Geant4 9.6.0
Toolkit for the simulation of the passage of particles through matter
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G4SmpNuDistDataPu239_241.cc
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51// Copyright (c) 2006 The Regents of the University of California.
52// All rights reserved.
53// UCRL-CODE-224807
54//
55//
56// $Id$
57//
58
59#include <cmath>
60#include "G4fissionEvent.hh"
61
62G4int G4fissionEvent::G4SmpNuDistDataPu239_241(G4double nubar) {
63
64/*
65 Description
66 Sample Number of Neutrons from fission in Pu-239 and Pu-241 using
67 Zucker and Holden's tabulated data for Pu-239
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 Pu-239 data from Zucker and Holden.
71*/
72
73/*
74 Input
75 nubar - average number of neutrons per fission
76 Output
77 G4SmpNuDistDataPu239_241 - 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 >= 2.85 && nubar <= 4.25) {
88/*
89 Use Zucker and Holden Data
90*/
91 pnu[0]=-2.412937e-3*std::pow(nubar,3)+3.210687e-2*std::pow(nubar,2)-1.434037e-1*nubar+2.150733e-1;
92 pnu[1]=-2.650615e-2*std::pow(nubar,3)+3.290389e-1*std::pow(nubar,2)-1.389007*nubar+2.002327;
93 pnu[2]=3.232028e-2*std::pow(nubar,3)-3.176093e-1*std::pow(nubar,2)+8.605098e-1*nubar-3.411191e-1;
94 pnu[3]=1.623289e-2*std::pow(nubar,3)-2.414705e-1*std::pow(nubar,2)+1.007282*nubar-9.583769e-1;
95 pnu[4]=1.932275e-2*std::pow(nubar,3)-2.923666e-1*std::pow(nubar,2)+1.421383*nubar-1.924025;
96 pnu[5]=-6.185679e-2*std::pow(nubar,3)+6.82888e-1*std::pow(nubar,2)-2.347653*nubar+2.647049;
97 pnu[6]=1.79773e-2*std::pow(nubar,3)-1.60516e-1*std::pow(nubar,2)+5.228077e-1*nubar-5.939556e-1;
98 pnu[7]=3.530038e-3*std::pow(nubar,4)-4.925425e-2*std::pow(nubar,3)+2.726784e-1*std::pow(nubar,2)-6.81281e-1*nubar+6.347577e-1;
99 pnu[8]=2.837523e-3*std::pow(nubar,3)-2.678644e-2*std::pow(nubar,2)+8.545638e-2*nubar-9.156078e-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}
double G4double
Definition: G4Types.hh:64
int G4int
Definition: G4Types.hh:66