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Redistributions of source code must retain the above copyright notice, 00033 // this list of conditions and the following disclaimer. 00034 // 2. Redistributions in binary form must reproduce the above copyright notice, 00035 // this list of conditions and the following disclaimer in the documentation 00036 // and/or other materials provided with the distribution. 00037 // 3. The name of the author may not be used to endorse or promote products 00038 // derived from this software without specific prior written permission. 00039 // 00040 // THIS SOFTWARE IS PROVIDED BY THE AUTHOR ``AS IS'' AND ANY EXPRESS OR IMPLIED 00041 // WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF 00042 // MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO 00043 // EVENT SHALL THE AUTHOR BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, 00044 // SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, 00045 // PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; 00046 // OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, 00047 // WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR 00048 // OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF 00049 // ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. 00050 // 00051 // Copyright (c) 2006 The Regents of the University of California. 00052 // All rights reserved. 00053 // UCRL-CODE-224807 00054 // 00055 // 00056 // $Id: G4SmpNuDistDataU233_235_MC.cc 69860 2013-05-16 14:39:02Z gcosmo $ 00057 // 00058 00059 #include <cmath> 00060 #include "G4fissionEvent.hh" 00061 00062 G4int G4fissionEvent::G4SmpNuDistDataU233_235_MC(G4double nubar) { 00063 00064 /* 00065 Description 00066 Sample Number of Neutrons from fission in U-233 and U-235 using 00067 Zucker and Holden's tabulated data for U-235 00068 The 11 P(nu) distributions are given as a function of nubar, 00069 the average number of neutrons from induced fission for the 00070 11 different energies (0 to 10 MeV), based on the U-235 data 00071 from Zucker and Holden. 00072 */ 00073 00074 /* 00075 Input 00076 nubar - average number of neutrons per fission 00077 Output 00078 G4SmpNuDistDataU233_235_MC - sampled multiplicity 00079 00080 */ 00081 00082 static G4double U235nu [11] [8] = { 00083 {.0317223, .1717071, .3361991, .3039695, .1269459, .0266793, .0026322, .0001449}, 00084 {.0237898, .1555525, .3216515, .3150433, .1444732, .0356013, .0034339, .0004546}, 00085 {.0183989, .1384891, .3062123, .3217566, .1628673, .0455972, .0055694, .0011093}, 00086 {.0141460, .1194839, .2883075, .3266568, .1836014, .0569113, .0089426, .0019504}, 00087 {.0115208, .1032624, .2716849, .3283426, .2021206, .0674456, .0128924, .0027307}, 00088 {.0078498, .0802010, .2456595, .3308175, .2291646, .0836912, .0187016, .0039148}, 00089 {.0046272, .0563321, .2132296, .3290407, .2599806, .1045974, .0265604, .0056322}, 00090 {.0024659, .0360957, .1788634, .3210507, .2892537, .1282576, .0360887, .0079244}, 00091 {.0012702, .0216090, .1472227, .3083032, .3123950, .1522540, .0462449, .0107009}, 00092 {.0007288, .0134879, .1231200, .2949390, .3258251, .1731879, .0551737, .0135376}, 00093 {.0004373, .0080115, .1002329, .2779283, .3342611, .1966100, .0650090, .0175099} 00094 }; 00095 static G4double U235nubar [11] = { 00096 2.4140000, 00097 2.5236700, 00098 2.6368200, 00099 2.7623400, 00100 2.8738400, 00101 3.0386999, 00102 3.2316099, 00103 3.4272800, 00104 3.6041900, 00105 3.7395900, 00106 3.8749800 00107 }; 00108 G4double fraction, r, cum; 00109 G4int engind, nu; 00110 00111 /* 00112 Check if nubar is within the range of experimental values 00113 */ 00114 if(nubar >= U235nubar[0] && nubar <= U235nubar[10]) { 00115 /* 00116 Use Zucker and Holden Data 00117 */ 00118 engind = 1; 00119 while (nubar > U235nubar[engind]){ engind++;} 00120 fraction = (nubar-U235nubar[engind-1])/(U235nubar[engind]-U235nubar[engind-1]); 00121 if(fisslibrng() > fraction) engind--; 00122 00123 r = fisslibrng(); 00124 nu = 0; 00125 cum = U235nu[engind][0]; 00126 while (r > cum && nu < 7){ 00127 nu++; 00128 cum += U235nu[engind][nu]; 00129 } 00130 return nu; 00131 } else { 00132 /* 00133 Use Terrell's formula 00134 */ 00135 return (G4int) G4SmpTerrell(nubar); 00136 } 00137 }