source: trunk/source/processes/hadronic/cross_sections/src/G4IonsShenCrossSection.cc@ 1315

Last change on this file since 1315 was 1055, checked in by garnier, 17 years ago

maj sur la beta de geant 4.9.3

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[819]1//
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25//
26// 18-Sep-2003 First version is written by T. Koi
27// 12-Nov-2003 Add energy check at lower side T. Koi
28// 15-Nov-2006 Above 10GeV/n Cross Section become constant T. Koi (SLAC/SCCS)
29// 23-Dec-2006 Isotope dependence adde by D. Wright
30//
31
32#include "G4IonsShenCrossSection.hh"
33#include "G4ParticleTable.hh"
34#include "G4IonTable.hh"
35
36
37G4double G4IonsShenCrossSection::
38GetIsoZACrossSection(const G4DynamicParticle* aParticle, G4double ZZ,
39 G4double AA, G4double /*temperature*/)
40{
41 G4double xsection = 0.0;
42
43 G4int Ap = aParticle->GetDefinition()->GetBaryonNumber();
44 G4int Zp = int ( aParticle->GetDefinition()->GetPDGCharge() / eplus + 0.5 );
45 G4double ke_per_N = aParticle->GetKineticEnergy() / Ap;
46 if ( ke_per_N > 10*GeV ) ke_per_N = 10*GeV;
47
48// Apply energy check, if less than lower limit then 0 value is returned
[1055]49 // if ( ke_per_N < lowerLimit ) return xsection;
[819]50
51 G4int At = G4int(AA);
52 G4int Zt = G4int(ZZ);
53
54 G4double one_third = 1.0 / 3.0;
55
56 G4double cubicrAt = std::pow ( G4double(At) , G4double(one_third) );
57 G4double cubicrAp = std::pow ( G4double(Ap) , G4double(one_third) );
58
59 G4double Rt = 1.12 * cubicrAt - 0.94 * ( 1.0 / cubicrAt );
60 G4double Rp = 1.12 * cubicrAp - 0.94 * ( 1.0 / cubicrAp );
61
62 G4double r = Rt + Rp + 3.2; // in fm
63 G4double b = 1.0; // in MeV/fm
[1055]64 G4double targ_mass = G4ParticleTable::GetParticleTable()->GetIonTable()->GetIonMass( Zt , At );
65 G4double proj_mass = aParticle->GetMass();
66 G4double proj_momentum = aParticle->GetMomentum().mag();
[819]67
[1055]68 G4double Ecm = calEcmValue ( proj_mass , targ_mass , proj_momentum );
69
[819]70 G4double B = 1.44 * Zt * Zp / r - b * Rt * Rp / ( Rt + Rp );
[1055]71 if(Ecm <= B) return xsection;
[819]72 //G4double ke_per_N = aParticle->GetKineticEnergy() / Ap;
73
74 G4double c = calCeValue ( ke_per_N / MeV );
75
76 G4double R1 = r0 * ( cubicrAt + cubicrAp + 1.85 * cubicrAt * cubicrAp / ( cubicrAt + cubicrAp ) - c);
77
78 G4double R2 = 1.0 * ( At - 2 * Zt ) * Zp / ( Ap * At );
79
80
81 G4double R3 = 0.176 / std::pow ( G4double(Ecm) , G4double(one_third) ) * cubicrAt * cubicrAp / ( cubicrAt + cubicrAp );
82
83 G4double R = R1 + R2 + R3;
84
85 xsection = 10 * pi * R * R * ( 1 - B / Ecm );
86 xsection = xsection * millibarn; // mulitply xsection by millibarn
87
88 return xsection;
89}
90
91
92G4double G4IonsShenCrossSection::
93GetCrossSection(const G4DynamicParticle* aParticle, const G4Element* anElement,
94 G4double temperature)
95{
96 G4int nIso = anElement->GetNumberOfIsotopes();
97 G4double xsection = 0;
98
99 if (nIso) {
100 G4double sig;
101 G4IsotopeVector* isoVector = anElement->GetIsotopeVector();
102 G4double* abundVector = anElement->GetRelativeAbundanceVector();
103 G4double ZZ;
104 G4double AA;
105
106 for (G4int i = 0; i < nIso; i++) {
107 ZZ = G4double( (*isoVector)[i]->GetZ() );
108 AA = G4double( (*isoVector)[i]->GetN() );
109 sig = GetIsoZACrossSection(aParticle, ZZ, AA, temperature);
110 xsection += sig*abundVector[i];
111 }
112
113 } else {
114 xsection =
115 GetIsoZACrossSection(aParticle, anElement->GetZ(), anElement->GetN(),
116 temperature);
117 }
118
119 return xsection;
120}
121
122
123G4double G4IonsShenCrossSection::calEcmValue( const G4double mp , const G4double mt , const G4double Plab )
124{
125 G4double Elab = std::sqrt ( mp * mp + Plab * Plab );
126 G4double Ecm = std::sqrt ( mp * mp + mt * mt + 2 * Elab * mt );
127 G4double Pcm = Plab * mt / Ecm;
128 G4double KEcm = std::sqrt ( Pcm * Pcm + mp * mp ) - mp;
129 return KEcm;
130}
131
132
133G4double G4IonsShenCrossSection::calCeValue( const G4double ke )
134{
135 // Calculate c value
136 // This value is indepenent from projectile and target particle
137 // ke is projectile kinetic energy per nucleon in the Lab system with MeV unit
138 // fitting function is made by T. Koi
139 // There are no data below 30 MeV/n in Kox et al.,
140
141 G4double Ce;
142 G4double log10_ke = std::log10 ( ke );
143 if ( log10_ke > 1.5 )
144 {
145 Ce = - 10.0 / std::pow ( G4double(log10_ke) , G4double(5) ) + 2.0;
146 }
147 else
148 {
149 Ce = ( - 10.0 / std::pow ( G4double(1.5) , G4double(5) ) + 2.0 ) / std::pow ( G4double(1.5) , G4double(3) ) * std::pow ( G4double(log10_ke) , G4double(3) );
150 }
151 return Ce;
152}
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