| [807] | 1 | //
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| 2 | // ********************************************************************
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| 3 | // * License and Disclaimer *
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| 4 | // * *
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| 5 | // * The Geant4 software is copyright of the Copyright Holders of *
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| 6 | // * the Geant4 Collaboration. It is provided under the terms and *
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| 7 | // * conditions of the Geant4 Software License, included in the file *
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| 8 | // * LICENSE and available at http://cern.ch/geant4/license . These *
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| 9 | // * include a list of copyright holders. *
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| 10 | // * *
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| 11 | // * Neither the authors of this software system, nor their employing *
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| 12 | // * institutes,nor the agencies providing financial support for this *
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| 13 | // * work make any representation or warranty, express or implied, *
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| 14 | // * regarding this software system or assume any liability for its *
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| 15 | // * use. Please see the license in the file LICENSE and URL above *
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| 16 | // * for the full disclaimer and the limitation of liability. *
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| 17 | // * *
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| 18 | // * This code implementation is the result of the scientific and *
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| 19 | // * technical work of the GEANT4 collaboration. *
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| 20 | // * By using, copying, modifying or distributing the software (or *
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| 21 | // * any work based on the software) you agree to acknowledge its *
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| 22 | // * use in resulting scientific publications, and indicate your *
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| 23 | // * acceptance of all terms of the Geant4 Software license. *
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| 24 | // ********************************************************************
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| 25 | //
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| 26 | //
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| 27 | // $Id: RemSimPrimaryGeneratorAction.cc,v 1.17 2006/06/29 16:24:09 gunter Exp $// Author: Susanna Guatelli, guatelli@ge.infn.it
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| 28 |
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| 29 | #include "RemSimPrimaryGeneratorAction.hh"
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| 30 | #ifdef G4ANALYSIS_USE
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| 31 | #include "RemSimAnalysisManager.hh"
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| 32 | #endif
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| 33 | #include "G4Event.hh"
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| 34 | #include "G4ParticleGun.hh"
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| 35 | #include "G4ParticleTable.hh"
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| 36 | #include "G4ParticleDefinition.hh"
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| 37 | #include "Randomize.hh"
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| 38 | #include <fstream>
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| 39 | #include "G4DataVector.hh"
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| 40 | #include "RemSimPrimaryGeneratorMessenger.hh"
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| 41 | #include <math.h>
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| 42 |
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| 43 | RemSimPrimaryGeneratorAction::RemSimPrimaryGeneratorAction()
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| 44 | {
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| 45 | readFile = false;
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| 46 |
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| 47 | particleGun = new G4ParticleGun(1);
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| 48 | messenger = new RemSimPrimaryGeneratorMessenger(this);
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| 49 |
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| 50 | energies = new G4DataVector;
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| 51 | data = new G4DataVector;
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| 52 |
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| 53 | size = 0;
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| 54 |
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| 55 | G4ParticleTable* particleTable = G4ParticleTable::GetParticleTable();
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| 56 | G4String ParticleName = "proton";
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| 57 | G4ParticleDefinition* particle = particleTable->FindParticle(ParticleName);
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| 58 |
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| 59 | particleGun->SetParticleDefinition(particle);
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| 60 |
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| 61 | // Default values of the primary generator
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| 62 | G4ThreeVector position(0,0,-25. *m);
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| 63 | particleGun -> SetParticlePosition(position);
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| 64 | G4ThreeVector direction(0., 0., 1.);
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| 65 | particleGun -> SetParticleMomentumDirection(direction);
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| 66 | particleGun -> SetParticleEnergy(250. * MeV);
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| 67 | }
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| 68 |
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| 69 | RemSimPrimaryGeneratorAction::~RemSimPrimaryGeneratorAction()
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| 70 | {
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| 71 | delete data;
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| 72 | delete energies;
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| 73 | delete [] cumulate;
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| 74 | delete [] energy;
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| 75 | delete messenger;
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| 76 | delete particleGun;
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| 77 | }
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| 78 |
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| 79 | G4double RemSimPrimaryGeneratorAction::GetInitialEnergy()
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| 80 | {
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| 81 | G4double primaryParticleEnergy = particleGun -> GetParticleEnergy();
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| 82 | return primaryParticleEnergy;
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| 83 | }
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| 84 |
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| 85 | void RemSimPrimaryGeneratorAction::GeneratePrimaries(G4Event* anEvent)
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| 86 | {
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| 87 | G4int baryon = particleGun -> GetParticleDefinition() -> GetBaryonNumber();
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| 88 |
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| 89 | // Generate the energy spectrum of primary particles according to
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| 90 | // the flux reported in the .txt file (firt column = Energy (MeV/nucl),
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| 91 | // second column = differnetila flux). The fluxes are derived from CREME96
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| 92 | if (readFile == true)
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| 93 | {
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| 94 | // Uniform number between 0. and 1.
