source: trunk/source/processes/hadronic/models/lll_fission/src/G4SmpNuDistDataU232_234_236_238.cc @ 1326

Last change on this file since 1326 was 819, checked in by garnier, 16 years ago

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56// $Id: G4SmpNuDistDataU232_234_236_238.cc,v 1.2 2007/06/01 13:46:53 gcosmo Exp $
57//
58
59#include <cmath>
60#include "G4fissionEvent.hh"
61
62G4int 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}
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