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source
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electromagnetic
xrays
include
G4GammaXTRadiator.hh
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//
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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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// $Id: G4GammaXTRadiator.hh 97385 2016-06-02 09:59:53Z gcosmo $
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//
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//
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//
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// Rough process describing a radiator of X-ray transition radiation.
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// Thicknesses of plates and gas gaps are distributed according to gamma
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// distribution. x are thicknesses of plates or gas gaps:
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//
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// p(x) = (alpha/<x>)^alpha * x^(alpha-1) * std::exp(-alpha*x/<x>) / G(alpha)
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//
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// G(alpha) is Euler's gamma function.
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// Plates have mean <x> = fPlateThick > 0 and power alpha = fAlphaPlate > 0 :
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// Gas gaps have mean <x> = fGasThick > 0 and power alpha = fAlphaGas > 0 :
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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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// 21.01.02 V. Grichine, first version
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//
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#ifndef G4GammaXTRadiator_h
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#define G4GammaXTRadiator_h 1
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#include "
G4VXTRenergyLoss.hh
"
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class
G4GammaXTRadiator
:
public
G4VXTRenergyLoss
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{
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public
:
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explicit
G4GammaXTRadiator
(
G4LogicalVolume
*anEnvelope,
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G4double
,
G4double
,
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G4Material
*,
G4Material
*,
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G4double
,
G4double
,
G4int
,
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const
G4String
& processName =
"XTRgammaRadiator"
);
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~G4GammaXTRadiator
();
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// Pure virtual function from base class
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G4double
GetStackFactor
(
G4double
energy
,
G4double
gamma,
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G4double
varAngle)
override
;
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private
:
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};
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#endif
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G4GammaXTRadiator::GetStackFactor
G4double GetStackFactor(G4double energy, G4double gamma, G4double varAngle) override
Definition:
G4GammaXTRadiator.cc:79
G4GammaXTRadiator::G4GammaXTRadiator
G4GammaXTRadiator(G4LogicalVolume *anEnvelope, G4double, G4double, G4Material *, G4Material *, G4double, G4double, G4int, const G4String &processName="XTRgammaRadiator")
Definition:
G4GammaXTRadiator.cc:41
G4Material
Definition:
G4Material.hh:121
G4String
Definition:
examples/extended/parallel/TopC/ParN02/AnnotatedFiles/G4String.hh:45
G4GammaXTRadiator::~G4GammaXTRadiator
~G4GammaXTRadiator()
Definition:
G4GammaXTRadiator.cc:63
G4VXTRenergyLoss
Definition:
G4VXTRenergyLoss.hh:74
G4double
double G4double
Definition:
G4Types.hh:76
energy
double energy
Definition:
plottest35.C:25
G4int
int G4int
Definition:
G4Types.hh:78
G4LogicalVolume
Definition:
G4LogicalVolume.hh:190
G4GammaXTRadiator
Definition:
G4GammaXTRadiator.hh:57
G4VXTRenergyLoss.hh
다음에 의해 생성됨 :
1.8.5