Page MenuHomeHEPForge
Files F19244250

EvtBtoXsgammaKagan.hh
No OneTemporary
Actions

Size
5 KB
Referenced Files
None
Subscribers
None

EvtBtoXsgammaKagan.hh
View Options

/***********************************************************************
* Copyright 1998-2020 CERN for the benefit of the EvtGen authors *
* *
* This file is part of EvtGen. *
* *
* EvtGen is free software: you can redistribute it and/or modify *
* it under the terms of the GNU General Public License as published by *
* the Free Software Foundation, either version 3 of the License, or *
* (at your option) any later version. *
* *
* EvtGen is distributed in the hope that it will be useful, *
* but WITHOUT ANY WARRANTY; without even the implied warranty of *
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the *
* GNU General Public License for more details. *
* *
* You should have received a copy of the GNU General Public License *
* along with EvtGen. If not, see <https://www.gnu.org/licenses/>. *
***********************************************************************/
#ifndef EVTBTOXSGAMMAKAGAN_HH
#define EVTBTOXSGAMMAKAGAN_HH
#include "EvtGenModels/EvtBtoXsgammaAbsModel.hh"
#include <vector>
// Description:
// Implimentation of the Kagan-Neubert model for non-resonant
// B->Xs,gamma decays.
// Description:
// Routine to perform two-body non-resonant B->Xs,gamma decays.
// The X_s mass spectrum generated is based on the Kagan-Neubert model.
// See hep-ph/9805303 for the model details and input parameters.
//
// The input parameters are 1:fermi_model, 2:mB, 3:mb, 4:mu, 5:lam1,
// 6:delta, 7:z, 8:nIntervalS, 9:nIntervalmH. Choosing fermi_model=1
// uses an exponential shape function, fermi_model=2 uses a gaussian
// shape function and fermi_model=3 a roman shape function. The complete mass
// spectrum for a given set of input parameters is calculated from
// scratch in bins of nIntervalmH. The s22, s27 and s28 coefficients are calculated
// in bins of nIntervalS. As the program includes lots of integration, the
// theoretical hadronic mass spectra is computed for the first time
// the init method is called. Then, all the other times (eg if we want to decay a B0
// as well as an anti-B0) the vector mass info stored the first time is used again.
class EvtBtoXsgammaKagan : public EvtBtoXsgammaAbsModel {
public:
void init( int, double* ) override;
void computeHadronicMass( int, double* );
void getDefaultHadronicMass();
double GetMass( int code ) override;
double CalcAlphaS( double );
void CalcWilsonCoeffs();
void CalcDelta();
double Fz( double );
private:
//Input parameters
double _mb;
double _mB;
double _delta;
double _nIntervalS;
double _nIntervalmH;
double _lambdabar;
double _lam1;
double _mHmin;
double _mHmax;
//Other parameters
double _r7;
double _gam77;
double _gam27;
double _gam87;
double _beta0;
double _beta1;
double _alphasmZ;
double _mZ;
double _z;
double _fz;
double _lam2;
double _kappabar;
double _rer2;
double _rer8;
double _kSLemmu;
double _mW;
double _mt;
double _ms;
double _mu;
double _c2mu;
double _c70mu;
double _c80mu;
double _c71mu;
double _c7emmu;
double _cDeltatot;
double _alpha;
double _alphasmW;
double _alphasmt;
double _alphasmu;
double _alphasmubar;
double _etamu;
std::vector<double> _mHVect;
static double ReG( double );
static double ImG( double );
static double s77( double );
static double s88( double, double, double );
static double s78( double );
static double s22Func( double var, const std::vector<double>& coeffs );
static double s27Func( double var, const std::vector<double>& coeffs );
static double Delta( double, double );
static double DeltaFermiFunc( double, const std::vector<double>& coeffs1,
const std::vector<double>& coeffs2,
const std::vector<double>& coeffs3 );
static double s77FermiFunc( double, const std::vector<double>& coeffs1,
const std::vector<double>& coeffs2 );
static double s88FermiFunc( double, const std::vector<double>& coeffs1,
const std::vector<double>& coeffs2,
const std::vector<double>& coeffs3 );
static double s78FermiFunc( double, const std::vector<double>& coeffs1,
const std::vector<double>& coeffs2 );
static double s22FermiFunc( double, std::vector<double>& coeffs );
static double s27FermiFunc( double, std::vector<double>& coeffs );
static double s28FermiFunc( double, std::vector<double>& coeffs );
static double GetArrayVal( double, double, double, double,
std::vector<double> );
static double sFermiFunc( double, const std::vector<double>& coeffs1,
const std::vector<double>& coeffs2,
const std::vector<double>& coeffs3,
const std::vector<double>& coeffs4 );
static double FermiFunc( double, const std::vector<double>& coeffs );
static double diLogFunc( double );
static double diLogMathematica( double );
std::vector<double> massHad, brHad;
static double intervalMH;
static bool bbprod;
};
#endif

File Metadata

Mime Type
text/x-c
Expires
Tue, Sep 30, 4:40 AM (15 h, 34 m)
Storage Engine
blob
Storage Format
Raw Data
Storage Handle
6531751
Default Alt Text
EvtBtoXsgammaKagan.hh (5 KB)

Event Timeline

HEPForge.org · .