Geant4 11.1.1
Toolkit for the simulation of the passage of particles through matter
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G4SmpNuDistDataU233_235.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//
57
58#include <cmath>
59#include "G4fissionEvent.hh"
60#include "G4Exp.hh"
61#include "G4Pow.hh"
62
63int G4fissionEvent::G4SmpNuDistDataU233_235(G4double nubar) {
64
66/*
67 Description
68 Sample Number of Neutrons from fission in U-233 and U-235 using
69 Zucker and Holden's tabulated data for U-235
70 The P(nu) distribution is given as a function of the average
71 number of neutrons from fission, based on interpolation of the
72 U-235 data from Zucker and Holden.
73*/
74
75/*
76 Input
77 nubar - average number of neutrons per fission
78 Output
79 G4SmpNuDistDataU233_235 - sampled multiplicity
80
81*/
82
83 G4double pnu[8], cpnu, sum;
84 G4double r;
85
86/*
87 Check if nubar is within the range of experimental values
88*/
89 if(nubar >= 2.25 && nubar <= 4.0) {
90/*
91 Use Zucker and Holden Data
92*/
93 if(nubar <= 2.8738) pnu[0]=-9.279554e-02*Pow->powN(nubar,3)+8.036687e-01*Pow->powN(nubar,2)-2.342684*nubar+2.309035;
94 else if(nubar > 2.8738 && nubar <= 3.4272) pnu[0]=1.50072e-2*Pow->powN(nubar,2)-1.109109e-1*nubar+2.063133e-1;
95 else pnu[0]=1.498897e+3*G4Exp(-3.883864*nubar);
96
97 if(nubar <= 3.2316) pnu[1]=3.531126e-2*Pow->powN(nubar,3)-2.787213e-1*Pow->powN(nubar,2)+5.824072e-1*nubar-1.067136e-1;
98 else pnu[1]=6.574492e-2*Pow->powN(nubar,2)-5.425741e-1*nubar+1.123199;
99
100 pnu[2]=1.274643e-2*Pow->powN(nubar,3)-1.387954e-1*Pow->powN(nubar,2)+3.264669e-1*nubar+1.77148e-1;
101
102 pnu[3]=5.473738e-2*Pow->powN(nubar,5)-8.835826e-1*Pow->powN(nubar,4)+5.657201*Pow->powN(nubar,3)-1.802669e+1*Pow->powN(nubar,2)+2.867937e+1*nubar-1.794296e+1;
103
104 pnu[4]=-3.591076e-2*Pow->powN(nubar,3)+3.092624e-1*Pow->powN(nubar,2)-7.184805e-1*nubar+5.649400e-1;
105
106 if(nubar <= 2.8738) pnu[5]=1.699374e-2*Pow->powN(nubar,2)-1.069558e-3*nubar-6.981430e-2;
107 else pnu[5]=2.100175e-2*Pow->powN(nubar,3)-1.705788e-1*Pow->powN(nubar,2)+5.575467e-1*nubar-6.245873e-1;
108
109 if(nubar <= 3.0387) pnu[6]=9.431919e-7*Pow->powA(nubar,8.958848);
110 else pnu[6]=4.322428e-3*Pow->powN(nubar,3)-2.094790e-2*Pow->powN(nubar,2)+4.449671e-2*nubar-4.435987e-2;
111
112 pnu[7]=5.689084e-3*Pow->powN(nubar,4)-6.591895e-2*Pow->powN(nubar,3)+2.886861e-1*Pow->powN(nubar,2)-5.588146e-1*nubar+4.009166e-1;
113
114 sum=pnu[0]+pnu[1]+pnu[2]+pnu[3]+pnu[4]+pnu[5]+pnu[6]+pnu[7];
115
116 pnu[0]=pnu[0]/sum;
117 pnu[1]=pnu[1]/sum;
118 pnu[2]=pnu[2]/sum;
119 pnu[3]=pnu[3]/sum;
120 pnu[4]=pnu[4]/sum;
121 pnu[5]=pnu[5]/sum;
122 pnu[6]=pnu[6]/sum;
123 pnu[7]=pnu[7]/sum;
124
125 r=fisslibrng();
126
127 if(r <= pnu[0]) return (int) 0;
128
129 cpnu=pnu[0]+pnu[1];
130 if(r <= cpnu) return (int) 1;
131
132 cpnu=cpnu+pnu[2];
133 if(r <= cpnu) return (int) 2;
134
135 cpnu=cpnu+pnu[3];
136 if(r <= cpnu) return (int) 3;
137
138 cpnu=cpnu+pnu[4];
139 if(r <= cpnu) return (int) 4;
140
141 cpnu=cpnu+pnu[5];
142 if(r <= cpnu) return (int) 5;
143
144 cpnu=cpnu+pnu[6];
145 if(r <= cpnu) return (int) 6;
146 else return (int) 7;
147 } else {
148/*
149 Use Terrell's formula
150*/
151 return (int) G4SmpTerrell(nubar);
152 }
153}
G4double G4Exp(G4double initial_x)
Exponential Function double precision.
Definition: G4Exp.hh:180
double G4double
Definition: G4Types.hh:83
Definition: G4Pow.hh:49
static G4Pow * GetInstance()
Definition: G4Pow.cc:41
G4double powN(G4double x, G4int n) const
Definition: G4Pow.cc:162
G4double powA(G4double A, G4double y) const
Definition: G4Pow.hh:230