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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: G4SmpNuDistDataPu239_241.cc,v 1.2 2007/06/01 13:46:53 gcosmo Exp $ // #include #include "G4fissionEvent.hh" G4int G4fissionEvent::G4SmpNuDistDataPu239_241(G4double nubar) { /* Description Sample Number of Neutrons from fission in Pu-239 and Pu-241 using Zucker and Holden's tabulated data for Pu-239 The P(nu) distribution is given as a function of the average number of neutrons from fission, based on interpolation of the Pu-239 data from Zucker and Holden. */ /* Input nubar - average number of neutrons per fission Output G4SmpNuDistDataPu239_241 - sampled multiplicity */ G4double pnu[9], cpnu, sum; G4double r; /* Check if nubar is within the range of experimental values */ if(nubar >= 2.85 && nubar <= 4.25) { /* Use Zucker and Holden Data */ pnu[0]=-2.412937e-3*std::pow(nubar,3)+3.210687e-2*std::pow(nubar,2)-1.434037e-1*nubar+2.150733e-1; pnu[1]=-2.650615e-2*std::pow(nubar,3)+3.290389e-1*std::pow(nubar,2)-1.389007*nubar+2.002327; pnu[2]=3.232028e-2*std::pow(nubar,3)-3.176093e-1*std::pow(nubar,2)+8.605098e-1*nubar-3.411191e-1; pnu[3]=1.623289e-2*std::pow(nubar,3)-2.414705e-1*std::pow(nubar,2)+1.007282*nubar-9.583769e-1; pnu[4]=1.932275e-2*std::pow(nubar,3)-2.923666e-1*std::pow(nubar,2)+1.421383*nubar-1.924025; pnu[5]=-6.185679e-2*std::pow(nubar,3)+6.82888e-1*std::pow(nubar,2)-2.347653*nubar+2.647049; pnu[6]=1.79773e-2*std::pow(nubar,3)-1.60516e-1*std::pow(nubar,2)+5.228077e-1*nubar-5.939556e-1; pnu[7]=3.530038e-3*std::pow(nubar,4)-4.925425e-2*std::pow(nubar,3)+2.726784e-1*std::pow(nubar,2)-6.81281e-1*nubar+6.347577e-1; pnu[8]=2.837523e-3*std::pow(nubar,3)-2.678644e-2*std::pow(nubar,2)+8.545638e-2*nubar-9.156078e-2; sum=pnu[0]+pnu[1]+pnu[2]+pnu[3]+pnu[4]+pnu[5]+pnu[6]+pnu[7]+pnu[8]; 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; pnu[8]=pnu[8]/sum; r=fisslibrng(); if(r <= pnu[0]) return 0; cpnu=pnu[0]+pnu[1]; if(r <= cpnu) return 1; cpnu=cpnu+pnu[2]; if(r <= cpnu) return 2; cpnu=cpnu+pnu[3]; if(r <= cpnu) return 3; cpnu=cpnu+pnu[4]; if(r <= cpnu) return 4; cpnu=cpnu+pnu[5]; if(r <= cpnu) return 5; cpnu=cpnu+pnu[6]; if(r <= cpnu) return 6; cpnu=cpnu+pnu[7]; if(r <= cpnu) return 7; else return 8; } else { /* Use Terrell's formula */ return (G4int) G4SmpTerrell(nubar); } }