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G4SmpNuDistDataU232_234_236_238.cc
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56 // $Id: G4SmpNuDistDataU232_234_236_238.cc 67966 2013-03-13 09:38:38Z gcosmo $
57 //
58 
59 #include <cmath>
60 #include "G4fissionEvent.hh"
61 
62 G4int G4fissionEvent::G4SmpNuDistDataU232_234_236_238(G4double nubar) {
63 
64 /*
65  Description
66  Sample Number of Neutrons from fission in U-232, U-234, U-236
67  and U-238 using Zucker and Holden's tabulated data for U-238
68  The P(nu) distribution is given as a function of the average
69  number of neutrons from fission, based on interpolation of the
70  U-238 data from Zucker and Holden.
71 */
72 
73 /*
74  Input
75  nubar - average number of neutrons per fission
76  Output
77  G4SmpNuDistDataU232_234_236_238 - sampled multiplicity
78 
79 */
80 
81  G4double pnu[9], cpnu, sum;
82  G4double r;
83 
84 /*
85  Check if nubar is within the range of experimental values
86 */
87  if (nubar >= 2.25 && nubar <= 3.80) {
88 /*
89  Use Zucker and Holden Data
90 */
91  pnu[0]=-7.705432e-3*std::pow(nubar,3)+8.904671e-2*std::pow(nubar,2)-3.488123e-1*nubar+4.627291e-1;
92  pnu[1]=-2.879938e-2*std::pow(nubar,3)+3.629189e-1*std::pow(nubar,2)-1.545284*nubar+2.229503;
93  pnu[2]=6.543684e-2*std::pow(nubar,3)-6.673117e-1*std::pow(nubar,2)+2.087358*nubar-1.771396;
94  pnu[3]=1.412971e-2*std::pow(nubar,3)-2.309842e-1*std::pow(nubar,2)+1.022451*nubar-1.032235;
95  pnu[4]=-5.163167e-2*std::pow(nubar,3)+4.457516e-1*std::pow(nubar,2)-1.114981*nubar+9.484241e-1;
96  pnu[5]=8.758841e-4*std::pow(nubar,3)+3.707461e-2*std::pow(nubar,2)-1.565149e-1*nubar+1.851039e-1;
97  pnu[6]=-3.871089e-5*std::pow(nubar,3)+1.936524e-2*std::pow(nubar,2)-8.091057e-2*nubar+9.019871e-2;
98  pnu[7]=3.945995e-3*std::pow(nubar,3)-2.697509e-2*std::pow(nubar,2)+6.237296e-2*nubar-4.820745e-2;
99  pnu[8]=1.708054e-3*std::pow(nubar,4)-1.706039e-2*std::pow(nubar,3)+6.550213e-2*std::pow(nubar,2)-1.135e-1*nubar+7.443828e-2;
100 
101  sum=pnu[0]+pnu[1]+pnu[2]+pnu[3]+pnu[4]+pnu[5]+pnu[6]+pnu[7]+pnu[8];
102 
103  pnu[0]=pnu[0]/sum;
104  pnu[1]=pnu[1]/sum;
105  pnu[2]=pnu[2]/sum;
106  pnu[3]=pnu[3]/sum;
107  pnu[4]=pnu[4]/sum;
108  pnu[5]=pnu[5]/sum;
109  pnu[6]=pnu[6]/sum;
110  pnu[7]=pnu[7]/sum;
111  pnu[8]=pnu[8]/sum;
112 
113  r=fisslibrng();
114 
115  if(r <= pnu[0]) return 0;
116 
117  cpnu=pnu[0]+pnu[1];
118  if(r <= cpnu) return 1;
119 
120  cpnu=cpnu+pnu[2];
121  if(r <= cpnu) return 2;
122 
123  cpnu=cpnu+pnu[3];
124  if(r <= cpnu) return 3;
125 
126  cpnu=cpnu+pnu[4];
127  if(r <= cpnu) return 4;
128 
129  cpnu=cpnu+pnu[5];
130  if(r <= cpnu) return 5;
131 
132  cpnu=cpnu+pnu[6];
133  if(r <= cpnu) return 6;
134 
135  cpnu=cpnu+pnu[7];
136  if(r <= cpnu) return 7;
137  else return 8;
138 
139  } else {
140 /*
141  Use Terrell's formula
142 */
143  return (G4int) G4SmpTerrell(nubar);
144  }
145 }
int G4int
Definition: G4Types.hh:78
double G4double
Definition: G4Types.hh:76