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| 95 | G4double random = G4UniformRand();
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| 96 |
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| 97 | G4int nbelow = 0; // largest k such that I[k] is known to be <= rand
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| 98 | G4int nabove = size; // largest k such that I[k] is known to be > rand
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| 99 | G4int middle;
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| 100 |
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| 101 | while (nabove > nbelow+1) {
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| 102 | middle = (nabove + nbelow+1)>>1;
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| 103 | if (random >= cumulate[middle]) {
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| 104 | nbelow = middle;
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| 105 | } else {
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| 106 | nabove = middle;
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| 107 | }
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| 108 | }
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| 109 |
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| 110 | // Linear interpolation
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| 111 |
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| 112 | G4double energy_gun = 0. * MeV;
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| 113 |
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| 114 | G4double binMeasure = cumulate[nabove] - cumulate[nbelow];
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| 115 |
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| 116 | if ( binMeasure == 0 ) {
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| 117 |
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| 118 | energy_gun = (energy[nbelow] + random*(energy[nabove] - energy[nbelow]))* baryon;
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| 119 | G4cout<<"BinMeasure is zero !!!!!"<<G4endl;
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| 120 | }
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| 121 |
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| 122 | else
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| 123 | {
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| 124 | G4double binFraction = (random - cumulate[nbelow]) / binMeasure;
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| 125 | energy_gun = energy[nbelow] + binFraction *(energy[nabove] - energy[nbelow]);
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| 126 | }
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| 127 | particleGun -> SetParticleEnergy(energy_gun * baryon);
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| 128 | }
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| 129 |
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| 130 | #ifdef G4ANALYSIS_USE
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| 131 | G4double energy_plot = (particleGun -> GetParticleEnergy())/baryon;
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| 132 | // plot of MeV/nucl
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| 133 | RemSimAnalysisManager* analysis = RemSimAnalysisManager::getInstance();
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| 134 | // Plot the energy spectrum of primary particles
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| 135 | analysis -> primaryParticleEnergyDistribution(energy_plot/MeV);
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| 136 | #endif
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| 137 |
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| 138 | particleGun -> GeneratePrimaryVertex(anEvent);
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| 139 | }
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| 140 |
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| 141 | void RemSimPrimaryGeneratorAction::ReadProbability(G4String fileName)
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| 142 | {
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| 143 | // This method allows to read the .txt files containing the
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| 144 | // fluxes of the galactic cosmic rays derived form CREME96
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| 145 | readFile = true;
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| 146 |
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| 147 | std::ifstream file(fileName, std::ios::in);
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| 148 | std::filebuf* lsdp = file.rdbuf();
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| 149 |
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| 150 | if (! (lsdp->is_open()) )
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| 151 | {
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| 152 | G4String excep = "RemSimPrimaryGenerator - data file: "
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| 153 | + fileName + " not found";
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| 154 | G4Exception(excep);
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| 155 | }
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| 156 |
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| 157 | G4double a = 0;
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| 158 | G4int index = 0;
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| 159 | G4int k = 1;
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| 160 |
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| 161 | do
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| 162 | {
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| 163 | file >> a;
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| 164 | G4int nColumns = 2;
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| 165 | // The file is organized into two columns:
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| 166 | // column contains the probability distribution
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| 167 | // The file terminates with the pattern: -1
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| 168 | // -2
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| 169 | if (a == -1 || a == -2)
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| 170 | {
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| 171 |
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| 172 | }
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| 173 | else
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| 174 | {
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| 175 | if (k%nColumns != 0)
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| 176 | {
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| 177 | G4double energy = a *MeV;
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| 178 | energies -> push_back(energy);
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| 179 | // G4cout << "energy: " << energy << G4endl;
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| 180 | k++;
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| 181 | }
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| 182 | else if (k%nColumns == 0)
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| 183 | {
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| 184 | G4double data_value = a;
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| 185 | data -> push_back(data_value);
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| 186 | //G4cout<< "probability: "<< data_value << G4endl;
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| 187 | k=1;
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| 188 | index++;
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| 189 | }
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| 190 | }
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| 191 | } while (a != -2); // end of file
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| 192 |
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| 193 | file.close();
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| 194 | size = index -1 ;
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| 195 | cumulate = new G4double[size+1];
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| 196 | energy = new G4double[size+1];
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| 197 | cumulate[0] = 0;
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| 198 | energy [0] = (*energies)[0];
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| 199 |
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| 200 | for (G4int ptn = 0; ptn <size; ptn++ ) {
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| 201 |
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| 202 | G4double yy = ((*data)[ptn+1] + (*data)[ptn])/2.;
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| 203 | G4double weight = yy *((*energies)[ptn +1] - (*energies)[ptn]);
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| 204 | cumulate[ptn +1] = cumulate[ptn] + weight;
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| 205 | energy[ptn+1] = (*energies)[ptn+1];
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| 206 | }
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| 207 |
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| 208 | // Normalise the cumulate to 1 (that corresponds to the last value)
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| 209 | for ( G4int ptn= 0; ptn < size + 1; ptn++ )
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| 210 | {
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| 211 | cumulate[ptn] /= cumulate[size];
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| 212 | }
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| 213 | }
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| 214 |
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| 215 |
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