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9.6.p02
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geant4_9_6_p02
source
processes
electromagnetic
xrays
include
G4SynchrotronRadiation.hh
Go to the documentation of this file.
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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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// $Id$
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//
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// ------------------------------------------------------------
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// GEANT 4 class header file
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// CERN Geneva Switzerland
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//
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//
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// History:
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// 21-5-98 1 version , V. Grichine
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// 28-05-01, V.Ivanchenko minor changes to provide ANSI -wall compilation
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// 23-05-06, H. Burkhardt: Energy spectrum from function rather than table
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//
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//
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// ------------------------------------------------------------
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#ifndef G4SynchrotronRadiation_h
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#define G4SynchrotronRadiation_h 1
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#include "
G4ios.hh
"
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#include "
globals.hh
"
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#include "
Randomize.hh
"
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#include "
G4VDiscreteProcess.hh
"
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#include "
G4TransportationManager.hh
"
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#include "
G4FieldManager.hh
"
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#include "
G4Field.hh
"
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#include "
G4ThreeVector.hh
"
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#include "
G4PropagatorInField.hh
"
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#include "
G4Track.hh
"
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#include "
G4Step.hh
"
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#include "
G4Gamma.hh
"
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#include "
G4Electron.hh
"
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#include "
G4Positron.hh
"
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class
G4SynchrotronRadiation
:
public
G4VDiscreteProcess
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{
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public
:
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G4SynchrotronRadiation
(
const
G4String
& pName =
"SynRad"
,
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G4ProcessType
type =
fElectromagnetic
);
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virtual
~G4SynchrotronRadiation
();
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G4double
GetMeanFreePath
(
const
G4Track
& track,
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G4double
previousStepSize,
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G4ForceCondition
*
condition
);
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G4VParticleChange
*
PostStepDoIt
(
const
G4Track
& track,
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const
G4Step
&
Step
);
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G4double
GetPhotonEnergy
(
const
G4Track
& trackData,
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const
G4Step
& stepData );
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G4double
GetRandomEnergySR
(
G4double
,
G4double
);
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G4double
InvSynFracInt
(
G4double
x
);
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G4double
Chebyshev
(
G4double
a
,
G4double
b
,
const
G4double
c
[],
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G4int
n
,
G4double
x);
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G4bool
IsApplicable
(
const
G4ParticleDefinition
&);
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void
BuildPhysicsTable
(
const
G4ParticleDefinition
& );
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void
PrintInfoDefinition
();
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private
:
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G4SynchrotronRadiation
& operator=(
const
G4SynchrotronRadiation
&
right
);
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G4SynchrotronRadiation
(
const
G4SynchrotronRadiation
&);
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G4ParticleDefinition
* theGamma;
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const
G4ParticleDefinition
* theElectron;
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const
G4ParticleDefinition
* thePositron;
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G4double
fLambdaConst;
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G4double
fEnergyConst;
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G4PropagatorInField
* fFieldPropagator;
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};
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inline
G4bool
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G4SynchrotronRadiation::IsApplicable
(
const
G4ParticleDefinition
& particle )
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{
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return
( ( &particle == (
const
G4ParticleDefinition
*)theElectron ) ||
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( &particle == (
const
G4ParticleDefinition
*)thePositron ) );
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}
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inline
G4double
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G4SynchrotronRadiation::Chebyshev
(
G4double
a
,
G4double
b
,
const
G4double
c
[],
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G4int
n
,
G4double
x
)
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{
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G4double
y
;
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G4double
y2
=2.0*(y=(2.0*x-a-
b
)/(b-a));
// Change of variable.
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G4double
d
=0,dd=0;
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for
(
G4int
j=n-1;j>=1;--j)
// Clenshaw's recurrence.
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{
G4double
sv=
d
;
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d=y2*d-dd+c[j];
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dd=sv;
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}
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return
y*d-dd+0.5*c[0];
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}
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#endif // end of G4SynchrotronRadiation.hh
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