| 1 | //
|
|---|
| 2 | // ********************************************************************
|
|---|
| 3 | // * License and Disclaimer *
|
|---|
| 4 | // * *
|
|---|
| 5 | // * The Geant4 software is copyright of the Copyright Holders of *
|
|---|
| 6 | // * the Geant4 Collaboration. It is provided under the terms and *
|
|---|
| 7 | // * conditions of the Geant4 Software License, included in the file *
|
|---|
| 8 | // * LICENSE and available at http://cern.ch/geant4/license . These *
|
|---|
| 9 | // * include a list of copyright holders. *
|
|---|
| 10 | // * *
|
|---|
| 11 | // * Neither the authors of this software system, nor their employing *
|
|---|
| 12 | // * institutes,nor the agencies providing financial support for this *
|
|---|
| 13 | // * work make any representation or warranty, express or implied, *
|
|---|
| 14 | // * regarding this software system or assume any liability for its *
|
|---|
| 15 | // * use. Please see the license in the file LICENSE and URL above *
|
|---|
| 16 | // * for the full disclaimer and the limitation of liability. *
|
|---|
| 17 | // * *
|
|---|
| 18 | // * This code implementation is the result of the scientific and *
|
|---|
| 19 | // * technical work of the GEANT4 collaboration. *
|
|---|
| 20 | // * By using, copying, modifying or distributing the software (or *
|
|---|
| 21 | // * any work based on the software) you agree to acknowledge its *
|
|---|
| 22 | // * use in resulting scientific publications, and indicate your *
|
|---|
| 23 | // * acceptance of all terms of the Geant4 Software license. *
|
|---|
| 24 | // ********************************************************************
|
|---|
| 25 | //
|
|---|
| 26 | // Implementation of formulas in analogy to NASA technical paper 3621 by
|
|---|
| 27 | // Tripathi, et al.
|
|---|
| 28 | //
|
|---|
| 29 | // 26-Dec-2006 Isotope dependence added by D. Wright
|
|---|
| 30 | //
|
|---|
| 31 |
|
|---|
| 32 | #include "G4TripathiCrossSection.hh"
|
|---|
| 33 | #include "G4ParticleTable.hh"
|
|---|
| 34 | #include "G4IonTable.hh"
|
|---|
| 35 | #include "G4HadTmpUtil.hh"
|
|---|
| 36 |
|
|---|
| 37 | G4TripathiCrossSection::G4TripathiCrossSection()
|
|---|
| 38 | {
|
|---|
| 39 | // G4cout <<"New G4TripathiCrossSection " << this << G4endl;
|
|---|
| 40 | }
|
|---|
| 41 | G4TripathiCrossSection::~G4TripathiCrossSection()
|
|---|
| 42 | {}
|
|---|
| 43 |
|
|---|
| 44 | G4double G4TripathiCrossSection::
|
|---|
| 45 | GetIsoZACrossSection(const G4DynamicParticle* aPart, G4double ZZ, G4double AA,
|
|---|
| 46 | G4double /*temperature*/)
|
|---|
| 47 | {
|
|---|
| 48 | G4double result = 0.;
|
|---|
| 49 |
|
|---|
| 50 | const G4double targetAtomicNumber = AA;
|
|---|
| 51 | const G4double nTargetProtons = ZZ;
|
|---|
| 52 |
|
|---|
| 53 | const G4double kineticEnergy = aPart->GetKineticEnergy()/MeV;
|
|---|
| 54 | const G4double nProjProtons = aPart->GetDefinition()->GetPDGCharge();
|
|---|
| 55 | const G4double projectileAtomicNumber =
|
|---|
| 56 | aPart->GetDefinition()->GetBaryonNumber();
|
|---|
| 57 |
|
|---|
| 58 | const G4double nuleonRadius=1.1E-15;
|
|---|
| 59 | const G4double myNuleonRadius=1.36E-15;
|
|---|
| 60 |
|
|---|
| 61 | // needs target mass
|
|---|
| 62 | G4double targetMass =
|
|---|
| 63 | G4ParticleTable::GetParticleTable()->GetIonTable()
|
|---|
| 64 | ->GetIonMass(G4lrint(nTargetProtons), G4lrint(targetAtomicNumber));
|
|---|
| 65 | G4LorentzVector pTarget(0,0,0,targetMass);
|
|---|
| 66 | G4LorentzVector pProjectile(aPart->Get4Momentum());
|
|---|
| 67 | pTarget = pTarget+pProjectile;
|
|---|
| 68 | G4double E_cm = (pTarget.mag()-targetMass-pProjectile.m())/MeV;
|
|---|
| 69 | if(E_cm <= DBL_MIN) return result;
|
|---|
| 70 | // done
|
|---|
| 71 | G4double r_rms_p = 0.6 * myNuleonRadius *
|
|---|
| 72 | std::pow(projectileAtomicNumber, 1./3.);
|
|---|
| 73 | G4double r_rms_t = 0.6 * myNuleonRadius *
|
|---|
| 74 | std::pow(targetAtomicNumber, 1./3.);
|
|---|
| 75 |
|
|---|
| 76 | // done
|
|---|
| 77 | G4double r_p = 1.29*r_rms_p/nuleonRadius ;
|
|---|
| 78 | G4double r_t = 1.29*r_rms_t/nuleonRadius;
|
|---|
| 79 |
|
|---|
| 80 | // done
|
|---|
| 81 | G4double Radius = r_p + r_t +
|
|---|
| 82 | 1.2*(std::pow(targetAtomicNumber, 1./3.) +
|
|---|
| 83 | std::pow(projectileAtomicNumber, 1./3.))/std::pow(E_cm, 1./3.);
|
|---|
| 84 |
|
|---|
| 85 | //done
|
|---|
| 86 | G4double B = 1.44*nProjProtons*nTargetProtons/Radius;
|
|---|
| 87 | if(E_cm <= B) return result;
|
|---|
| 88 | // done
|
|---|
| 89 | G4double Energy = kineticEnergy/projectileAtomicNumber;
|
|---|
| 90 |
|
|---|
| 91 | // done
|
|---|
| 92 | //
|
|---|
| 93 | // Note that this correction to G4TripathiCrossSection is just to accurately
|
|---|
| 94 | // reflect Tripathi's algorithm. However, if you're using alpha
|
|---|
| 95 | // particles/protons consider using the more accurate
|
|---|
| 96 | // G4TripathiLightCrossSection, which Tripathi developed specifically for
|
|---|
| 97 | // light systems.
