348 lines
12 KiB
C++
348 lines
12 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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//
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// MODULE: G4SPSEneDistribution.hh
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//
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// Version: 1.0
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// Date: 5/02/04
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// Author: Fan Lei
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// Organisation: QinetiQ ltd.
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// Customer: ESA/ESTEC
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//
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///////////////////////////////////////////////////////////////////////////////
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//
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// CHANGE HISTORY
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// --------------
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//
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//
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// Version 1.0, 05/02/2004, Fan Lei, Created.
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// Based on the G4GeneralParticleSource class in Geant4 v6.0
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//
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//
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// 26/03/2014, Andrew Green.
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// Modification to used STL vectors instead of C-style arrays. This should save some space,
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// particularly when the blackbody function is not used. Also moved to dynamically allocated
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// memory in the LinearInterpolation, ExpInterpolation and LogInterpolation functions. Again,
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// this will save space if these functions are unused.
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//
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// 06/06/2014 A Dotti
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// For thread safety: this is a shared object,
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// mutex has been added to control access to shared resources (data members).
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// in Getters and Setters, mutex is NOT used in GenerateOne because it is
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// assumed that properties are not changed during event loop.
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//
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// 24/11/2017 Fan Lei
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// Added cutoff power-law distribution option. Implementation is similar to that of the BlackBody one.
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//
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///////////////////////////////////////////////////////////////////////////////
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//
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//
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// Class Description:
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//
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// To generate the energy of a primary vertex according to the defined distribution
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//
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///////////////////////////////////////////////////////////////////////////////
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//
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// MEMBER FUNCTIONS
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// ----------------
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//
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// G4SPSEneDistribution ()
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// Constructor: Initializes variables
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//
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// ~G4SPSEneDistribution ()
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// Destructor:
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//
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// void SetEnergyDisType(G4String)
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// Allows the user to choose the energy distribution type. The arguments
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// are Mono (mono-energetic), Lin (linear), Pow (power-law), Exp
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// (exponential), Gauss (gaussian), Brem (bremsstrahlung), BBody (black-body), Cdg
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// (cosmic diffuse gamma-ray), User (user-defined), Arb (arbitrary
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// point-wise), Epn (energy per nucleon).
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//
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// void SetEmin(G4double)
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// Sets the minimum energy.
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//
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// void SetEmax(G4double)
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// Sets the maximum energy.
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//
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// void SetMonoEnergy(G4double)
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// Sets energy for mono-energetic distribution.
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//
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// void SetAlpha(G4double)
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// Sets alpha for a power-law distribution.
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//
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// void SetTemp(G4double)
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// Sets Temperature for a Brem or BBody distributions.
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//
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// void SetEzero(G4double)
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// Sets Ezero for an exponential distribution.
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//
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// void SetGradient(G4double)
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// Sets gradient for a linear distribution.
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//
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// void SetInterCept(G4double)
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// Sets intercept for a linear distribution.
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//
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// void UserEnergyHisto(G4ThreeVector)
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// Allows user to defined a histogram for the energy distribution.
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//
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// void ArbEnergyHisto(G4ThreeVector)
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// Allows the user to define an Arbitrary set of points for the
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// energy distribution.
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//
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// void EpnEnergyHisto(G4ThreeVector)
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// Allows the user to define an Energy per nucleon histogram.
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//
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// void Calculate()
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// Controls the calculation of Integral PDF for the Cdg and BBody
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// distributions.
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//
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// void InputEnergySpectra(G4bool)
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// Allows the user to choose between momentum and energy histograms
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// for user-defined histograms and arbitrary point-wise spectr.
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// The default is true (energy).
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//
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// void InputDifferentialSpectra(G4bool)
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// Allows the user to choose between integral and differential
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// distributions when using the arbitrary point-wise option.
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//
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// void ArbInterpolate(G4String)
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// ArbInterpolate allows the user to specify the type of function to
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// interpolate the Arbitrary points spectrum with.
