Difference between revisions of "Calculation of radiation yield"
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'''Case B:''' For <math>\varepsilon < 0.88</math> we have <math>\psi(\varepsilon) = 19.70 + 4.117(0.88-\varepsilon)-3.806(0.88-\varepsilon)^2 + 31.84(0.88-\varepsilon)^3-58.63(0.88-\varepsilon)^4+40.77(0.88-\varepsilon)^5</math> | '''Case B:''' For <math>\varepsilon < 0.88</math> we have <math>\psi(\varepsilon) = 19.70 + 4.117(0.88-\varepsilon)-3.806(0.88-\varepsilon)^2 + 31.84(0.88-\varepsilon)^3-58.63(0.88-\varepsilon)^4+40.77(0.88-\varepsilon)^5</math> | ||
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Reference: | Reference: | ||
− | [*] J.L. Matthews, R.O. Owens, ''Accurate Formulae For the Calculation of High Energy Electron Bremsstrahlung Spectra'', NIM III (1973) I57-I68 | + | [*] J.L. Matthews, R.O. Owens, ''Accurate Formulae For the Calculation of High Energy Electron Bremsstrahlung Spectra'', NIM III (1973) I57-I68. |
Revision as of 20:58, 8 May 2008
The number of photons per MeV per incident electron per
of radiator (Z,A) is given by [*]:,
where
- photon kinetic energy in MeV;- incident electron total energy (in units of the electron rest mass);
- incident photon energy (in units of the electron rest mass);
;
;
;
;
;
;
;
Case A: For
the screening effect is negligible, (free electron form) and in this case .Case B: For
we have
Reference: [*] J.L. Matthews, R.O. Owens, Accurate Formulae For the Calculation of High Energy Electron Bremsstrahlung Spectra, NIM III (1973) I57-I68.