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>
  
<math>\gamma(=100k/E_0EZ^{1/3}) \leq 15</math>, <math>k<k_x</math>
+
<math>\gamma(=100k/E_0EZ^{1/3}) \leq 15</math> , <math>k<k_x</math>
  
 
<math>\Phi_n(Z,E_0,k) = \Phi_{CS} (for \gamma \leq 15)</math>
 
<math>\Phi_n(Z,E_0,k) = \Phi_{CS} (for \gamma \leq 15)</math>

Revision as of 19:49, 9 May 2008

The number of photons per MeV per incident electron per g/cm2 of radiator (Z,A) is given by [*]:

d2ndκdt=3.495×104Aκ[Z2Φn(Z,E0,k)+ZΦe(Z,E0,k)](MeV1g1cm2),

where κ - photon kinetic energy in MeV;

E0 - incident electron total energy (in units of the electron rest mass);

k - incident photon energy (in units of the electron rest mass);

Φe(Z,E0,k)=CB{2[12E3E0+(EE)2][Lη]+η[1L22ρ1ρ2(12L[ρ(ρ+2)(E0+1)E01]12)2]};

E=E0k;

ρ=E0k(1+E0E21);

η=ρ/(ρ+2);

L=2ln((E01)12+[η(E0+1)12](E01)12[η(E0+1)12]);

CB=14ψ(ε)1lnZ233.798lnεlnZ23;

ε=100k/E0EZ2/3;

Case A: For ε0.88 the screening effect is negligible, ψ(ε)=19.194lnε (free electron form) and in this case CB=1.

Case B: For ε<0.88 we have ψ(ε)=19.70+4.117(0.88ε)3.806(0.88ε)2+31.84(0.88ε)358.63(0.88ε)4+40.77(0.88ε)5

γ(=100k/E0EZ1/3)15 , k<kx

Φn(Z,E0,k)=ΦCS(forγ15)




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