Geant4 11.2.2
Toolkit for the simulation of the passage of particles through matter
Loading...
Searching...
No Matches
G4LLNLFission.cc
Go to the documentation of this file.
1//
2// ********************************************************************
3// * License and Disclaimer *
4// * *
5// * The Geant4 software is copyright of the Copyright Holders of *
6// * the Geant4 Collaboration. It is provided under the terms and *
7// * conditions of the Geant4 Software License, included in the file *
8// * LICENSE and available at http://cern.ch/geant4/license . These *
9// * include a list of copyright holders. *
10// * *
11// * Neither the authors of this software system, nor their employing *
12// * institutes,nor the agencies providing financial support for this *
13// * work make any representation or warranty, express or implied, *
14// * regarding this software system or assume any liability for its *
15// * use. Please see the license in the file LICENSE and URL above *
16// * for the full disclaimer and the limitation of liability. *
17// * *
18// * This code implementation is the result of the scientific and *
19// * technical work of the GEANT4 collaboration. *
20// * By using, copying, modifying or distributing the software (or *
21// * any work based on the software) you agree to acknowledge its *
22// * use in resulting scientific publications, and indicate your *
23// * acceptance of all terms of the Geant4 Software license. *
24// ********************************************************************
25//
26//
27// This software was developed by Lawrence Livermore National Laboratory.
28//
29// Redistribution and use in source and binary forms, with or without
30// modification, are permitted provided that the following conditions are met:
31//
32// 1. Redistributions of source code must retain the above copyright notice,
33// this list of conditions and the following disclaimer.
34// 2. Redistributions in binary form must reproduce the above copyright notice,
35// this list of conditions and the following disclaimer in the documentation
36// and/or other materials provided with the distribution.
37// 3. The name of the author may not be used to endorse or promote products
38// derived from this software without specific prior written permission.
39//
40// THIS SOFTWARE IS PROVIDED BY THE AUTHOR ``AS IS'' AND ANY EXPRESS OR IMPLIED
41// WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF
42// MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO
43// EVENT SHALL THE AUTHOR BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL,
44// SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO,
45// PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS;
46// OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY,
47// WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR
48// OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF
49// ADVISED OF THE POSSIBILITY OF SUCH DAMAGE.
50//
51// Copyright (c) 2006 The Regents of the University of California.
52// All rights reserved.
53// UCRL-CODE-224807
54//
55//
56//
57// This class is a copy of Fission.cc, made for use with Geant4.
58//
59
60#include "G4fissionEvent.hh"
61
63
64 extern G4float (*rngfptr) (void);
65
66 extern G4double (*rngdptr) (void);
67
68 extern G4double rngf2d(void);
69
70 void genspfissevt_(G4int *isotope, G4double *time) {
71 if (fe != 0) delete fe;
72 fe = new G4fissionEvent(*isotope, *time, -1., 0.);
73 }
74
75 void genfissevt_(G4int *isotope, G4double *time, G4double *nubar, G4double *eng) {
76 if (fe != 0) delete fe;
77 fe = new G4fissionEvent(*isotope, *time, *nubar, *eng);
78 }
79
81 return (*fe).getNeutronNu();
82 }
83
85 return (*fe).getPhotonNu();
86 }
87
89 return (*fe).getNeutronEnergy(*index);
90 }
91
93 return (*fe).getNeutronVelocity(*index);
94 }
95
97 return (*fe).getNeutronDircosu(*index);
98 }
99
101 return (*fe).getNeutronDircosv(*index);
102 }
103
105 return (*fe).getNeutronDircosw(*index);
106 }
107
109 return (*fe).getPhotonEnergy(*index);
110 }
111
113 return (*fe).getPhotonVelocity(*index);
114 }
115
117 return (*fe).getPhotonDircosu(*index);
118 }
119
121 return (*fe).getPhotonDircosv(*index);
122 }
123
125 return (*fe).getPhotonDircosw(*index);
126 }
127
129 return (*fe).getNeutronAge(*index);
130 }
131
133 return (*fe).getPhotonAge(*index);
134 }
135
136 void setdelay_(G4int *delay) {
137 (*fe).setDelayOption(*delay);
138 }
139
140 void setcorrel_(G4int *correlation) {
141 (*fe).setCorrelationOption(*correlation);
142 }
143
144 void setnudist_(G4int *nudist) {
145/*
146 where the argument *nudist affects induced fissions only, it
147 is set to
148 0 for sampling Zucker and Holden probability distributions
149 for U-235,238 and Pu-239. Terrell for other isotopes.
