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Geant4/processes/hadronic/models/binary_cascade/src/G4KM_OpticalEqRhs.cc

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 27 // -------------------------------------------------------------------
 28 //      GEANT 4 class implementation file 
 29 //
 30 //      CERN, Geneva, Switzerland
 31 //
 32 //      File name:     G4KM_OpticalEqRhs.cc
 33 //
 34 //      Author:        Alessandro Brunengo (Alessandro.Brunengo@ge.infn.it)
 35 // 
 36 //      Creation date: 5 June 2000
 37 // -------------------------------------------------------------------
 38 
 39 #include "G4KM_OpticalEqRhs.hh"
 40 #include "G4PhysicalConstants.hh"
 41 #include "G4NucleiProperties.hh"
 42 #include "G4VNuclearDensity.hh"
 43 #include "G4HadTmpUtil.hh"
 44 
 45 G4KM_OpticalEqRhs::G4KM_OpticalEqRhs(G4KM_DummyField *field,
 46              G4V3DNucleus * nucleus) :
 47   G4Mag_EqRhs(field), theNucleus(nucleus)
 48 {
 49   theFactor = 0;
 50   theMass = 0;
 51 }
 52 
 53 
 54 void G4KM_OpticalEqRhs::SetFactor(G4double mass, G4double opticalParameter)
 55 {
 56   G4double A = theNucleus->GetMassNumber();
 57   G4double Z = theNucleus->GetCharge();
 58   G4double bindingEnergy = G4NucleiProperties::GetBindingEnergy(G4lrint(A), G4lrint(Z));
 59   G4double nucleusMass = Z*proton_mass_c2+(A-Z)*neutron_mass_c2+bindingEnergy;
 60   G4double reducedMass = mass*nucleusMass/(mass+nucleusMass);
 61 
 62   G4double nucleonMass = (proton_mass_c2+neutron_mass_c2)/2;
 63 
 64 // _factor in (MeV*fermi)*fermi/MeV = fermi*fermi  -- need to have A as density normalized to 1
 65   theFactor = 2*pi*hbarc*hbarc*(1+mass/nucleonMass)* opticalParameter/reducedMass * A;
 66 
 67   theMass = mass;
 68 }
 69 
 70 
 71 void G4KM_OpticalEqRhs::EvaluateRhsGivenB(const G4double y[], const G4double *,
 72             G4double dydx[]) const
 73 {
 74   G4double yMod = std::sqrt(y[0]*y[0]+y[1]*y[1]+y[2]*y[2]);
 75   G4double e = std::sqrt(theMass*theMass+y[3]*y[3]+y[4]*y[4]+y[5]*y[5]);
 76   dydx[0] = c_light*y[3]/e;   //
 77   dydx[1] = c_light*y[4]/e;   //  dq/dt=dH/dp = c*p/e
 78   dydx[2] = c_light*y[5]/e;   // 
 79 
 80 // V=K*rho(r) ==> dydx[3] = -dV/dr*dr/dx = -K*d(rho)/dr*dr/dx.
 81 // Idem for dydx[4] and dydx[5]
 82 
 83   const G4VNuclearDensity * nuclearDensity=theNucleus->GetNuclearDensity();
 84 
 85   G4ThreeVector pos(y[0],y[1],y[2]);
 86   G4double deriv = theFactor*nuclearDensity->GetDeriv(pos);
 87 
 88   dydx[3] = yMod == 0 ? 0 : -deriv*y[0]/yMod*c_light;
 89   dydx[4] = yMod == 0 ? 0 : -deriv*y[1]/yMod*c_light;
 90   dydx[5] = yMod == 0 ? 0 : -deriv*y[2]/yMod*c_light;
 91 }
 92 
 93 // Here by design, but it is unnecessary for nuclear fields
 94 void G4KM_OpticalEqRhs::SetChargeMomentumMass(G4ChargeState,G4double ,G4double )
 95 { 
 96 }
 97