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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 // $Id: G4SmpTerrell.cc 67966 2013-03-13 09:38:38Z gcosmo $ 56 // 57 // 57 58 58 #include <cmath> 59 #include <cmath> 59 #include "G4Exp.hh" << 60 #include "G4Log.hh" << 61 #include "G4fissionEvent.hh" 60 #include "G4fissionEvent.hh" 62 61 63 #define TWOPI 6.283185307 62 #define TWOPI 6.283185307 64 #define SQRT2 1.414213562 63 #define SQRT2 1.414213562 65 #define BSHIFT -0.43287 64 #define BSHIFT -0.43287 66 #define WIDTH 1.079 65 #define WIDTH 1.079 67 66 68 G4double G4fissionEvent::G4SmpTerrell(G4double 67 G4double G4fissionEvent::G4SmpTerrell(G4double nubar) { 69 /* 68 /* 70 Description 69 Description 71 Sample Fission Number from Terrell's modif 70 Sample Fission Number from Terrell's modified Gaussian distribution 72 71 73 method uses Red Cullen's algoritm UCRL-TR- 72 method uses Red Cullen's algoritm UCRL-TR-222526 74 */ 73 */ 75 74 76 /* 75 /* 77 Input 76 Input 78 nubar - average number of neutrons per 77 nubar - average number of neutrons per fission 79 Output 78 Output 80 G4SmpTerrell - sampled multiplicity 79 G4SmpTerrell - sampled multiplicity 81 80 82 */ 81 */ 83 82 84 G4double width; 83 G4double width; 85 G4double temp1, temp2, expo, cshift; 84 G4double temp1, temp2, expo, cshift; 86 G4double rw, theta, sampleg; 85 G4double rw, theta, sampleg; 87 86 88 87 89 if (nubar < WIDTH) { 88 if (nubar < WIDTH) { 90 std::ostringstream o; 89 std::ostringstream o; 91 o << nubar; 90 o << nubar; 92 const std::string& errMsg = "fission nubar << 91 std::string errMsg = "fission nubar out of range, nubar=" + o.str(); 93 G4fissionerr(6, "SmpTerrell", errMsg); 92 G4fissionerr(6, "SmpTerrell", errMsg); 94 } 93 } 95 94 96 width = SQRT2 * WIDTH; 95 width = SQRT2 * WIDTH; 97 temp1 = nubar + 0.5; 96 temp1 = nubar + 0.5; 98 temp2 = temp1/width; 97 temp2 = temp1/width; 99 temp2 *= temp2; 98 temp2 *= temp2; 100 expo = G4Exp(-temp2); << 99 expo = std::exp(-temp2); 101 cshift = temp1 + BSHIFT * WIDTH * expo/(1. - 100 cshift = temp1 + BSHIFT * WIDTH * expo/(1. - expo); 102 101 103 G4int icounter = 0; << 104 G4int icounter_max = 1024; << 105 do { 102 do { 106 rw = std::sqrt(-G4Log(fisslibrng())); << 103 rw = std::sqrt(-std::log(fisslibrng())); 107 theta = TWOPI * fisslibrng(); 104 theta = TWOPI * fisslibrng(); 108 sampleg = width * rw * std::cos(theta) + c 105 sampleg = width * rw * std::cos(theta) + cshift; 109 icounter++; << 110 if ( icounter > icounter_max ) { << 111 G4cout << "Loop-counter exceeded the thr << 112 break; << 113 } << 114 } while (sampleg < 0.0); 106 } while (sampleg < 0.0); 115 // Loop checking, 11.03.2015, T. Koi << 116 107 117 return std::floor(sampleg); 108 return std::floor(sampleg); 118 } 109 } 119 110