Gabriele Cosmo
126 lines
4.9 KiB
C++
126 lines
4.9 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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//
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// $Id: G4AugerTransition.hh v0.1
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//
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//
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// Author: Alfonso Mantero (Alfosno.Mantero@ge.infn.it)
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//
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// History:
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// -----------
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// 1 Jun 2002: first Commited to CVS
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// -------------------------------------------------------------------
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// Class description:
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// Low Energy Electromagnetic Physics
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// This Class stores all the information of auger effect relative
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// to one main vacancy in a atom, like possible auger emission with
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// relative probabilites, originating shell's Ids, probabilities of
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// transition and auger electron energies.
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// Further documentation available from http://www.ge.infn.it/geant4/lowE
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// -------------------------------------------------------------------
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#ifndef G4AugerTransition_h
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#define G4AugerTransition_h 1
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#include "G4DataVector.hh"
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#include "globals.hh"
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#include <vector>
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#include <map>
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class G4AugerTransition {
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public:
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G4AugerTransition(G4int finalShell, std::vector<G4int> transIds,
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const std::map<G4int, std::vector<G4int>, std::less<G4int> >* idMap,
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const std::map<G4int, G4DataVector, std::less<G4int> >* energyMap,
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const std::map<G4int, G4DataVector, std::less<G4int> >* probabilityMap);
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~G4AugerTransition();
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// All the data stored and provided by this class are relative to a
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// given vacancy, whose identity is provided by the FinalShellId() method,
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// in an atom of a given material
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// Returns the ids of the shells from wich an auger electron culd came from, given the shell
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// from wich the transition electron comes from.
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const std::vector<G4int>* AugerOriginatingShellIds(G4int startShellId) const;
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// Returns the ids of the shells from wich an electron cuuld fill the vacancy in finalShellId
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const std::vector<G4int>* TransitionOriginatingShellIds() const;
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// Returns the energiess of the possible auger electrons, given th shell
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// from wich the transition electron comes from.
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const G4DataVector* AugerTransitionEnergies(G4int startShellId) const;
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// Returns the emission probabilities of the auger electrons, given th shell
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// from wich the transition electron comes from.
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const G4DataVector* AugerTransitionProbabilities(G4int startShellId) const;
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// returns the id of the shell in wich the transition electron arrives
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G4int FinalShellId() const;
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// Returns the id of the shell from wich come the auger electron , given the shell
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// from wich the transition electron comes from and the index number.
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G4int AugerOriginatingShellId(G4int index, G4int startShellId) const;
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// Returns the energy of the auger electron, given the shell
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// from wich the transition electron comes from and the index number.
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G4double AugerTransitionEnergy(G4int index, G4int startShellId) const;
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// Returns the probability of the auger emission, given the shell
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// from wich the transition electron comes from and the index number.
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G4double AugerTransitionProbability(G4int index, G4int startShellId) const;
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// Returns the id of the shell form wich the transition electron come from
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G4int TransitionOriginatingShellId(G4int index) const;
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private:
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G4int finalShellId;
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std::map<G4int,std::vector<G4int>,std::less<G4int> > augerOriginatingShellIdsMap;
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std::map<G4int,G4DataVector,std::less<G4int> > augerTransitionEnergiesMap;
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std::map<G4int,G4DataVector,std::less<G4int> > augerTransitionProbabilitiesMap;
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std::vector<G4int> transitionOriginatingShellIds;
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};
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#endif
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