For qa 1 , the arguments of exponents in ( 14.111 ) are all so small that the exponential factors can be approximated by unity . Then the differential ...
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... limit . The constant value is the semi- classical result . The curve marked " Bethe - Heitler " is the quantum- mechanical Born approximation . For extremely relativistic particles the screening can be " complete . " Complete screening ...
... limit . The constant value is the semi- classical result . The curve marked " Bethe - Heitler " is the quantum- mechanical Born approximation . For extremely relativistic particles the screening can be " complete . " Complete screening ...
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Greens theorem | 14 |
BoundaryValue Problems in Electrostatics I | 26 |
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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 classical coefficients collisions component conducting conductor constant coordinate cross section cylinder d³x dielectric diffraction dimensions dipole direction discussed E₁ effects electric field electromagnetic fields electrons electrostatic energy loss energy transfer factor force equation formula frequency given Green's function impact parameter incident particle integral Kirchhoff Lorentz invariant Lorentz transformation magnetic field magnetic induction magnitude Maxwell's equations meson modes momentum motion multipole nonrelativistic obtain oscillations P₁ parallel perpendicular plane wave plasma plasma oscillations polarization power radiated Poynting's vector problem propagation quantum quantum-mechanical radius region relativistic result 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