// // ******************************************************************** // * DISCLAIMER * // * * // * The following disclaimer summarizes all the specific disclaimers * // * of contributors to this software. The specific disclaimers,which * // * govern, are listed with their locations in: * // * http://cern.ch/geant4/license * // * * // * 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. * // * * // * This code implementation is the intellectual property of the * // * GEANT4 collaboration. * // * By copying, distributing or modifying the Program (or any work * // * based on the Program) you indicate your acceptance of this * // * statement, and all its terms. * // ******************************************************************** // // // $Id: G4FluoData.hh,v 1.1 ????? // GEANT4 tag $Name: geant4-04-00 $ // // Author: Elena Guardincerri (Elena.Guardincerri@ge.infn.it) // // History: // ----------- // 16 Sept 2001 First committed to cvs // // ------------------------------------------------------------------- // Class description: // Low Energy Electromagnetic Physics // Fluorescence data set: shell identifiers, transition probabilities, // transition energies // Further documentation available from http://www.ge.infn.it/geant4/lowE // ------------------------------------------------------------------- #ifndef G4FLUODATA_HH #define G4FLUODATA_HH 1 #include "globals.hh" #include "g4std/vector" #include "g4std/map" class G4DataVector; class G4FluoData { public: G4FluoData(); ~G4FluoData(); // The method returns the number of shells in wich a // vacancy can be filled by a radiative transition size_t NumberOfVacancies() const; // Given the index of the vacancy returns its identity G4int VacancyId(G4int vacancyIndex) const; // Given the index of a vacancy returns the number of //shells starting from wich an electrons can fill the vacancy size_t NumberOfTransitions(G4int vacancyIndex) const; // Given the indexes of the starting and final shells for the // transition, returns the identity of the starting one G4int StartShellId(G4int initIndex,G4int vacancyIndex); // Given the indexes of the starting and final shells for the // transition, returns the transition energy G4double StartShellEnergy(G4int initIndex,G4int vacancyIndex); // Given the indexes of the starting and final shells for the // transition, returns the probability of this transition G4double StartShellProb(G4int initIndex,G4int vacancyIndex); void LoadData( G4int Z); void PrintData(); private: G4std::map > idMap; G4std::map > energyMap; G4std::map > probabilityMap; G4std::vector nInitShells; G4int numberOfVacancies; }; #endif