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Redistributions in binary form must reproduce the above copyright notice, // this list of conditions and the following disclaimer in the documentation // and/or other materials provided with the distribution. // 3. The name of the author may not be used to endorse or promote products // derived from this software without specific prior written permission. // // THIS SOFTWARE IS PROVIDED BY THE AUTHOR ``AS IS'' AND ANY EXPRESS OR IMPLIED // WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF // MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO // EVENT SHALL THE AUTHOR BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, // SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, // PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; // OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, // WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR // OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF // ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. // // Copyright (c) 2006 The Regents of the University of California. // All rights reserved. // UCRL-CODE-224807 // // // $Id: G4SmpNuDistDataU233_235_MC.cc,v 1.2 2007/06/01 13:46:53 gcosmo Exp $ // #include #include "G4fissionEvent.hh" G4int G4fissionEvent::G4SmpNuDistDataU233_235_MC(G4double nubar) { /* Description Sample Number of Neutrons from fission in U-233 and U-235 using Zucker and Holden's tabulated data for U-235 The 11 P(nu) distributions are given as a function of nubar, the average number of neutrons from induced fission for the 11 different energies (0 to 10 MeV), based on the U-235 data from Zucker and Holden. */ /* Input nubar - average number of neutrons per fission Output G4SmpNuDistDataU233_235_MC - sampled multiplicity */ static G4double U235nu [11] [8] = { {.0317223, .1717071, .3361991, .3039695, .1269459, .0266793, .0026322, .0001449}, {.0237898, .1555525, .3216515, .3150433, .1444732, .0356013, .0034339, .0004546}, {.0183989, .1384891, .3062123, .3217566, .1628673, .0455972, .0055694, .0011093}, {.0141460, .1194839, .2883075, .3266568, .1836014, .0569113, .0089426, .0019504}, {.0115208, .1032624, .2716849, .3283426, .2021206, .0674456, .0128924, .0027307}, {.0078498, .0802010, .2456595, .3308175, .2291646, .0836912, .0187016, .0039148}, {.0046272, .0563321, .2132296, .3290407, .2599806, .1045974, .0265604, .0056322}, {.0024659, .0360957, .1788634, .3210507, .2892537, .1282576, .0360887, .0079244}, {.0012702, .0216090, .1472227, .3083032, .3123950, .1522540, .0462449, .0107009}, {.0007288, .0134879, .1231200, .2949390, .3258251, .1731879, .0551737, .0135376}, {.0004373, .0080115, .1002329, .2779283, .3342611, .1966100, .0650090, .0175099} }; static G4double U235nubar [11] = { 2.4140000, 2.5236700, 2.6368200, 2.7623400, 2.8738400, 3.0386999, 3.2316099, 3.4272800, 3.6041900, 3.7395900, 3.8749800 }; G4double fraction, r, cum; G4int engind, nu; /* Check if nubar is within the range of experimental values */ if(nubar >= U235nubar[0] && nubar <= U235nubar[10]) { /* Use Zucker and Holden Data */ engind = 1; while (nubar > U235nubar[engind]){ engind++;} fraction = (nubar-U235nubar[engind-1])/(U235nubar[engind]-U235nubar[engind-1]); if(fisslibrng() > fraction) engind--; r = fisslibrng(); nu = 0; cum = U235nu[engind][0]; while (r > cum && nu < 7){ nu++; cum += U235nu[engind][nu]; } return nu; } else { /* Use Terrell's formula */ return (G4int) G4SmpTerrell(nubar); } }