Gabriele Cosmo
138 lines
4.4 KiB
C++
138 lines
4.4 KiB
C++
//
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// ********************************************************************
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// * License and Disclaimer *
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// * *
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// * The Geant4 software is copyright of the Copyright Holders of *
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// * the Geant4 Collaboration. It is provided under the terms and *
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// * conditions of the Geant4 Software License, included in the file *
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// * LICENSE and available at http://cern.ch/geant4/license . These *
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// * include a list of copyright holders. *
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// * *
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// * Neither the authors of this software system, nor their employing *
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// * institutes,nor the agencies providing financial support for this *
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// * work make any representation or warranty, express or implied, *
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// * regarding this software system or assume any liability for its *
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// * use. Please see the license in the file LICENSE and URL above *
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// * for the full disclaimer and the limitation of liability. *
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// * *
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// * This code implementation is the result of the scientific and *
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// * technical work of the GEANT4 collaboration. *
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// * By using, copying, modifying or distributing the software (or *
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// * any work based on the software) you agree to acknowledge its *
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// * use in resulting scientific publications, and indicate your *
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// * acceptance of all terms of the Geant4 Software license. *
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// ********************************************************************
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//
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// File name: G4PiMinusStopCo
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//
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// Author: Maria Grazia Pia (pia@genova.infn.it)
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//
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// Creation date: 8 May 1998
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//
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// -------------------------------------------------------------------
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#include "G4ios.hh"
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#include "G4PiMinusStopCo.hh"
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#include <vector>
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#include "globals.hh"
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#include "Randomize.hh"
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#include "G4Proton.hh"
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#include "G4Neutron.hh"
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#include "G4ParticleTypes.hh"
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#include "G4ReactionKinematics.hh"
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#include "G4DynamicParticleVector.hh"
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#include "G4LorentzVector.hh"
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#include "G4PiMinusStopMaterial.hh"
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#include "G4DistributionGenerator.hh"
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// np/pp production ratio
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// Experimental values:
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// R(np/pp) (E. Gadioli et al., Phys Rev C36 (1987) 741
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G4double G4PiMinusStopCo::npRatio = 2.5;
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// Average numbers of final nucleons detected, for N-pair absorption
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// (Hartmann et al., Nucl. Phys. A300 (1978) 345
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G4double G4PiMinusStopCo::nFinalNucleons = 1.38;
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// Kinetic energy (MeV) distributions measured for coincident nucleon
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// emission
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// P. Heusi et al., Nucl. Phys. A407(1983) 429
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G4int G4PiMinusStopCo::eKinEntries = 11;
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G4double G4PiMinusStopCo::eKinData[11] = {0.085, 0.09, 0.09, 0.15,
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0.1, 0.09, 0.08,
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0.04, 0.03, 0.02, 0.01};
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G4double G4PiMinusStopCo::eKin[12] = { 15., 17.5, 25., 33.,
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42., 52., 62.,
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75., 85., 95., 105. };
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// Opening angle distributions measured for coincident nucleon emission
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// (P.Heusi et al., Nucl. Phys. A407 (1983) 429
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G4int G4PiMinusStopCo::angleEntries = 7;
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G4double G4PiMinusStopCo::angleData[7] =
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{6., 8., 9., 10., 25., 40., 45. };
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G4double G4PiMinusStopCo::angle[8] = { 0.5, 0.7, 0.87, 1.4, 2.1,
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2.44, 2.8, 3.1415927 };
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// Constructor
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G4PiMinusStopCo::G4PiMinusStopCo()
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{
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// Cluster size: nucleon pair, alpha, triton etc.
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// First implementation: interaction with nucleon pair only
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_clusterSize = 2;
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// R ratio
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theR = 1. / (1. + npRatio);
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_definitions = new std::vector<G4ParticleDefinition*>();
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_momenta = new std::vector<G4LorentzVector*>();
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std::vector<double> eKinVector;
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std::vector<double> eKinDataVector;
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int i;
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for (i=0; i<eKinEntries; i++)
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{
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eKinVector.push_back(eKin[i]);
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eKinDataVector.push_back(eKinData[i]);
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}
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eKinVector.push_back(eKin[eKinEntries]);
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_distributionE = new G4DistributionGenerator(eKinVector,eKinDataVector);
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std::vector<double> angleVector;
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std::vector<double> angleDataVector;
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for (i=0; i<angleEntries; i++)
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{
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angleVector.push_back(angle[i]);
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angleDataVector.push_back(angleData[i]);
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}
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angleVector.push_back(angle[angleEntries]);
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_distributionAngle = new G4DistributionGenerator(angleVector,angleDataVector);
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}
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// Destructor
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G4PiMinusStopCo::~G4PiMinusStopCo()
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{}
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G4double G4PiMinusStopCo::FinalNucleons()
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{
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return nFinalNucleons;
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}
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