Gabriele Cosmo
156 lines
6.8 KiB
C++
156 lines
6.8 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: G4IonisParamElm.cc 96794 2016-05-09 10:09:30Z gcosmo $
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//
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//
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//....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo.... ....oooOO0OOooo....
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//
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// 09-07-98, data moved from G4Element. M.Maire
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// 22-11-00, tabulation of ionisation potential from
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// the ICRU Report N#37. V.Ivanchenko
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// 08-03-01, correct handling of fShellCorrectionVector. M.Maire
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// 17-10-02, Fix excitation energy interpolation. V.Ivanchenko
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// 06-09-04, Update calculated values after any change of ionisation
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// potential change. V.Ivanchenko
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// 29-04-10, Using G4Pow and mean ionisation energy from NIST V.Ivanchenko
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// 27.10.11: new scheme for G4Exception (mma)
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//
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//....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo.... ....oooOO0OOooo....
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#include "G4IonisParamElm.hh"
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#include "G4NistManager.hh"
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#include "G4Pow.hh"
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#include "G4PhysicalConstants.hh"
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#include "G4SystemOfUnits.hh"
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//....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo.... ....oooOO0OOooo....
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G4IonisParamElm::G4IonisParamElm(G4double AtomNumber)
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{
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G4int Z = G4lrint(AtomNumber);
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if (Z < 1) {
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G4Exception("G4IonisParamElm::G4IonisParamElm()", "mat501", FatalException,
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"It is not allowed to create an Element with Z<1");
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}
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G4Pow* g4pow = G4Pow::GetInstance();
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// some basic functions of the atomic number
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fZ = Z;
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fZ3 = g4pow->Z13(Z);
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fZZ3 = fZ3*g4pow->Z13(Z+1);
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flogZ3 = g4pow->logZ(Z)/3.;
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fMeanExcitationEnergy =
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G4NistManager::Instance()->GetMeanIonisationEnergy(Z);
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// compute parameters for ion transport
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// The aproximation from:
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// J.F.Ziegler, J.P. Biersack, U. Littmark
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// The Stopping and Range of Ions in Matter,
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// Vol.1, Pergamon Press, 1985
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// Fast ions or hadrons
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G4int iz = Z - 1;
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if(91 < iz) { iz = 91; }
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static const G4double vFermi[92] = {
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1.0309, 0.15976, 0.59782, 1.0781, 1.0486, 1.0, 1.058, 0.93942, 0.74562, 0.3424,
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0.45259, 0.71074, 0.90519, 0.97411, 0.97184, 0.89852, 0.70827, 0.39816, 0.36552, 0.62712,
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0.81707, 0.9943, 1.1423, 1.2381, 1.1222, 0.92705, 1.0047, 1.2, 1.0661, 0.97411,
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0.84912, 0.95, 1.0903, 1.0429, 0.49715, 0.37755, 0.35211, 0.57801, 0.77773, 1.0207,
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1.029, 1.2542, 1.122, 1.1241, 1.0882, 1.2709, 1.2542, 0.90094, 0.74093, 0.86054,
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0.93155, 1.0047, 0.55379, 0.43289, 0.32636, 0.5131, 0.695, 0.72591, 0.71202, 0.67413,
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0.71418, 0.71453, 0.5911, 0.70263, 0.68049, 0.68203, 0.68121, 0.68532, 0.68715, 0.61884,
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0.71801, 0.83048, 1.1222, 1.2381, 1.045, 1.0733, 1.0953, 1.2381, 1.2879, 0.78654,
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0.66401, 0.84912, 0.88433, 0.80746, 0.43357, 0.41923, 0.43638, 0.51464, 0.73087, 0.81065,
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1.9578, 1.0257} ;
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static const G4double lFactor[92] = {
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1.0, 1.0, 1.1, 1.06, 1.01, 1.03, 1.04, 0.99, 0.95, 0.9,
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0.82, 0.81, 0.83, 0.88, 1.0, 0.95, 0.97, 0.99, 0.98, 0.97,
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0.98, 0.97, 0.96, 0.93, 0.91, 0.9, 0.88, 0.9, 0.9, 0.9,
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0.9, 0.85, 0.9, 0.9, 0.91, 0.92, 0.9, 0.9, 0.9, 0.9,
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0.9, 0.88, 0.9, 0.88, 0.88, 0.9, 0.9, 0.88, 0.9, 0.9,
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0.9, 0.9, 0.96, 1.2, 0.9, 0.88, 0.88, 0.85, 0.9, 0.9,
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0.92, 0.95, 0.99, 1.03, 1.05, 1.07, 1.08, 1.1, 1.08, 1.08,
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1.08, 1.08, 1.09, 1.09, 1.1, 1.11, 1.12, 1.13, 1.14, 1.15,
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1.17, 1.2, 1.18, 1.17, 1.17, 1.16, 1.16, 1.16, 1.16, 1.16,
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1.16, 1.16} ;
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fVFermi = vFermi[iz];
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fLFactor = lFactor[iz];
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// obsolete parameters for ionisation
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fTau0 = 0.1*fZ3*MeV/proton_mass_c2;
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fTaul = 2.*MeV/proton_mass_c2;
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// compute the Bethe-Bloch formula for energy = fTaul*particle mass
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G4double rate = fMeanExcitationEnergy/electron_mass_c2 ;
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G4double w = fTaul*(fTaul+2.) ;
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fBetheBlochLow = (fTaul+1.)*(fTaul+1.)*std::log(2.*w/rate)/w - 1. ;
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fBetheBlochLow = 2.*fZ*twopi_mc2_rcl2*fBetheBlochLow ;
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fClow = std::sqrt(fTaul)*fBetheBlochLow;
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fAlow = 6.458040 * fClow/fTau0;
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G4double Taum = 0.035*fZ3*MeV/proton_mass_c2;
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fBlow =-3.229020*fClow/(fTau0*std::sqrt(Taum));
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// Shell correction parameterization
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fShellCorrectionVector = new G4double[3]; //[3]
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rate = 0.001*fMeanExcitationEnergy/eV;
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G4double rate2 = rate*rate;
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/*
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fShellCorrectionVector[0] = ( 1.10289e5 + 5.14781e8*rate)*rate2 ;
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fShellCorrectionVector[1] = ( 7.93805e3 - 2.22565e7*rate)*rate2 ;
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fShellCorrectionVector[2] = (-9.92256e1 + 2.10823e5*rate)*rate2 ;
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*/
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fShellCorrectionVector[0] = ( 0.422377 + 3.858019*rate)*rate2 ;
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fShellCorrectionVector[1] = ( 0.0304043 - 0.1667989*rate)*rate2 ;
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fShellCorrectionVector[2] = (-0.00038106 + 0.00157955*rate)*rate2 ;
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}
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//....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo.... ....oooOO0OOooo....
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// Fake default constructor - sets only member data and allocates memory
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// for usage restricted to object persistency
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G4IonisParamElm::G4IonisParamElm(__void__&)
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: fShellCorrectionVector(nullptr)
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{
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fZ=fZ3=fZZ3=flogZ3=fTau0=fTaul=fBetheBlochLow=fAlow=fBlow=fClow
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=fMeanExcitationEnergy=fVFermi=fLFactor=0.0;
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}
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//....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo.... ....oooOO0OOooo....
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G4IonisParamElm::~G4IonisParamElm()
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{
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if (fShellCorrectionVector) { delete [] fShellCorrectionVector; }
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}
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//....oooOO0OOooo........oooOO0OOooo........oooOO0OOooo.... ....oooOO0OOooo....
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