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// $Id: QGSP_INCL_ABLA.hh,v 1.1 2009/07/19 18:24:03 kaitanie Exp $
// GEANT4 tag $Name: geant4-09-03-cand-03 $
//
//---------------------------------------------------------------------------
//
// ClassName:   QGSP_INCL_ABLA
//
// Author: 2002 J.P. Wellisch
//
// Modified:
//
//----------------------------------------------------------------------------
//
#ifndef TQGSP_INCL_ABLA_h
#define TQGSP_INCL_ABLA_h 1

#include "G4VModularPhysicsList.hh"
#include "globals.hh"
#include "CompileTimeConstraints.hh"

/**
 * <h1>Physics list QGSP_INCL_ABLA</h1>
 *
 * <h2>Use case</h2>
 * This list is mainly intended for use with energies less than 3
 * GeV. This is useful for e.g. spallation studies and Accelerator
 * Driven Systems (ADS) applications.
 *
 * <h2>Usage</h2>
 * The physics list can be activated in a simulation application by
 * giving it as part of the user initialization to the run manager:
 * @code
 * G4RunManager *runManager = new G4RunManager;
 * G4VUserPhysicsList *physics = new QGSP_INCL_ABLA;
 * runManager->SetUserInitialization(physics);
 * @endcode
 *
 * <h2>Hadronic models</h2>
 * The list uses INCL/ABLA intra-nuclear cascade and de-excitation
 * models in the energy range 0 - 3 GeV. Between 3 - 15 GeV Bertini
 * cascade is used and above 15 GeV the high energy QGSP model.
 *
 * @see HadronPhysicsQGSP_INCL_ABLA
 * @see G4InclAblaProtonBuilder
 * @see G4InclAblaNeutronBuilder
 * @see G4InclAblaPiKBuilder
 */
template<class T>
class TQGSP_INCL_ABLA: public T
{
public:
  TQGSP_INCL_ABLA(G4int ver = 1);
  virtual ~TQGSP_INCL_ABLA();
  
public:
  // SetCuts() 
  virtual void SetCuts();

private:
  enum {ok = CompileTimeConstraints::IsA<T, G4VModularPhysicsList>::ok };
};

#include "QGSP_INCL_ABLA.icc"
typedef TQGSP_INCL_ABLA<G4VModularPhysicsList> QGSP_INCL_ABLA;

// 2002 by J.P. Wellisch

#endif