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Please see the license in the file LICENSE and URL above * 16 // * for the full disclaimer and the limitatio 16 // * for the full disclaimer and the limitation of liability. * 17 // * 17 // * * 18 // * This code implementation is the result 18 // * This code implementation is the result of the scientific and * 19 // * technical work of the GEANT4 collaboratio 19 // * technical work of the GEANT4 collaboration. * 20 // * By using, copying, modifying or distri 20 // * By using, copying, modifying or distributing the software (or * 21 // * any work based on the software) you ag 21 // * any work based on the software) you agree to acknowledge its * 22 // * use in resulting scientific publicati 22 // * use in resulting scientific publications, and indicate your * 23 // * acceptance of all terms of the Geant4 Sof 23 // * acceptance of all terms of the Geant4 Software license. * 24 // ******************************************* 24 // ******************************************************************** 25 // 25 // 26 // G4RToEConvForGamma class implementation << 27 // 26 // 28 // Author: H.Kurashige, 05 October 2002 - Firs << 27 // $Id: G4RToEConvForGamma.cc 70745 2013-06-05 10:54:00Z gcosmo $ 29 // ------------------------------------------- << 28 // >> 29 // >> 30 // -------------------------------------------------------------- >> 31 // GEANT 4 class implementation file/ History: >> 32 // 5 Oct. 2002, H.Kuirashige : Structure created based on object model >> 33 // -------------------------------------------------------------- 30 34 31 #include "G4RToEConvForGamma.hh" 35 #include "G4RToEConvForGamma.hh" 32 #include "G4ParticleDefinition.hh" 36 #include "G4ParticleDefinition.hh" 33 #include "G4ParticleTable.hh" 37 #include "G4ParticleTable.hh" >> 38 #include "G4Material.hh" >> 39 #include "G4PhysicsLogVector.hh" >> 40 >> 41 #include "G4ios.hh" 34 #include "G4SystemOfUnits.hh" 42 #include "G4SystemOfUnits.hh" 35 #include "G4Log.hh" << 36 #include "G4Exp.hh" << 37 #include "G4Pow.hh" << 38 43 39 // ------------------------------------------- << 40 G4RToEConvForGamma::G4RToEConvForGamma() 44 G4RToEConvForGamma::G4RToEConvForGamma() 41 : G4VRangeToEnergyConverter() << 45 : G4VRangeToEnergyConverter(), >> 46 Z(-1), >> 47 s200keV(0.), s1keV(0.), >> 48 tmin(0.), tlow(0.), >> 49 smin(0.), slow(0.), >> 50 cmin(0.), clow(0.), chigh(0.) 42 { 51 { 43 theParticle = G4ParticleTable::GetParticleTa << 52 theParticle = G4ParticleTable::GetParticleTable()->FindParticle("gamma"); 44 if (theParticle == nullptr) << 53 if (theParticle ==0) { 45 { << 46 #ifdef G4VERBOSE 54 #ifdef G4VERBOSE 47 if (GetVerboseLevel()>0) << 55 if (GetVerboseLevel()>0) { 48 { << 56 G4cout << " G4RToEConvForGamma::G4RToEConvForGamma() "; 49 G4cout << " G4RToEConvForGamma::G4RToECo << 57 G4cout << " Gamma is not defined !!" << G4endl; 50 G4cout << "Gamma is not defined !!" << G << 51 } 58 } 52 #endif 59 #endif 53 } 60 } 54 else << 61 } 55 { << 62 56 fPDG = theParticle->GetPDGEncoding(); << 63 G4RToEConvForGamma::~G4RToEConvForGamma() >> 64 { >> 65 } >> 66 >> 67 >> 68 // *********************************************************************** >> 69 // ******************* BuildAbsorptionLengthVector *********************** >> 70 // *********************************************************************** >> 71 void G4RToEConvForGamma::BuildAbsorptionLengthVector( >> 72 const G4Material* aMaterial, >> 73 G4RangeVector* absorptionLengthVector ) >> 74 { >> 75 // fill the absorption length vector for this material >> 76 // absorption length is defined here as >> 77 // >> 78 // absorption length = 5./ macroscopic absorption cross section >> 79 // >> 80 const G4CrossSectionTable* aCrossSectionTable = (G4CrossSectionTable*)(theLossTable); >> 81 const G4ElementVector* elementVector = aMaterial->GetElementVector(); >> 82 const G4double* atomicNumDensityVector = aMaterial->GetAtomicNumDensityVector(); >> 83 >> 84 // fill absorption length vector >> 85 G4int NumEl = aMaterial->GetNumberOfElements(); >> 86 G4double absorptionLengthMax = 0.0; >> 87 for (size_t ibin=0; ibin<size_t(TotBin); ibin++) { >> 88 G4double SIGMA = 0. ; >> 89 for (size_t iel=0; iel<size_t(NumEl); iel++) { >> 90 G4int IndEl = (*elementVector)[iel]->GetIndex(); >> 91 SIGMA += atomicNumDensityVector[iel]* >> 