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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 58 #include <cmath> 59 #include "G4fissionEvent.hh" 60 61 G4int G4fissionEvent::G4SmpNuDistDataU233_235_MC(G4double nubar) { 62 63 /* 64 Description 65 Sample Number of Neutrons from fission in U-233 and U-235 using 66 Zucker and Holden's tabulated data for U-235 67 The 11 P(nu) distributions are given as a function of nubar, 68 the average number of neutrons from induced fission for the 69 11 different energies (0 to 10 MeV), based on the U-235 data 70 from Zucker and Holden. 71 */ 72 73 /* 74 Input 75 nubar - average number of neutrons per fission 76 Output 77 G4SmpNuDistDataU233_235_MC - sampled multiplicity 78 79 */ 80 81 static G4double U235nu [11] [8] = { 82 {.0317223, .1717071, .3361991, .3039695, .1269459, .0266793, .0026322, .0001449}, 83 {.0237898, .1555525, .3216515, .3150433, .1444732, .0356013, .0034339, .0004546}, 84 {.0183989, .1384891, .3062123, .3217566, .1628673, .0455972, .0055694, .0011093}, 85 {.0141460, .1194839, .2883075, .3266568, .1836014, .0569113, .0089426, .0019504}, 86 {.0115208, .1032624, .2716849, .3283426, .2021206, .0674456, .0128924, .0027307}, 87 {.0078498, .0802010, .2456595, .3308175, .2291646, .0836912, .0187016, .0039148}, 88 {.0046272, .0563321, .2132296, .3290407, .2599806, .1045974, .0265604, .0056322}, 89 {.0024659, .0360957, .1788634, .3210507, .2892537, .1282576, .0360887, .0079244}, 90 {.0012702, .0216090, .1472227, .3083032, .3123950, .1522540, .0462449, .0107009}, 91 {.0007288, .0134879, .1231200, .2949390, .3258251, .1731879, .0551737, .0135376}, 92 {.0004373, .0080115, .1002329, .2779283, .3342611, .1966100, .0650090, .0175099} 93 }; 94 static G4double U235nubar [11] = { 95 2.4140000, 96 2.5236700, 97 2.6368200, 98 2.7623400, 99 2.8738400, 100 3.0386999, 101 3.2316099, 102 3.4272800, 103 3.6041900, 104 3.7395900, 105 3.8749800 106 }; 107 G4double fraction, r, cum; 108 G4int engind, nu; 109 110 /* 111 Check if nubar is within the range of experimental values 112 */ 113 if(nubar >= U235nubar[0] && nubar <= U235nubar[10]) { 114 /* 115 Use Zucker and Holden Data 116 */ 117 engind = 1; 118 while (nubar > U235nubar[engind]){ engind++;} 119 // Loop checking, 11.03.2015, T. Koi 120 fraction = (nubar-U235nubar[engind-1])/(U235nubar[engind]-U235nubar[engind-1]); 121 if(fisslibrng() > fraction) engind--; 122 123 r = fisslibrng(); 124 nu = 0; 125 cum = U235nu[engind][0]; 126 while (r > cum && nu < 7){ 127 // Loop checking, 11.03.2015, T. Koi 128 nu++; 129 cum += U235nu[engind][nu]; 130 } 131 return nu; 132 } else { 133 /* 134 Use Terrell's formula 135 */ 136 return (G4int) G4SmpTerrell(nubar); 137 } 138 } 139