source: trunk/source/processes/hadronic/models/binary_cascade/src/G4KM_OpticalEqRhs.cc @ 1347

Last change on this file since 1347 was 962, checked in by garnier, 15 years ago

update processes

File size: 3.7 KB
Line 
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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 "G4NucleiProperties.hh"
41#include "G4VNuclearDensity.hh"
42#include "G4HadTmpUtil.hh"
43
44
45G4KM_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
54void 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
71void 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
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