92 (*((*aCrossSectionTable)[IndEl]))[ibin]; >> 93 } >> 94 // absorption length=5./SIGMA >> 95 absorptionLengthVector->PutValue(ibin, 5./SIGMA); >> 96 if (absorptionLengthMax < 5./SIGMA ) absorptionLengthMax = 5./SIGMA; 57 } 97 } 58 } 98 } 59 99 60 // ------------------------------------------- << 100 61 G4RToEConvForGamma::~G4RToEConvForGamma() << 101 62 {} << 102 // *********************************************************************** 63 << 103 // ********************** ComputeCrossSection **************************** 64 // ------------------------------------------- << 104 // *********************************************************************** 65 G4double G4RToEConvForGamma::ComputeValue(cons << 105 G4double G4RToEConvForGamma::ComputeCrossSection(G4double AtomicNumber, 66 cons << 106 G4double KineticEnergy) 67 { 107 { 68 // Compute the "absorption" cross-section of << 108 // Compute the "absorption" cross section of the photon "absorption" 69 // Cross-section means here the sum of the c << 109 // cross section means here the sum of the cross sections of the 70 // pair production, Compton scattering and p << 110 // pair production, Compton scattering and photoelectric processes 71 << 111 const G4double t1keV = 1.*keV; 72 const G4double t1keV = 1.*CLHEP::keV; << 112 const G4double t200keV = 200.*keV; 73 const G4double t200keV = 200.*CLHEP::keV; << 113 const G4double t100MeV = 100.*MeV; 74 const G4double t100MeV = 100.*CLHEP::MeV; << 114 75 << 115 // compute Z dependent quantities in the case of a new AtomicNumber 76 G4double Zsquare = Z*Z; << 116 if(std::abs(AtomicNumber-Z)>0.1) { 77 G4double Zlog = G4Pow::GetInstance()->logZ(Z << 117 Z = AtomicNumber; 78 G4double Zlogsquare = Zlog*Zlog; << 118 G4double Zsquare = Z*Z; 79 << 119 G4double Zlog = std::log(Z); 80 G4double tmin = (0.552+218.5/Z+557.17/Zsquar << 120 G4double Zlogsquare = Zlog*Zlog; 81 G4double tlow = 0.2*G4Exp(-7.355/std::sqrt(Z << 121 82 << 122 s200keV = (0.2651-0.1501*Zlog+0.02283*Zlogsquare)*Zsquare; 83 G4double smin = (0.01239+0.005585*Zlog-0.000 << 123 tmin = (0.552+218.5/Z+557.17/Zsquare)*MeV; 84 G4double s200keV = (0.2651-0.1501*Zlog+0.022 << 124 smin = (0.01239+0.005585*Zlog-0.000923*Zlogsquare)*std::exp(1.5*Zlog); 85 << 125 cmin=std::log(s200keV/smin)/(std::log(tmin/t200keV)*std::log(tmin/t200keV)); 86 G4double cminlog = G4Log(tmin/t200keV); << 126 tlow = 0.2*std::exp(-7.355/std::sqrt(Z))*MeV; 87 G4double cmin = G4Log(s200keV/smin)/(cminlog << 127 slow = s200keV*std::exp(0.042*Z*std::log(t200keV/tlow)*std::log(t200keV/tlow)); 88 << 128 s1keV = 300.*Zsquare; 89 G4double slowlog = G4Log(t200keV/tlow); << 129 clow =std::log(s1keV/slow)/std::log(tlow/t1keV); 90 G4double slow = s200keV * G4Exp(0.042*Z*slow << 91 G4double logtlow = G4Log(tlow/t1keV); << 92 G4double clow = G4Log(300.*Zsquare/slow)/log << 93 G4double chigh = (7.55e-5 - 0.0542e-5*Z)*Zsq << 94 130 95 // Calculate the cross-section (using an app << 131 chigh=(7.55e-5-0.0542e-5*Z)*Zsquare*Z/std::log(t100MeV/tmin); 96 G4double xs; << 97 if ( energy < tlow ) << 98 { << 99 xs = (energy < t1keV) ? slow*G4Exp(clow*lo << 100 slow*G4Exp(clow*G4Log(tlow/energy)); << 101 } << 102 else if ( energy < t200keV ) << 103 { << 104 G4double x = G4Log(t200keV/energy); << 105 xs = s200keV * G4Exp(0.042*Z*x*x); << 106 } << 107 else if( energy<tmin ) << 108 { << 109 const G4double x = G4Log(tmin/energy); << 110 xs = smin * G4Exp(cmin*x*x); << 111 } 132 } 112 else << 133 113 { << 134 // calculate the cross section (using an approximate empirical formula) 114 xs = smin + chigh*G4Log(energy/tmin); << 135 G4double xs; >> 136 if ( KineticEnergy<tlow ) { >> 137 if(KineticEnergy<t1keV) xs = slow*std::exp(clow*std::log(tlow/t1keV)); >> 138 else xs = slow*std::exp(clow*std::log(tlow/KineticEnergy)); >> 139 >> 140 } else if ( KineticEnergy<t200keV ) { >> 141 xs = s200keV >> 142 * std::exp(0.042*Z*std::log(t200keV/KineticEnergy)*std::log(t200keV/KineticEnergy)); >> 143 >> 144 } else if( KineticEnergy<tmin ){ >> 145 xs = smin >> 146 * std::exp(cmin*std::log(tmin/KineticEnergy)*std::log(tmin/KineticEnergy)); >> 147 >> 148 } else { >> 149 xs = smin + chigh*std::log(KineticEnergy/tmin); >> 150 115 } 151 } 116 return xs * CLHEP::barn; << 152 return xs * barn; 117 } 153 } 118 154 119 // ------------------------------------------- << 120 155