source: trunk/source/processes/electromagnetic/lowenergy/src/G4PhotoElectricAngularGeneratorSauterGavrila.cc@ 1058

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[819]1//
2// ********************************************************************
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24// ********************************************************************
25//
26//
27// -------------------------------------------------------------------
28//
29// GEANT4 Class file
30//
31//
32// File name: G4PhotoElectricAngularGeneratorSauterGavrila
33//
34// Creation date: 10 May 2004
35//
36// Modifications:
37// 10 May 2003 P. Rodrigues First implementation acording with new design
38//
39// Class Description:
40//
41// Concrete class for PhotoElectric Electron Angular Distribution Generation
42// This model is a re-implementation of the Photolectric angular distribution
43// developed my M. Maire for the Standard EM Physics G4PhotoElectricEffect
44//
45// Class Description: End
46//
47// -------------------------------------------------------------------
48//
49//
50
51#include "G4PhotoElectricAngularGeneratorSauterGavrila.hh"
52#include "Randomize.hh"
53
54//
55
56G4PhotoElectricAngularGeneratorSauterGavrila::G4PhotoElectricAngularGeneratorSauterGavrila(const G4String& name):G4VPhotoElectricAngularDistribution(name)
57{;}
58
59//
60
61G4PhotoElectricAngularGeneratorSauterGavrila::~G4PhotoElectricAngularGeneratorSauterGavrila()
62{;}
63
64//
65
66G4ThreeVector G4PhotoElectricAngularGeneratorSauterGavrila::GetPhotoElectronDirection(const G4ThreeVector& direction, const G4double eKineticEnergy, const G4ThreeVector&, const G4int) const
67{
68
69 // Compute Theta distribution of the emitted electron, with respect to the
70 // incident Gamma.
71 // The Sauter-Gavrila distribution for the K-shell is used. (adapted from G4PhotoElectricEffect)
72
73 G4double costeta = 1.;
74 G4double Phi = twopi * G4UniformRand();
75 G4double cosphi = std::cos(Phi);
76 G4double sinphi = std::sin(Phi);
77 G4double sinteta = 0;
78 G4double gamma = 1. + eKineticEnergy/electron_mass_c2;
79
80 if (gamma > 5.) {
81 G4ThreeVector direction (sinteta*cosphi, sinteta*sinphi, costeta);
82 return costeta;
83 }
84
85 G4double beta = std::sqrt(gamma*gamma-1.)/gamma;
86 G4double b = 0.5*gamma*(gamma-1.)*(gamma-2);
87
88 G4double rndm,term,greject,grejsup;
89 if (gamma < 2.) grejsup = gamma*gamma*(1.+b-beta*b);
90 else grejsup = gamma*gamma*(1.+b+beta*b);
91
92 do { rndm = 1.-2*G4UniformRand();
93 costeta = (rndm+beta)/(rndm*beta+1.);
94 term = 1.-beta*costeta;
95 greject = (1.-costeta*costeta)*(1.+b*term)/(term*term);
96 } while(greject < G4UniformRand()*grejsup);
97
98
99 sinteta = std::sqrt(1.-costeta*costeta);
100 G4ThreeVector photoelectrondirection (sinteta*cosphi, sinteta*sinphi, costeta);
101 photoelectrondirection.rotateUz(direction);
102 return photoelectrondirection;
103}
104
105//
106
107void G4PhotoElectricAngularGeneratorSauterGavrila::PrintGeneratorInformation() const
108{
109 G4cout << "\n" << G4endl;
110 G4cout << "" << G4endl;
111 G4cout << "Re-implementation of the photolectric angular distribution" << G4endl;
112 G4cout << "developed my M. Maire for the Standard EM Physics G4PhotoElectricEffect" << G4endl;
113 G4cout << "It computes the theta distribution of the emitted electron, with respect to the" << G4endl;
114 G4cout << "incident Gamma, using the Sauter-Gavrila distribution for the K-shell\n" << G4endl;
115}
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