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24 | // ******************************************************************** |
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25 | // |
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26 | // |
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27 | // $Id: G4AugerTransition.hh v0.1 |
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28 | // |
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29 | // |
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30 | // Author: Alfonso Mantero (Alfosno.Mantero@ge.infn.it) |
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31 | // |
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32 | // History: |
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33 | // ----------- |
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34 | // 1 Jun 2002: first Commited to CVS |
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35 | // ------------------------------------------------------------------- |
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36 | |
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37 | // Class description: |
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38 | // Low Energy Electromagnetic Physics |
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39 | // This Class stores all the information of auger effect relative |
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40 | // to one main vacancy in a atom, like possible auger emission with |
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41 | // relative probabilites, originating shell's Ids, probabilities of |
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42 | // transition and auger electron energies. |
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43 | // Further documentation available from http://www.ge.infn.it/geant4/lowE |
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44 | |
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45 | // ------------------------------------------------------------------- |
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46 | |
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47 | #ifndef G4AugerTransition_h |
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48 | #define G4AugerTransition_h 1 |
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49 | |
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50 | #include "G4DataVector.hh" |
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51 | #include "globals.hh" |
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52 | #include <vector> |
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53 | #include <map> |
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54 | |
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55 | class G4AugerTransition { |
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56 | |
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57 | public: |
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58 | |
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59 | G4AugerTransition(G4int finalShell, std::vector<G4int> transIds, |
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60 | const std::map<G4int, std::vector<G4int>, std::less<G4int> >* idMap, |
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61 | const std::map<G4int, G4DataVector, std::less<G4int> >* energyMap, |
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62 | const std::map<G4int, G4DataVector, std::less<G4int> >* probabilityMap); |
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63 | |
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64 | ~G4AugerTransition(); |
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65 | |
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66 | // All the data stored and provided by this class are relative to a |
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67 | // given vacancy, whose identity is provided by the FinalShellId() method, |
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68 | // in an atom of a given material |
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69 | |
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70 | // Returns the ids of the shells from wich an auger electron culd came from, given the shell |
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71 | // from wich the transition electron comes from. |
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72 | |
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73 | const std::vector<G4int>* AugerOriginatingShellIds(G4int startShellId) const; |
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74 | |
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75 | // Returns the ids of the shells from wich an electron cuuld fill the vacancy in finalShellId |
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76 | |
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77 | const std::vector<G4int>* TransitionOriginatingShellIds() const; |
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78 | |
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79 | // Returns the energiess of the possible auger electrons, given th shell |
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80 | // from wich the transition electron comes from. |
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81 | |
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82 | const G4DataVector* AugerTransitionEnergies(G4int startShellId) const; |
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83 | |
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84 | // Returns the emission probabilities of the auger electrons, given th shell |
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85 | // from wich the transition electron comes from. |
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86 | |
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87 | const G4DataVector* AugerTransitionProbabilities(G4int startShellId) const; |
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88 | |
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89 | // returns the id of the shell in wich the transition electron arrives |
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90 | |
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91 | G4int FinalShellId() const; |
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92 | |
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93 | // Returns the id of the shell from wich come the auger electron , given the shell |
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94 | // from wich the transition electron comes from and the index number. |
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95 | |
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96 | G4int AugerOriginatingShellId(G4int index, G4int startShellId) const; |
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97 | |
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98 | // Returns the energy of the auger electron, given the shell |
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99 | // from wich the transition electron comes from and the index number. |
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100 | |
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101 | G4double AugerTransitionEnergy(G4int index, G4int startShellId) const; |
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102 | |
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103 | // Returns the probability of the auger emission, given the shell |
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104 | // from wich the transition electron comes from and the index number. |
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105 | |
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106 | G4double AugerTransitionProbability(G4int index, G4int startShellId) const; |
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107 | |
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108 | // Returns the id of the shell form wich the transition electron come from |
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109 | |
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110 | G4int TransitionOriginatingShellId(G4int index) const; |
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111 | |
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112 | |
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113 | private: |
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114 | |
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115 | G4int finalShellId; |
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116 | std::map<G4int,std::vector<G4int>,std::less<G4int> > augerOriginatingShellIdsMap; |
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117 | std::map<G4int,G4DataVector,std::less<G4int> > augerTransitionEnergiesMap; |
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118 | std::map<G4int,G4DataVector,std::less<G4int> > augerTransitionProbabilitiesMap; |
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119 | std::vector<G4int> transitionOriginatingShellIds; |
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120 | |
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121 | }; |
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122 | |
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123 | #endif |
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124 | |
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125 | |
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