150 1 same as above, but using Gwin, Spencer and Ingle
151 tabulated distributions for thermal energies for U-235.
152 Terrell for other isotopes.
153 2 for sampling fission-induced neutron multiplicity in
154 (a) U-232, U-234, U-236 and U-238 using Zucker and
155 Holden's tabulated data for U-238
156 (b) U-233 and U-235 using Zucker and Holden's tabulated
157 data for U-235
158 (c) Pu-239 and Pu-241 using Zucker and Holden's tabulated
159 data for Pu-239
160 The P(nu) distributions for *nudist=2 are given as a
161 function of the average number of neutrons from fission,
162 based on interpolation of the data from Zucker and Holden.
163 Terrell for other isotopes.
164 3 for sampling fission-induced neutron multiplicity in
165 (a) U-232, U-234, U-236 and U-238 using Zucker and
166 Holden's tabulated data for U-238
167 (b) U-233 and U-235 using Zucker and Holden's tabulated
168 data for U-235
169 (c) Pu-239 and Pu-241 using Zucker and Holden's tabulated
170 data for Pu-239
171 The Z&H tables have P(nu) distributions for 11 energies
172 (0 MeV through 10 MeV), along with their nubars. For
173 *nudist=3, we select the P(nu) distribution that has
174 a nubar closest either from above, or from below, to the
175 to the nubar entered for the induced fission, based on a
176 random number and fractional distances to the end of the
177 nubar interval thus formed.
178 Terrell for other isotopes.
179*/
180
181 (*fe).setNudistOption(*nudist);
182 }
183
184 void setcf252_(G4int *ndist, G4int *neng) {
185/*
186 where the argument
187 *ndist is set to
188 0 to sample the spontaneous fission neutron multiplicity
189 using tabulated data from Spencer
190 1 to sample the spontaneous fission neutron multiplicity
191 using tabulated data from Boldeman
192 *neng is set to
193 0 to sample the Mannhart corrected Maxwellian spectrum
194 1 to sample the Madland-Nix theoretical spectrum
195 2 to sample the Froehner Watt spectrum
196*/
197 (*fe).setCf252Option(*ndist, *neng);
198 }
199
200 void setrngf_(G4float (*funcptr) (void)) {
202 }
203
204 void setrngd_(G4double (*funcptr) (void)) {
206 }
207// }
void setrngf_(G4float(*funcptr)(void))
G4double rngf2d(void)
void setdelay_(G4int *delay)
G4double getndircosu_(G4int *index)
G4double(* rngdptr)(void)
void setcorrel_(G4int *correlation)
void setcf252_(G4int *ndist, G4int *neng)
G4double getpdircosw_(G4int *index)
G4float(* rngfptr)(void)
G4int getnnu_()
G4double getndircosw_(G4int *index)
G4double getpdircosu_(G4int *index)
G4double getneng_(G4int *index)
void genspfissevt_(G4int *isotope, G4double *time)
void genfissevt_(G4int *isotope, G4double *time, G4double *nubar, G4double *eng)
G4double getpeng_(G4int *index)
G4double getpage_(G4int *index)
G4double getndircosv_(G4int *index)
G4double getnage_(G4int *index)
G4fissionEvent * fe
G4double getpdircosv_(G4int *index)
G4double getpvel_(G4int *index)
G4int getpnu_()
G4double getnvel_(G4int *index)
void setnudist_(G4int *nudist)
void setrngd_(G4double(*funcptr)(void))
float G4float
Definition G4Types.hh:84
double G4double
Definition G4Types.hh:83
int G4int
Definition G4Types.hh:85
static void setRNGf(float(*funcptr)(void))
static void setRNGd(G4double(*funcptr)(void))