// // ******************************************************************** // * 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 Class file // // // File name: G4PhotoElectricAngularGeneratorSauterGavrila // // Creation date: 10 May 2004 // // Modifications: // 10 May 2003 P. Rodrigues First implementation acording with new design // // Class Description: // // Concrete class for PhotoElectric Electron Angular Distribution Generation // This model is a re-implementation of the Photolectric angular distribution // developed my M. Maire for the Standard EM Physics G4PhotoElectricEffect // // Class Description: End // // ------------------------------------------------------------------- // // #include "G4PhotoElectricAngularGeneratorSauterGavrila.hh" #include "Randomize.hh" // G4PhotoElectricAngularGeneratorSauterGavrila::G4PhotoElectricAngularGeneratorSauterGavrila(const G4String& name):G4VPhotoElectricAngularDistribution(name) {;} // G4PhotoElectricAngularGeneratorSauterGavrila::~G4PhotoElectricAngularGeneratorSauterGavrila() {;} // G4ThreeVector G4PhotoElectricAngularGeneratorSauterGavrila::GetPhotoElectronDirection(const G4ThreeVector& direction, const G4double eKineticEnergy, const G4ThreeVector&, const G4int) const { // Compute Theta distribution of the emitted electron, with respect to the // incident Gamma. // The Sauter-Gavrila distribution for the K-shell is used. (adapted from G4PhotoElectricEffect) G4double costeta = 1.; G4double Phi = twopi * G4UniformRand(); G4double cosphi = std::cos(Phi); G4double sinphi = std::sin(Phi); G4double sinteta = 0; G4double gamma = 1. + eKineticEnergy/electron_mass_c2; if (gamma > 5.) { G4ThreeVector direction (sinteta*cosphi, sinteta*sinphi, costeta); return costeta; } G4double beta = std::sqrt(gamma*gamma-1.)/gamma; G4double b = 0.5*gamma*(gamma-1.)*(gamma-2); G4double rndm,term,greject,grejsup; if (gamma < 2.) grejsup = gamma*gamma*(1.+b-beta*b); else grejsup = gamma*gamma*(1.+b+beta*b); do { rndm = 1.-2*G4UniformRand(); costeta = (rndm+beta)/(rndm*beta+1.); term = 1.-beta*costeta; greject = (1.-costeta*costeta)*(1.+b*term)/(term*term); } while(greject < G4UniformRand()*grejsup); sinteta = std::sqrt(1.-costeta*costeta); G4ThreeVector photoelectrondirection (sinteta*cosphi, sinteta*sinphi, costeta); photoelectrondirection.rotateUz(direction); return photoelectrondirection; } // void G4PhotoElectricAngularGeneratorSauterGavrila::PrintGeneratorInformation() const { G4cout << "\n" << G4endl; G4cout << "" << G4endl; G4cout << "Re-implementation of the photolectric angular distribution" << G4endl; G4cout << "developed my M. Maire for the Standard EM Physics G4PhotoElectricEffect" << G4endl; G4cout << "It computes the theta distribution of the emitted electron, with respect to the" << G4endl; G4cout << "incident Gamma, using the Sauter-Gavrila distribution for the K-shell\n" << G4endl; }