G4SynchrotronRadiation.hh

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// $Id: G4SynchrotronRadiation.hh 74582 2013-10-15 12:06:25Z gcosmo $
//
// ------------------------------------------------------------
//      GEANT 4 class header file
//      CERN Geneva Switzerland
//
//
//      History:
//      21-5-98  1 version , V. Grichine
//      28-05-01, V.Ivanchenko minor changes to provide ANSI -wall compilation
//      23-05-06, H. Burkhardt: Energy spectrum from function rather than table
//
//
// ------------------------------------------------------------

#ifndef G4SynchrotronRadiation_h
#define G4SynchrotronRadiation_h 1

#include "G4ios.hh"
#include "globals.hh"
#include "Randomize.hh"
#include "G4VDiscreteProcess.hh"
#include "G4TransportationManager.hh"
#include "G4FieldManager.hh"
#include "G4Field.hh"
#include "G4ThreeVector.hh"
#include "G4PropagatorInField.hh"

#include "G4Track.hh"
#include "G4Step.hh"

#include "G4Gamma.hh"
#include "G4Electron.hh"
#include "G4Positron.hh"

class G4VEmAngularDistribution;

class G4SynchrotronRadiation : public G4VDiscreteProcess
{
public:

  G4SynchrotronRadiation(const G4String& pName = "SynRad",
                         G4ProcessType type = fElectromagnetic);

  virtual ~G4SynchrotronRadiation();

  virtual G4double GetMeanFreePath( const G4Track& track,
                                    G4double previousStepSize,
                                    G4ForceCondition* condition );

  virtual G4VParticleChange *PostStepDoIt( const G4Track& track,
                                           const G4Step& Step    );

  G4double GetPhotonEnergy( const G4Track& trackData,
                               const G4Step&  stepData      );

  G4double GetRandomEnergySR( G4double, G4double );

  G4double InvSynFracInt(G4double x);
  G4double Chebyshev(G4double a,G4double b,const G4double c[],
                     G4int n, G4double x);

  virtual G4bool IsApplicable(const G4ParticleDefinition&);
  virtual void BuildPhysicsTable(const G4ParticleDefinition& );
  virtual void PrintInfoDefinition();

  void SetAngularGenerator(G4VEmAngularDistribution* p);

private:

  G4SynchrotronRadiation & operator=(const G4SynchrotronRadiation &right);
  G4SynchrotronRadiation(const G4SynchrotronRadiation&);

  G4VEmAngularDistribution*   genAngle;

  G4ParticleDefinition*       theGamma;
  const G4ParticleDefinition* theElectron;
  const G4ParticleDefinition* thePositron;

  G4double fLambdaConst;
  G4double fEnergyConst;

  G4PropagatorInField* fFieldPropagator;
  G4bool FirstTime;
  G4bool FirstTime1;
};


inline G4double 
G4SynchrotronRadiation::Chebyshev(G4double a, G4double b, const G4double c[],
                                  G4int n, G4double x)
{
  G4double y;
  G4double y2=2.0*(y=(2.0*x-a-b)/(b-a)); // Change of variable.
  G4double d=0,dd=0;
  for (G4int j=n-1;j>=1;--j) // Clenshaw's recurrence.
  { G4double sv=d;
        d=y2*d-dd+c[j];
        dd=sv;
  }
  return y*d-dd+0.5*c[0];
}

#endif  // end of G4SynchrotronRadiation.hh