| [819] | 1 | //
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| 2 | // ********************************************************************
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| 3 | // * License and Disclaimer *
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| 4 | // * *
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| 5 | // * The Geant4 software is copyright of the Copyright Holders of *
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| 6 | // * the Geant4 Collaboration. It is provided under the terms and *
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| 7 | // * conditions of the Geant4 Software License, included in the file *
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| 8 | // * LICENSE and available at http://cern.ch/geant4/license . These *
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| 9 | // * include a list of copyright holders. *
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| 10 | // * *
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| 11 | // * Neither the authors of this software system, nor their employing *
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| 12 | // * institutes,nor the agencies providing financial support for this *
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| 13 | // * work make any representation or warranty, express or implied, *
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| 14 | // * regarding this software system or assume any liability for its *
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| 15 | // * use. Please see the license in the file LICENSE and URL above *
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| 16 | // * for the full disclaimer and the limitation of liability. *
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| 17 | // * *
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| 18 | // * This code implementation is the result of the scientific and *
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| 19 | // * technical work of the GEANT4 collaboration. *
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| 20 | // * By using, copying, modifying or distributing the software (or *
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| 21 | // * any work based on the software) you agree to acknowledge its *
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| 22 | // * use in resulting scientific publications, and indicate your *
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| 23 | // * acceptance of all terms of the Geant4 Software license. *
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| 24 | // ********************************************************************
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| 25 | //
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| 26 | //
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| [1196] | 27 | // $Id: G4RToEConvForGamma.cc,v 1.6 2009/09/12 12:09:42 kurasige Exp $
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| [1228] | 28 | // GEANT4 tag $Name: geant4-09-03 $
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| [819] | 29 | //
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| 30 | //
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| 31 | // --------------------------------------------------------------
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| 32 | // GEANT 4 class implementation file/ History:
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| 33 | // 5 Oct. 2002, H.Kuirashige : Structure created based on object model
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| 34 | // --------------------------------------------------------------
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| 35 |
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| 36 | #include "G4RToEConvForGamma.hh"
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| 37 | #include "G4ParticleDefinition.hh"
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| 38 | #include "G4ParticleTable.hh"
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| 39 | #include "G4Material.hh"
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| 40 | #include "G4PhysicsLogVector.hh"
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| 41 |
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| 42 | #include "G4ios.hh"
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| 43 |
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| 44 | G4RToEConvForGamma::G4RToEConvForGamma() : G4VRangeToEnergyConverter()
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| 45 | {
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| 46 | theParticle = G4ParticleTable::GetParticleTable()->FindParticle("gamma");
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| 47 | if (theParticle ==0) {
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| 48 | #ifdef G4VERBOSE
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| 49 | if (GetVerboseLevel()>0) {
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| 50 | G4cout << " G4RToEConvForGamma::G4RToEConvForGamma() ";
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| 51 | G4cout << " Gamma is not defined !!" << G4endl;
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| 52 | }
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| 53 | #endif
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| 54 | }
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| 55 | }
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| 56 |
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| 57 | G4RToEConvForGamma::~G4RToEConvForGamma()
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| 58 | {
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| 59 | }
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| 60 |
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| 61 |
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| 62 | // ***********************************************************************
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| 63 | // ******************* BuildAbsorptionLengthVector ***********************
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| 64 | // ***********************************************************************
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| 65 | void G4RToEConvForGamma::BuildAbsorptionLengthVector(
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| 66 | const G4Material* aMaterial,
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| 67 | G4RangeVector* absorptionLengthVector )
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| 68 | {
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| 69 | // fill the absorption length vector for this material
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| 70 | // absorption length is defined here as
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| 71 | //
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| 72 | // absorption length = 5./ macroscopic absorption cross section
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| 73 | //
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| 74 | const G4CrossSectionTable* aCrossSectionTable = (G4CrossSectionTable*)(theLossTable);
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| 75 | const G4ElementVector* elementVector = aMaterial->GetElementVector();
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| 76 | const G4double* atomicNumDensityVector = aMaterial->GetAtomicNumDensityVector();
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| 77 |
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| 78 | // fill absorption length vector
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| 79 | G4int NumEl = aMaterial->GetNumberOfElements();
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| 80 | G4double absorptionLengthMax = 0.0;