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//
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// void SetBiasRndm (G4SPSRandomGenerator* a)
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// Sets the biased random number generator
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//
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// G4double GenerateOne(G4ParticleDefinition*);
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// Generate one random energy for the specified particle
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//
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// void ReSetHist(G4String);
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// Re-sets the histogram for user defined distribution
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//
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// void SetVerbosity(G4int)
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// Sets the verbosity level.
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//
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///////////////////////////////////////////////////////////////////////////////
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#ifndef G4SPSEneDistribution_h
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#define G4SPSEneDistribution_h 1
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#include "G4PhysicsOrderedFreeVector.hh"
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#include "G4ParticleMomentum.hh"
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#include "G4ParticleDefinition.hh"
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#include "G4DataInterpolation.hh"
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#include "G4Threading.hh"
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#include "G4Cache.hh"
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#include <vector>
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#include "G4SPSRandomGenerator.hh"
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/** Andrea Dotti Feb 2015
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* Important: This is a shared class between threads.
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* Only one thread should use the set-methods here.
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* Note that this is exactly what is achieved using UI commands.
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* If you use the set methods to set defaults in your
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* application take care that only one thread is executing them.
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* In addition take care of calling these methods before the run is started
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* Do not use these setters during the event loop
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*/
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class G4SPSEneDistribution {
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public:
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G4SPSEneDistribution();//
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~G4SPSEneDistribution();//
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void SetEnergyDisType(G4String);//
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G4String GetEnergyDisType();//
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void SetEmin(G4double);//
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G4double GetEmin();//
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G4double GetArbEmin();//
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void SetEmax(G4double);//
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G4double GetEmax();//
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G4double GetArbEmax();//
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void SetMonoEnergy(G4double);//
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void SetAlpha(G4double);//
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void SetBiasAlpha(G4double);//
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void SetTemp(G4double);//
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void SetBeamSigmaInE(G4double);////
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void SetEzero(G4double);//
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void SetGradient(G4double);//
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void SetInterCept(G4double);//
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void UserEnergyHisto(G4ThreeVector);//
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void ArbEnergyHisto(G4ThreeVector);//
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void ArbEnergyHistoFile(G4String);//
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void EpnEnergyHisto(G4ThreeVector);//
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void InputEnergySpectra(G4bool);//
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void InputDifferentialSpectra(G4bool);//
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void ArbInterpolate(G4String);//
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G4String GetIntType();//
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void Calculate();//
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void SetBiasRndm(G4SPSRandomGenerator* a);//
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// method to re-set the histograms
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void ReSetHist(G4String);//
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// Set the verbosity level.
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void SetVerbosity(G4int a);//
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//x
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G4double GetWeight();
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G4double GetMonoEnergy(); //Mono-energteic energy
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G4double GetSE();// Standard deviation for Gaussion distrbution in energy
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G4double Getalpha(); // alpha (pow)
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G4double GetEzero(); // E0 (exp)
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G4double GetTemp(); // Temp (bbody,brem)
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G4double Getgrad(); // gradient and intercept for linear spectra
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G4double Getcept(); //
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G4PhysicsOrderedFreeVector GetUserDefinedEnergyHisto(); //
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G4PhysicsOrderedFreeVector GetArbEnergyHisto(); //
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G4double GenerateOne(G4ParticleDefinition*);
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G4double GetProbability (G4double);
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private:
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void LinearInterpolation();//
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void LogInterpolation();//
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void ExpInterpolation();//
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void SplineInterpolation();//
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void CalculateCdgSpectrum();//
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void CalculateBbodySpectrum();//
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void CalculateCPowSpectrum();//
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// The following methods generate energies according to the spectral
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// parameters defined above.
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void GenerateMonoEnergetic();//G4double& outputEne);//
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void GenerateBiasPowEnergies();//G4double& outputEne,G4double& outputWeight);//
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void GenerateGaussEnergies();//
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void GenerateBremEnergies();//
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void GenerateBbodyEnergies();//
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void GenerateCdgEnergies();//
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void GenUserHistEnergies();//
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void GenEpnHistEnergies();//
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void GenArbPointEnergies();//<<<<<<<<<<< DOES NOT WORK, REQUIRES UPDATE OF DATA MEMBERS.
