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> | ||
| + | |||
| + | ---- | ||
Reference: [*] J.L. Matthews, R.O. Owens, ''Accurate Formulae For the Calculation of High Energy Electron Bremsstrahlung Spectra'', NIM III (1973) I57-I68. | Reference: [*] 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 20:59, 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.