|
|---|
| 98 | //
|
|---|
| 99 |
|
|---|
| 100 | G4double D;
|
|---|
| 101 | if (nProjProtons==1 && projectileAtomicNumber==1)
|
|---|
| 102 | {
|
|---|
| 103 | D = 2.05;
|
|---|
| 104 | }
|
|---|
| 105 | else if (nProjProtons==2 && projectileAtomicNumber==4)
|
|---|
| 106 | {
|
|---|
| 107 | D = 2.77-(8.0E-3*targetAtomicNumber)+
|
|---|
| 108 | (1.8E-5*targetAtomicNumber*targetAtomicNumber)
|
|---|
| 109 | - 0.8/(1+std::exp((250.-Energy)/75.));
|
|---|
| 110 | }
|
|---|
| 111 | else
|
|---|
| 112 | {
|
|---|
| 113 | //
|
|---|
| 114 | // This is the original value used in the G4TripathiCrossSection
|
|---|
| 115 | // implementation, and was used for all projectile/target conditions.
|
|---|
| 116 | // I'm not touching this, although judging from Tripathi's paper, this is
|
|---|
| 117 | // valid for cases where the nucleon density changes little with A.
|
|---|
| 118 | //
|
|---|
| 119 | D = 1.75;
|
|---|
| 120 | }
|
|---|
| 121 | // done
|
|---|
| 122 | G4double C_E = D * (1-std::exp(-Energy/40.)) -
|
|---|
| 123 | 0.292*std::exp(-Energy/792.)*std::cos(0.229*std::pow(Energy, 0.453));
|
|---|
| 124 |
|
|---|
| 125 | // done
|
|---|
| 126 | G4double S = std::pow(projectileAtomicNumber, 1./3.)*
|
|---|
| 127 | std::pow(targetAtomicNumber, 1./3.)/
|
|---|
| 128 | (std::pow(projectileAtomicNumber, 1./3.) +
|
|---|
| 129 | std::pow(targetAtomicNumber, 1./3.));
|
|---|
| 130 |
|
|---|
| 131 | // done
|
|---|
| 132 | G4double deltaE = 1.85*S + 0.16*S/std::pow(E_cm,1./3.) - C_E +
|
|---|
| 133 | 0.91*(targetAtomicNumber-2.*nTargetProtons)*nProjProtons/
|
|---|
| 134 | (targetAtomicNumber*projectileAtomicNumber);
|
|---|
| 135 |
|
|---|
| 136 | // done
|
|---|
| 137 | result = pi * nuleonRadius*nuleonRadius *
|
|---|
| 138 | std::pow(( std::pow(targetAtomicNumber, 1./3.) +
|
|---|
| 139 | std::pow(projectileAtomicNumber, 1./3.) + deltaE),2.) *
|
|---|
| 140 | (1-B/E_cm);
|
|---|
| 141 |
|
|---|
| 142 | if(result < 0.) result = 0.;
|
|---|
| 143 | return result*m2;
|
|---|
| 144 |
|
|---|
| 145 | }
|
|---|
| 146 |
|
|---|
| 147 |
|
|---|
| 148 | G4double G4TripathiCrossSection::
|
|---|
| 149 | GetCrossSection(const G4DynamicParticle* aPart, const G4Element* anEle,
|
|---|
| 150 | G4double temperature)
|
|---|
| 151 | {
|
|---|
| 152 | G4int nIso = anEle->GetNumberOfIsotopes();
|
|---|
| 153 | G4double xsection = 0;
|
|---|
| 154 |
|
|---|
| 155 | if (nIso) {
|
|---|
| 156 | G4double sig;
|
|---|
| 157 | G4IsotopeVector* isoVector = anEle->GetIsotopeVector();
|
|---|
| 158 | G4double* abundVector = anEle->GetRelativeAbundanceVector();
|
|---|
| 159 | G4double ZZ;
|
|---|
| 160 | G4double AA;
|
|---|
| 161 |
|
|---|
| 162 | for (G4int i = 0; i < nIso; i++) {
|
|---|
| 163 | ZZ = G4double( (*isoVector)[i]->GetZ() );
|
|---|
| 164 | AA = G4double( (*isoVector)[i]->GetN() );
|
|---|
| 165 | sig = GetIsoZACrossSection(aPart, ZZ, AA, temperature);
|
|---|
| 166 | xsection += sig*abundVector[i];
|
|---|
| 167 | }
|
|---|
| 168 |
|
|---|
| 169 | } else {
|
|---|
| 170 | xsection =
|
|---|
| 171 | GetIsoZACrossSection(aPart, anEle->GetZ(), anEle->GetN(),
|
|---|
| 172 | temperature);
|
|---|
| 173 | }
|
|---|
| 174 |
|
|---|
| 175 | return xsection;
|
|---|
| 176 | }
|
|---|