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IN NO 43 // EVENT SHALL THE AUTHOR BE LIABLE FOR ANY DI 43 // EVENT SHALL THE AUTHOR BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, 44 // SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGE 44 // SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, 45 // PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES 45 // PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; 46 // OR BUSINESS INTERRUPTION) HOWEVER CAUSED AN 46 // OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, 47 // WHETHER IN CONTRACT, STRICT LIABILITY, OR T 47 // WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR 48 // OTHERWISE) ARISING IN ANY WAY OUT OF THE US 48 // OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF 49 // ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. 49 // ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. 50 // 50 // 51 // Copyright (c) 2006 The Regents of the Unive 51 // Copyright (c) 2006 The Regents of the University of California. 52 // All rights reserved. 52 // All rights reserved. 53 // UCRL-CODE-224807 53 // UCRL-CODE-224807 54 // 54 // 55 // 55 // 56 // 56 // 57 57 58 #include <cmath> 58 #include <cmath> 59 #include "G4fissionEvent.hh" 59 #include "G4fissionEvent.hh" 60 60 61 G4int G4fissionEvent::G4SmpNuDistDataPu239_241 61 G4int G4fissionEvent::G4SmpNuDistDataPu239_241_MC(G4double nubar) { 62 62 63 /* 63 /* 64 Description 64 Description 65 Sample Number of Neutrons from fission in 65 Sample Number of Neutrons from fission in Pu-239 and Pu-241 using 66 Zucker and Holden's tabulated data for Pu- 66 Zucker and Holden's tabulated data for Pu-239 67 The 11 P(nu) distributions are given as a 67 The 11 P(nu) distributions are given as a function of nubar, 68 the average number of neutrons from induce 68 the average number of neutrons from induced fission for the 69 11 different energies (0 to 10 MeV), based 69 11 different energies (0 to 10 MeV), based on the Pu-239 data 70 from Zucker and Holden. 70 from Zucker and Holden. 71 */ 71 */ 72 72 73 /* 73 /* 74 Input 74 Input 75 nubar - average number of neutrons per 75 nubar - average number of neutrons per fission 76 Output 76 Output 77 G4SmpNuDistDataPu239_241_MC - sampled mul 77 G4SmpNuDistDataPu239_241_MC - sampled multiplicity 78 78 79 */ 79 */ 80 80 81 static G4double Pu239nu [11] [9] = { 81 static G4double Pu239nu [11] [9] = { 82 {.0108826, .0994916, .2748898, .3269196, 82 {.0108826, .0994916, .2748898, .3269196, .2046061, .0726834, .0097282, .0006301, .0001685}, 83 {.0084842, .0790030, .2536175, .3289870, 83 {.0084842, .0790030, .2536175, .3289870, .2328111, .0800161, .0155581, .0011760, .0003469}, 84 {.0062555, .0611921, .2265608, .3260637, 84 {.0062555, .0611921, .2265608, .3260637, .2588354, .0956070, .0224705, .0025946, .0005205}, 85 {.0045860, .0477879, .1983002, .3184667, 85 {.0045860, .0477879, .1983002, .3184667, .2792811, .1158950, .0301128, .0048471, .0007233}, 86 {.0032908, .0374390, .1704196, .3071862, 86 {.0032908, .0374390, .1704196, .3071862, .2948565, .1392594, .0386738, .0078701, .0010046}, 87 {.0022750, .0291416, .1437645, .2928006, 87 {.0022750, .0291416, .1437645, .2928006, .3063902, .1641647, .0484343, .0116151, .0014149}, 88 {.0014893, .0222369, .1190439, .2756297, 88 {.0014893, .0222369, .1190439, .2756297, .3144908, .1892897, .0597353, .0160828, .0029917}, 89 {.0009061, .0163528, .0968110, .2558524, 89 {.0009061, .0163528, .0968110, .2558524, .3194566, .2134888, .0729739, .0213339, .0020017}, 90 {.0004647, .0113283, .0775201, .2335926, 90 {.0004647, .0113283, .0775201, .2335926, .3213289, .2356614, .0886183, .0274895, .0039531}, 91 {.0002800, .0071460, .0615577, .2089810, 91 {.0002800, .0071460, .0615577, .2089810, .3200121, .2545846, .1072344, .0347255, .0054786}, 92 {.0002064, .0038856, .0492548, .1822078, 92 {.0002064, .0038856, .0492548, .1822078, .3154159, .2687282, .1295143, .0432654, .0075217} 93 }; 93 }; 94 static G4double Pu239nubar [11] = { 94 static G4double Pu239nubar [11] = { 95 2.8760000, 95 2.8760000, 96 3.0088800, 96 3.0088800, 97 3.1628300, 97 3.1628300, 98 3.3167800, 98 3.3167800, 99 3.4707300, 99 3.4707300, 100 3.6246800, 100 3.6246800, 101 3.7786300, 101 3.7786300, 102 3.9325800, 102 3.9325800, 103 4.0865300, 103 4.0865300, 104 4.2404900, 104 4.2404900, 105 4.3944400 105 4.3944400 106 }; 106 }; 107 G4double fraction, r, cum; 107 G4double fraction, r, cum; 108 G4int engind, nu; 108 G4int engind, nu; 109 109 110 /* 110 /* 111 Check if nubar is within the range of experi 111 Check if nubar is within the range of experimental values 112 */ 112 */ 113 if(nubar >= Pu239nubar[0] && nubar <= Pu239n 113 if(nubar >= Pu239nubar[0] && nubar <= Pu239nubar[10]) { 114 /* 114 /* 115 Use Zucker and Holden Data 115 Use Zucker and Holden Data 116 */ 116 */ 117 engind = 1; 117 engind = 1; 118 while (nubar > Pu239nubar[engind]){ engin 118 while (nubar > Pu239nubar[engind]){ engind++;} 119 // Loop checking, 11.03.2015, T. Koi 119 // Loop checking, 11.03.2015, T. Koi 120 fraction = (nubar-Pu239nubar[engind-1])/( 120 fraction = (nubar-Pu239nubar[engind-1])/(Pu239nubar[engind]-Pu239nubar[engind-1]); 121 if(fisslibrng() > fraction) engind--; 121 if(fisslibrng() > fraction) engind--; 122 122 123 r = fisslibrng(); 123 r = fisslibrng(); 124 nu = 0; 124 nu = 0; 125 cum = Pu239nu[engind][0]; 125 cum = Pu239nu[engind][0]; 126 while (r > cum && nu < 8){ 126 while (r > cum && nu < 8){ 127 // Loop checking, 11.03.2015, T. Koi 127 // Loop checking, 11.03.2015, T. Koi 128 nu++; 128 nu++; 129 cum += Pu239nu[engind][nu]; 129 cum += Pu239nu[engind][nu]; 130 } 130 } 131 return nu; 131 return nu; 132 } else { 132 } else { 133 /* 133 /* 134 Use Terrell's formula 134 Use Terrell's formula 135 */ 135 */ 136 return (G4int) G4SmpTerrell(nubar); 136 return (G4int) G4SmpTerrell(nubar); 137 } 137 } 138 } 138 } 139 139