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G4hPairProductionModel.cc
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26 // $Id: G4hPairProductionModel.cc 66996 2013-01-29 14:50:52Z gcosmo $
27 //
28 // -------------------------------------------------------------------
29 //
30 // GEANT4 Class file
31 //
32 //
33 // File name: G4hPairProductionModel
34 //
35 // Author: Vladimir Ivanchenko on base of G4MuPairProductionModel
36 //
37 // Creation date: 28.02.2008
38 //
39 // Modifications:
40 //
41 
42 //
43 // Class Description:
44 //
45 //
46 // -------------------------------------------------------------------
47 //
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50 
52 #include "G4PhysicalConstants.hh"
53 
54 using namespace std;
55 
57  const G4String& nam)
58  : G4MuPairProductionModel(p, nam)
59 {}
60 
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62 
64 {}
65 
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67 
69  G4double tkin,
70  G4double Z,
71  G4double pairEnergy)
72 // differential cross section
73 {
74  G4double bbbtf= 183. ;
75  G4double bbbh = 202.4 ;
76  G4double g1tf = 1.95e-5 ;
77  G4double g2tf = 5.3e-5 ;
78  G4double g1h = 4.4e-5 ;
79  G4double g2h = 4.8e-5 ;
80 
81  G4double totalEnergy = tkin + particleMass;
82  G4double residEnergy = totalEnergy - pairEnergy;
83  G4double massratio = particleMass/electron_mass_c2 ;
84  G4double massratio2 = massratio*massratio ;
85  G4double cross = 0.;
86 
88 
89  G4double c3 = 0.75*sqrte*particleMass;
90  if (residEnergy <= c3*z13) return cross;
91 
92  G4double c7 = 4.*electron_mass_c2;
93  G4double c8 = 6.*particleMass*particleMass;
94  G4double alf = c7/pairEnergy;
95  G4double a3 = 1. - alf;
96  if (a3 <= 0.) return cross;
97 
98  // zeta calculation
99  G4double bbb,g1,g2;
100  if( Z < 1.5 ) { bbb = bbbh ; g1 = g1h ; g2 = g2h ; }
101  else { bbb = bbbtf; g1 = g1tf; g2 = g2tf; }
102 
103  G4double zeta = 0;
104  G4double zeta1 = 0.073*log(totalEnergy/(particleMass+g1*z23*totalEnergy))-0.26;
105  if ( zeta1 > 0.)
106  {
107  G4double zeta2 = 0.058*log(totalEnergy/(particleMass+g2*z13*totalEnergy))-0.14;
108  zeta = zeta1/zeta2 ;
109  }
110 
111  G4double z2 = Z*(Z+zeta);
112  G4double screen0 = 2.*electron_mass_c2*sqrte*bbb/(z13*pairEnergy);
113  G4double a0 = totalEnergy*residEnergy;
114  G4double a1 = pairEnergy*pairEnergy/a0;
115  G4double bet = 0.5*a1;
116  G4double xi0 = 0.25*massratio2*a1;
117  G4double del = c8/a0;
118 
119  G4double rta3 = sqrt(a3);
120  G4double tmnexp = alf/(1. + rta3) + del*rta3;
121  if(tmnexp >= 1.0) return cross;
122 
123  G4double tmn = log(tmnexp);
124  G4double sum = 0.;
125 
126  // Gaussian integration in ln(1-ro) ( with 8 points)
127  for (G4int i=0; i<8; i++)
128  {
129  G4double a4 = exp(tmn*xgi[i]); // a4 = (1.-asymmetry)
130  G4double a5 = a4*(2.-a4) ;
131  G4double a6 = 1.-a5 ;
132  G4double a7 = 1.+a6 ;
133  G4double a9 = 3.+a6 ;
134  G4double xi = xi0*a5 ;
135  G4double xii = 1./xi ;
136  G4double xi1 = 1.+xi ;
137  G4double screen = screen0*xi1/a5 ;
138  G4double yeu = 5.-a6+4.*bet*a7 ;
139  G4double yed = 2.*(1.+3.*bet)*log(3.+xii)-a6-a1*(2.-a6) ;
140  G4double ye1 = 1.+yeu/yed ;
141  G4double ale=log(bbb/z13*sqrt(xi1*ye1)/(1.+screen*ye1)) ;
142  G4double cre = 0.5*log(1.+2.25*z23*xi1*ye1/massratio2) ;
143  G4double be;
144 
145  if (xi <= 1.e3) be = ((2.+a6)*(1.+bet)+xi*a9)*log(1.+xii)+(a5-bet)/xi1-a9;
146  else be = (3.-a6+a1*a7)/(2.*xi);
147 
148  G4double fe = (ale-cre)*be;
149  if ( fe < 0.) fe = 0. ;
150 
151  G4double ymu = 4.+a6 +3.*bet*a7 ;
152  G4double ymd = a7*(1.5+a1)*log(3.+xi)+1.-1.5*a6 ;
153  G4double ym1 = 1.+ymu/ymd ;
154  G4double alm_crm = log(bbb*massratio/(1.5*z23*(1.+screen*ym1)));
155  G4double a10,bm;
156  if ( xi >= 1.e-3)
157  {
158  a10 = (1.+a1)*a5 ;
159  bm = (a7*(1.+1.5*bet)-a10*xii)*log(xi1)+xi*(a5-bet)/xi1+a10;
160  } else {
161  bm = (5.-a6+bet*a9)*(xi/2.);
162  }
163 
164  G4double fm = alm_crm*bm;
165  if ( fm < 0.) fm = 0. ;
166 
167  sum += wgi[i]*a4*(fe+fm/massratio2);
168  }
169 
170  cross = -tmn*sum*factorForCross*z2*residEnergy/(totalEnergy*pairEnergy);
171 
172  return cross;
173 }
174 
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