Gabriele Cosmo
100 lines
3.4 KiB
C++
100 lines
3.4 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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// $Id$
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//
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//---------------------------------------------------------------------------
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//
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// ClassName: QGSP_INCLXX
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//
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// Author: 2011 P. Kaitaniemi
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//
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// Modified:
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// D. Mancusi 23.03.2012 Extended INCL++ to incident heavy ions up to 16O
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//
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//----------------------------------------------------------------------------
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//
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#ifndef TQGSP_INCLXX_h
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#define TQGSP_INCLXX_h 1
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#include <CLHEP/Units/SystemOfUnits.h>
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#include "globals.hh"
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#include "G4VModularPhysicsList.hh"
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#include "CompileTimeConstraints.hh"
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/**
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* <h1>Physics list QGSP_INCLXX</h1>
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*
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* <h2>Use case</h2>
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* This list is mainly intended for use with energies less than 3
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* GeV. This is useful for e.g. spallation studies and Accelerator
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* Driven Systems (ADS) applications.
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*
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* <h2>Usage</h2>
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* The physics list can be activated in a simulation application by
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* giving it as part of the user initialization to the run manager:
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* @code
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* G4RunManager *runManager = new G4RunManager;
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* G4VUserPhysicsList *physics = new QGSP_INCLXX;
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* runManager->SetUserInitialization(physics);
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* @endcode
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*
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* <h2>Hadronic models</h2>
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* The list uses INCL++ intra-nuclear cascade model in the energy range 0 - 3
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* GeV. Between 3 - 15 GeV Bertini cascade is used and above 15 GeV the high
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* energy QGSP model.
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*
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* @see HadronPhysicsQGSP_INCLXX
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* @see G4INCLXXProtonBuilder
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* @see G4INCLXXNeutronBuilder
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* @see G4INCLXXPiKBuilder
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* @see G4IonINCLXXPhysics
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*/
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template<class T>
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class TQGSP_INCLXX: public T
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{
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public:
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TQGSP_INCLXX(G4int ver = 1);
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virtual ~TQGSP_INCLXX();
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public:
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// SetCuts()
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virtual void SetCuts();
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private:
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enum {ok = CompileTimeConstraints::IsA<T, G4VModularPhysicsList>::ok };
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};
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#include "QGSP_INCLXX.icc"
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typedef TQGSP_INCLXX<G4VModularPhysicsList> QGSP_INCLXX;
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// 2011 by P. Kaitaniemi
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#endif
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