Gabriele Cosmo
106 lines
3.8 KiB
C++
106 lines
3.8 KiB
C++
//
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// ********************************************************************
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// * DISCLAIMER *
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// * *
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// * The following disclaimer summarizes all the specific disclaimers *
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// * of contributors to this software. The specific disclaimers,which *
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// * govern, are listed with their locations in: *
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// * http://cern.ch/geant4/license *
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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. *
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// * *
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// * This code implementation is the intellectual property of the *
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// * GEANT4 collaboration. *
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// * By copying, distributing or modifying the Program (or any work *
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// * based on the Program) you indicate your acceptance of this *
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// * statement, and all its terms. *
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// ********************************************************************
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//
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// Author: Elena Guardincerri (Elena.Guardincerri@ge.infn.it)
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//
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// History:
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// -----------
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// 16 Sept 2001 First committed to cvs
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//
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// -------------------------------------------------------------------
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// Class description:
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// Low Energy Electromagnetic Physics
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// Fluorescence data set: shell identifiers, transition probabilities,
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// transition 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 G4FLUODATA_HH
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#define G4FLUODATA_HH 1
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#include "globals.hh"
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#include <vector>
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#include <map>
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class G4FluoTransition;
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class G4DataVector;
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class G4FluoData
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{
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public:
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G4FluoData();
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~G4FluoData();
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// The method returns the number of shells in wich a
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// vacancy can be filled by a radiative transition
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size_t NumberOfVacancies() const;
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// Given the index of the vacancy returns its identity
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G4int VacancyId(G4int vacancyIndex) const;
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// Given the index of a vacancy returns the number of
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//shells starting from wich an electrons can fill the vacancy
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size_t NumberOfTransitions(G4int vacancyIndex) const;
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// Given the indexes of the starting and final shells for the
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// transition, returns the identity of the starting one
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G4int StartShellId(G4int initIndex, G4int vacancyIndex) const;
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// Given the indexes of the starting and final shells for the
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// transition, returns the transition energy
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G4double StartShellEnergy(G4int initIndex, G4int vacancyIndex) const;
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// Given the indexes of the starting and final shells for the
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// transition, returns the probability of this transition
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G4double StartShellProb(G4int initIndex, G4int vacancyIndex) const;
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void LoadData(G4int Z);
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void PrintData();
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//void BuildFluoTransitionTable();
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//std::vector<G4FluoTransition*> GetFluoTransitions(G4int Z);
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//G4FluoTransition GetFluoTransition(G4int Z, G4int shellId);
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private:
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// Hide copy constructor and assignment operator
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G4FluoData& operator=(const G4FluoData& right);
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G4FluoData(const G4FluoData&);
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std::map<G4int,G4DataVector*,std::less<G4int> > idMap;
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std::map<G4int,G4DataVector*,std::less<G4int> > energyMap;
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std::map<G4int,G4DataVector*,std::less<G4int> > probabilityMap;
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std::vector<G4int> nInitShells;
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G4int numberOfVacancies;
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std::map<G4int,std::vector<G4FluoTransition*>,std::less<G4int> > fluoTransitionTable;
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};
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#endif
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