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void GenerateExpEnergies(G4bool);//
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void GenerateLinearEnergies(G4bool);//
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void GeneratePowEnergies(G4bool);//
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void GenerateCPowEnergies();//
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// converts energy per nucleon to energy.
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void ConvertEPNToEnergy();
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void BBInitHists();//
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void CPInitHists();//
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private:
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G4String EnergyDisType; // energy dis type Variable - Mono,Lin,Exp,etc
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G4double weight; // particle weight //// NOT INVARIANT
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G4double MonoEnergy; //Mono-energteic energy
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G4double SE; // Standard deviation for Gaussion distrbution in energy
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//Non invariant data members become G4Cache
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G4double Emin, Emax; // emin and emax ////// NOT INVARIANT
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G4double alpha, Ezero;// alpha (pow), E0 (exp) ////// NOT INVARIANT
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G4double Temp; // Temp (bbody,brem)
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G4double biasalpha; // biased power index
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G4double grad, cept; // gradient and intercept for linear spectra ////// NOT INVARIANT
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G4double prob_norm; // normalisation factor use in calculate the probability
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G4bool Biased; // true - biased to power-law
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G4bool EnergySpec; // true - energy spectra, false - momentum spectra
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G4bool DiffSpec; // true - differential spec, false integral spec
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//G4bool ApplyRig; // false no rigidity cutoff, true then apply one
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//G4double ERig; // energy of rigidity cutoff
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G4PhysicsOrderedFreeVector UDefEnergyH; // energy hist data
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G4PhysicsOrderedFreeVector IPDFEnergyH;
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G4bool IPDFEnergyExist, IPDFArbExist, Epnflag;
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G4PhysicsOrderedFreeVector ArbEnergyH; // Arb x,y histogram
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G4PhysicsOrderedFreeVector IPDFArbEnergyH; // IPDF for Arb
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G4PhysicsOrderedFreeVector EpnEnergyH;
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G4double CDGhist[3]; // cumulative histo for cdg
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//AG: Begin edit to use STL vectors.
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// G4double BBHist[10001], Bbody_x[10001];
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std::vector<G4double>* BBHist;
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std::vector<G4double>* Bbody_x;
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G4bool BBhistInit;
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G4bool BBhistCalcd;
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// For cutoff power-law
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std::vector<G4double>* CPHist;
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std::vector<G4double>* CP_x;
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G4bool CPhistInit;
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G4bool CPhistCalcd;
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//AG: Edit here to use dynamic memory, will save space inless these functions are used.
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G4String IntType; // Interpolation type
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// G4double Arb_grad[1024], Arb_cept[1024]; // grad and cept for 1024 segments AG: Switched to DMA
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G4double* Arb_grad;
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G4double* Arb_cept;
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G4bool Arb_grad_cept_flag;
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// G4double Arb_alpha[1024], Arb_Const[1024]; // alpha and constants AG: Switched to DMA
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G4double* Arb_alpha;
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G4double* Arb_Const;
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G4bool Arb_alpha_Const_flag;
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// G4double Arb_ezero[1024]; // ezero AG: Switched to DMA
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G4double* Arb_ezero;
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G4bool Arb_ezero_flag;
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G4double ArbEmin, ArbEmax; // Emin and Emax for the whole arb distribution used primarily for debug.
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G4double particle_energy;
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G4SPSRandomGenerator* eneRndm;
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// Verbosity
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G4int verbosityLevel;
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G4PhysicsOrderedFreeVector ZeroPhysVector; // for re-set only
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std::vector<G4DataInterpolation*> SplineInt;//[1024]; // holds Spline stuff required for sampling
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G4DataInterpolation *Splinetemp; // holds a temp Spline used for calculating area
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G4Mutex mutex; // protect access to shared resources
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//Thread local data (non-invariant during event loop).
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//These are copied from master one at the beginning of generation
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//of each event
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struct threadLocal_t {
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G4double Emin;
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G4double Emax;
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G4double alpha;
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G4double Ezero;
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G4double grad;
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G4double cept;
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G4ParticleDefinition* particle_definition;
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G4double weight;
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G4double particle_energy;
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};
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G4Cache<threadLocal_t> threadLocalData;
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};
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#endif
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