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G4SmpNVel.cc
Go to the documentation of this file.
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// ********************************************************************
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//
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//
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// This software was developed by Lawrence Livermore National Laboratory.
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//
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// Redistribution and use in source and binary forms, with or without
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// modification, are permitted provided that the following conditions are met:
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// 1. Redistributions of source code must retain the above copyright notice,
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// derived from this software without specific prior written permission.
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// THIS SOFTWARE IS PROVIDED BY THE AUTHOR ``AS IS'' AND ANY EXPRESS OR IMPLIED
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// ADVISED OF THE POSSIBILITY OF SUCH DAMAGE.
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//
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// Copyright (c) 2006 The Regents of the University of California.
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// All rights reserved.
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// UCRL-CODE-224807
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//
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//
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// $Id: G4SmpNVel.cc 67966 2013-03-13 09:38:38Z gcosmo $
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//
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#include <cmath>
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#include "
G4fissionEvent.hh
"
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G4double
G4fissionEvent::G4SmpNVel(
G4double
eng,
G4double
* cosdiru,
G4double
* cosdirv,
G4double
* cosdirw) {
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/*
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Description
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Knowing the neutron energy, determine its velocity and the 3 direction cosines
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*/
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/*
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Input
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eng - energy of neutron
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Output
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- velocity
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- 3 components of the neutron velocity
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in arguments (cosdiru, cosdirv, cosdirw)
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*/
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const
G4double
rme = 939.56563;
/* Rest Mass Energy equivalents for neutrons (MeV) */
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const
G4double
cspeed = 2.99792458e+8;
/* speed of light (m/sec) */
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G4double
vel;
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G4double
ratio = eng/rme;
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if
(ratio > 1.e-8) {
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/* Relativistic vel calculation */
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vel = cspeed*std::sqrt(1.-rme*rme/((rme+eng)*(rme+eng)));
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}
else
{
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/* Non-relativistic vel calculation */
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vel = cspeed*std::sqrt(2.*eng/rme);
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}
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G4SmpIsoDir(cosdiru, cosdirv, cosdirw);
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return
vel;
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}
G4fissionEvent.hh
G4double
double G4double
Definition:
G4Types.hh:76
source
geant4.10.03.p03
source
processes
hadronic
models
fission
src
G4SmpNVel.cc
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