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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: G4SmpNuDistDataU232_234_236_238_MC.cc,v 1.2 2007/06/01 13:46:53 gcosmo Exp $ // #include #include "G4fissionEvent.hh" G4int G4fissionEvent::G4SmpNuDistDataU232_234_236_238_MC(G4double nubar) { /* Description Sample Number of Neutrons from fission in U-232, U-234, U-236, and U-238 using Zucker and Holden's tabulated data for U-238 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-238 data from Zucker and Holden. */ /* Input nubar - average number of neutrons per fission Output G4SmpNuDistDataU232_234_236_238_MC - sampled multiplicity */ static G4double U238nu [11] [9] = { {.0396484, .2529541, .2939544, .2644470, .1111758, .0312261, .0059347, .0005436, .0001158}, {.0299076, .2043215, .2995886, .2914889, .1301480, .0363119, .0073638, .0006947, .0001751}, {.0226651, .1624020, .2957263, .3119098, .1528786, .0434233, .0097473, .0009318, .0003159}, {.0170253, .1272992, .2840540, .3260192, .1779579, .0526575, .0130997, .0013467, .0005405}, {.0124932, .0984797, .2661875, .3344938, .2040116, .0640468, .0173837, .0020308, .0008730}, {.0088167, .0751744, .2436570, .3379711, .2297901, .0775971, .0225619, .0030689, .0013626}, {.0058736, .0565985, .2179252, .3368863, .2541575, .0933127, .0286200, .0045431, .0031316}, {.0035997, .0420460, .1904095, .3314575, .2760413, .1112075, .0355683, .0065387, .0031316}, {.0019495, .0309087, .1625055, .3217392, .2943792, .1313074, .0434347, .0091474, .0046284}, {.0008767, .0226587, .1356058, .3076919, .3080816, .1536446, .0522549, .0124682, .0067176}, {.0003271, .0168184, .1111114, .2892434, .3160166, .1782484, .0620617, .0166066, .0095665} }; static G4double U238nubar [11] = { 2.2753781, 2.4305631, 2.5857481, 2.7409331, 2.8961181, 3.0513031, 3.2064881, 3.3616731, 3.5168581, 3.6720432, 3.8272281 }; G4double fraction, r, cum; G4int engind, nu; /* Check if nubar is within the range of experimental values */ if(nubar >= U238nubar[0] && nubar <= U238nubar[10]) { /* Use Zucker and Holden Data */ engind = 1; while (nubar > U238nubar[engind]){ engind++;} fraction = (nubar-U238nubar[engind-1])/(U238nubar[engind]-U238nubar[engind-1]); if(fisslibrng() > fraction) engind--; r = fisslibrng(); nu = 0; cum = U238nu[engind][0]; while (r > cum && nu < 8){ nu++; cum += U238nu[engind][nu]; } return nu; } else { /* Use Terrell's formula */ return (G4int) G4SmpTerrell(nubar); } }