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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.cc,v 1.2 2007/06/01 13:46:53 gcosmo Exp $ // #include #include "G4fissionEvent.hh" int G4fissionEvent::G4SmpNuDistDataU233_235(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 P(nu) distribution is given as a function of the average number of neutrons from fission, based on interpolation of the U-235 data from Zucker and Holden. */ /* Input nubar - average number of neutrons per fission Output G4SmpNuDistDataU233_235 - sampled multiplicity */ G4double pnu[8], cpnu, sum; G4double r; /* Check if nubar is within the range of experimental values */ if(nubar >= 2.25 && nubar <= 4.0) { /* Use Zucker and Holden Data */ if(nubar <= 2.8738) pnu[0]=-9.279554e-02*std::pow(nubar,3)+8.036687e-01*std::pow(nubar,2)-2.342684*nubar+2.309035; else if(nubar > 2.8738 && nubar <= 3.4272) pnu[0]=1.50072e-2*std::pow(nubar,2)-1.109109e-1*nubar+2.063133e-1; else pnu[0]=1.498897e+3*std::exp(-3.883864*nubar); if(nubar <= 3.2316) pnu[1]=3.531126e-2*std::pow(nubar,3)-2.787213e-1*std::pow(nubar,2)+5.824072e-1*nubar-1.067136e-1; else pnu[1]=6.574492e-2*std::pow(nubar,2)-5.425741e-1*nubar+1.123199; pnu[2]=1.274643e-2*std::pow(nubar,3)-1.387954e-1*std::pow(nubar,2)+3.264669e-1*nubar+1.77148e-1; pnu[3]=5.473738e-2*std::pow(nubar,5)-8.835826e-1*std::pow(nubar,4)+5.657201*std::pow(nubar,3)-1.802669e+1*std::pow(nubar,2)+2.867937e+1*nubar-1.794296e+1; pnu[4]=-3.591076e-2*std::pow(nubar,3)+3.092624e-1*std::pow(nubar,2)-7.184805e-1*nubar+5.649400e-1; if(nubar <= 2.8738) pnu[5]=1.699374e-2*std::pow(nubar,2)-1.069558e-3*nubar-6.981430e-2; else pnu[5]=2.100175e-2*std::pow(nubar,3)-1.705788e-1*std::pow(nubar,2)+5.575467e-1*nubar-6.245873e-1; if(nubar <= 3.0387) pnu[6]=9.431919e-7*std::pow(nubar,8.958848); else pnu[6]=4.322428e-3*std::pow(nubar,3)-2.094790e-2*std::pow(nubar,2)+4.449671e-2*nubar-4.435987e-2; pnu[7]=5.689084e-3*std::pow(nubar,4)-6.591895e-2*std::pow(nubar,3)+2.886861e-1*std::pow(nubar,2)-5.588146e-1*nubar+4.009166e-1; sum=pnu[0]+pnu[1]+pnu[2]+pnu[3]+pnu[4]+pnu[5]+pnu[6]+pnu[7]; pnu[0]=pnu[0]/sum; pnu[1]=pnu[1]/sum; pnu[2]=pnu[2]/sum; pnu[3]=pnu[3]/sum; pnu[4]=pnu[4]/sum; pnu[5]=pnu[5]/sum; pnu[6]=pnu[6]/sum; pnu[7]=pnu[7]/sum; r=fisslibrng(); if(r <= pnu[0]) return (int) 0; cpnu=pnu[0]+pnu[1]; if(r <= cpnu) return (int) 1; cpnu=cpnu+pnu[2]; if(r <= cpnu) return (int) 2; cpnu=cpnu+pnu[3]; if(r <= cpnu) return (int) 3; cpnu=cpnu+pnu[4]; if(r <= cpnu) return (int) 4; cpnu=cpnu+pnu[5]; if(r <= cpnu) return (int) 5; cpnu=cpnu+pnu[6]; if(r <= cpnu) return (int) 6; else return (int) 7; } else { /* Use Terrell's formula */ return (int) G4SmpTerrell(nubar); } }