Gabriele Cosmo
63 lines
2.5 KiB
C++
63 lines
2.5 KiB
C++
//
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// ********************************************************************
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// * DISCLAIMER *
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// * *
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// * The following disclaimer summarizes all the specific disclaimers *
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// * of contributors to this software. The specific disclaimers,which *
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// * govern, are listed with their locations in: *
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// * http://cern.ch/geant4/license *
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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. *
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// * *
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// * This code implementation is the intellectual property of the *
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// * GEANT4 collaboration. *
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// * By copying, distributing or modifying the Program (or any work *
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// * based on the Program) you indicate your acceptance of this *
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// * statement, and all its terms. *
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// ********************************************************************
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//
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//
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//
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//
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///////////////////////////////////////////////////////////////////////////
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//
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// Model describing a regular radiator of X-ray transition radiation.
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// It is Garibian like model for XTR after radiator
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// Thicknesses of plates and gas gaps are fixed.
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// We suppose that:
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// formation zone ~ mean thickness << absorption length
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// for each material and in the range 1-100 keV. This allows us to simplify
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// interference effects in radiator stack (GetStackFactor method).
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//
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//
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// History:
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// 10.10.05 V. Grichine, first version
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//
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#ifndef G4XTRRegularRadModel_h
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#define G4XTRRegularRadModel_h 1
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#include "G4VXTRenergyLoss.hh"
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class G4XTRRegularRadModel : public G4XTRenergyLoss
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{
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public:
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G4XTRRegularRadModel (G4LogicalVolume *anEnvelope,G4Material*,G4Material*,
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G4double,G4double,G4int,
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const G4String & processName = "XTRegularModel");
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~G4XTRRegularRadModel ();
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// Pure virtual function from base class
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G4double GetStackFactor( G4double energy, G4double gamma, G4double varAngle);
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};
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#endif
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