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| [1196] | 81 | G4double previous = 0.;
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| [819] | 82 | for (size_t ibin=0; ibin<size_t(TotBin); ibin++) {
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| 83 | G4double SIGMA = 0. ;
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| 84 | for (size_t iel=0; iel<size_t(NumEl); iel++) {
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| 85 | G4int IndEl = (*elementVector)[iel]->GetIndex();
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| 86 | SIGMA += atomicNumDensityVector[iel]*
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| [1196] | 87 | (*((*aCrossSectionTable)[IndEl]))[ibin];
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| [819] | 88 | }
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| 89 | // absorption length=5./SIGMA
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| 90 | absorptionLengthVector->PutValue(ibin, 5./SIGMA);
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| 91 | if (absorptionLengthMax < 5./SIGMA ) absorptionLengthMax = 5./SIGMA;
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| [1196] | 92 |
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| 93 | //if (previous > 5./SIGMA) {
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| 94 | // G4cout << "G4RToEConvForGamma::BuildAbsorptionLengthVector"
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| 95 | // << ": WARNING absorptionVector "
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| 96 | // << ibin << ":" << 5./SIGMA << " <-- "
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| 97 | // << ibin -1 << ":" << previous <<G4endl;
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| 98 | //}
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| 99 |
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| 100 | previous = 5./SIGMA;
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| [819] | 101 | }
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| 102 | }
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| 103 |
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| 104 |
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| 105 |
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| 106 | // ***********************************************************************
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| 107 | // ********************** ComputeCrossSection ****************************
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| 108 | // ***********************************************************************
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| 109 | G4double G4RToEConvForGamma::ComputeCrossSection(G4double AtomicNumber,
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| 110 | G4double KineticEnergy) const
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| 111 | {
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| 112 | // Compute the "absorption" cross section of the photon "absorption"
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| 113 | // cross section means here the sum of the cross sections of the
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| 114 | // pair production, Compton scattering and photoelectric processes
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| 115 | static G4double Z;
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| 116 | const G4double t1keV = 1.*keV;
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| 117 | const G4double t200keV = 200.*keV;
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| 118 | const G4double t100MeV = 100.*MeV;
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| 119 |
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| 120 | static G4double s200keV, s1keV;
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| 121 | static G4double tmin, tlow;
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| 122 | static G4double smin, slow;
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| 123 | static G4double cmin, clow, chigh;
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| 124 | // compute Z dependent quantities in the case of a new AtomicNumber
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| 125 | if(std::abs(AtomicNumber-Z)>0.1) {
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| 126 | Z = AtomicNumber;
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| 127 | G4double Zsquare = Z*Z;
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| 128 | G4double Zlog = std::log(Z);
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| 129 | G4double Zlogsquare = Zlog*Zlog;
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| 130 |
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| 131 | s200keV = (0.2651-0.1501*Zlog+0.02283*Zlogsquare)*Zsquare;
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| 132 | tmin = (0.552+218.5/Z+557.17/Zsquare)*MeV;
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| 133 | smin = (0.01239+0.005585*Zlog-0.000923*Zlogsquare)*std::exp(1.5*Zlog);
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| 134 | cmin=std::log(s200keV/smin)/(std::log(tmin/t200keV)*std::log(tmin/t200keV));
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| 135 | tlow = 0.2*std::exp(-7.355/std::sqrt(Z))*MeV;
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| 136 | slow = s200keV*std::exp(0.042*Z*std::log(t200keV/tlow)*std::log(t200keV/tlow));
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| 137 | s1keV = 300.*Zsquare;
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| 138 | clow =std::log(s1keV/slow)/std::log(tlow/t1keV);
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| 139 |
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| 140 | chigh=(7.55e-5-0.0542e-5*Z)*Zsquare*Z/std::log(t100MeV/tmin);
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| 141 | }
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| 142 |
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| 143 | // calculate the cross section (using an approximate empirical formula)
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| 144 | G4double s;
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| 145 | if ( KineticEnergy<tlow ) {
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| 146 | if(KineticEnergy<t1keV) s = slow*std::exp(clow*std::log(tlow/t1keV));
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| 147 | else s = slow*std::exp(clow*std::log(tlow/KineticEnergy));
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| 148 |
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| 149 | } else if ( KineticEnergy<t200keV ) {
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| 150 | s = s200keV
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| 151 | * std::exp(0.042*Z*std::log(t200keV/KineticEnergy)*std::log(t200keV/KineticEnergy));
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| 152 |
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| 153 | } else if( KineticEnergy<tmin ){
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| 154 | s = smin
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| 155 | * std::exp(cmin*std::log(tmin/KineticEnergy)*std::log(tmin/KineticEnergy));
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| 156 |
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| 157 | } else {
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| 158 | s = smin + chigh*std::log(KineticEnergy/tmin);
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| 159 |
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| 160 | }
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| 161 | return s * barn;
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| 162 | }
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| 163 |
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