// // ******************************************************************** // * License and Disclaimer * // * * // * The Geant4 software is copyright of the Copyright Holders of * // * the Geant4 Collaboration. It is provided under the terms and * // * conditions of the Geant4 Software License, included in the file * // * LICENSE and available at http://cern.ch/geant4/license . These * // * include a list of copyright holders. * // * * // * Neither the authors of this software system, nor their employing * // * institutes,nor the agencies providing financial support for this * // * work make any representation or warranty, express or implied, * // * regarding this software system or assume any liability for its * // * use. Please see the license in the file LICENSE and URL above * // * for the full disclaimer and the limitation of liability. * // * * // * This code implementation is the result of the scientific and * // * technical work of the GEANT4 collaboration. * // * By using, copying, modifying or distributing the software (or * // * any work based on the software) you agree to acknowledge its * // * use in resulting scientific publications, and indicate your * // * acceptance of all terms of the Geant4 Software license. * // ******************************************************************** // // -------------------------------------------------------------------- // // GEANT4 Test file // // File name: PIXEtest // // Author: Simona Saliceti (simona.saliceti@ge.infn.it) // // History: // -------- // // 22 Apr 2009 ALF 1st implementation based on work of Simona Saliceti // 24 Apr 2009 ALF revision // -------------------------------------------------------------------- // // Test Description: // ------------------ // Test of second implementation of the Empiric Model for shell cross sections in proton ionisation // -------------------------------------------------------------------- // $Id: PIXEtest.cc,v 1.2 2009/06/18 16:18:42 mantero Exp $ // GEANT4 tag $Name: geant4-09-03-cand-01 $ #include "globals.hh" #include "G4ios.hh" #include #include #include #include #include "G4VhShellCrossSection.hh" #include "G4hShellCrossSection.hh" #include "G4hShellCrossSectionDoubleExp.hh" #include "G4teoCrossSection.hh" #include "G4empCrossSection.hh" #include "G4AtomicTransitionManager.hh" #include "G4Proton.hh" //#include "AIDA/AIDA.h" int main() { G4int Z; G4double incidentEnergy; G4double mass; G4double deltaEnergy; size_t shellNumber; G4String fileName; // G4VhShellCrossSection* shellExp = new G4hShellCrossSectionDoubleExp(); // here you deciude the implementation: G4teoCrossSection is ECPSSR for K + Orlic for L shells // G4hShellCrossSectionDoubleExp is previous work with ownmade fitting functions to Pauli for Alpha. G4VhShellCrossSection* shellCS = new G4teoCrossSection("ecpssr"); //G4VhShellCrossSection* shellCS = new G4empCrossSection(); //proton mass in Kg //mass = 1.67262158e-27 * kg; G4Proton* aProtone = G4Proton::Proton(); mass = aProtone->GetPDGMass(); std::vector energies; //Energy from 0.005 MeV to 500 MeV for (G4double i=-5.5; i<6.5; i=i+0.125) { energies.push_back(std::exp(i)*MeV); } G4cout << "Enter shell number: " << G4endl; G4cin >> shellNumber; G4cout << "Enter filename: " << G4endl; G4cin >> fileName; if (fileName == "" ) {fileName = "PIXECrossSection";} G4String fileNameTxt = fileName; char buffer[3]; std::ofstream myfile; //Z is the atomic number for (Z = 6; Z<=92; Z++) { G4cout << "Z = " << Z << G4endl; snprintf(buffer, 3, "%d", Z); fileNameTxt = fileName + buffer + ".dat"; myfile.open (fileNameTxt); //Cross section for each incident energy for (size_t k=0; k CS = shellCS->GetCrossSection(Z,incidentEnergy,mass,deltaEnergy,false); myfile << incidentEnergy << "\t" << CS[shellNumber] << G4endl; //barn //error in ecpssr/orlic class: correct units management! } myfile.close(); fileNameTxt = fileName; } delete shellCS; G4cout<<"END OF THE MAIN PROGRAM"<