GModelSpectralPlaw.hpp
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/***************************************************************************
* GModelSpectralPlaw.hpp - Spectral power law model class *
* ----------------------------------------------------------------------- *
* copyright (C) 2009-2011 by Jurgen Knodlseder *
* ----------------------------------------------------------------------- *
* *
* This program 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. *
* *
* This program 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 this program. If not, see <http://www.gnu.org/licenses/>. *
* *
***************************************************************************/
/**
* @file GModelSpectralPlaw.hpp
* @brief Power law spectral model class interface definition
* @author J. Knodlseder
*/
#ifndef GMODELSPECTRALPLAW_HPP
#define GMODELSPECTRALPLAW_HPP
/* __ Includes ___________________________________________________________ */
#include <string>
#include "GModelPar.hpp"
#include "GModelSpectral.hpp"
#include "GEnergy.hpp"
#include "GXmlElement.hpp"
/***********************************************************************//**
* @class GModelSpectralPlaw
*
* @brief Power law spectral model class
*
* This class implements a power law as the spectral component of the
* gamma-ray sky model. The power law is defined as
* \f[I(E)=norm (E/pivot)^{index}\f]
* where
* \f$norm\f$ is the normalization or prefactor,
* \f$pivot\f$ is the pivot energy, and
* \f$index\f$ is the spectral index.
***************************************************************************/
class GModelSpectralPlaw : public GModelSpectral {
public:
// Constructors and destructors
GModelSpectralPlaw(void);
explicit GModelSpectralPlaw(const double& norm, const double& index);
explicit GModelSpectralPlaw(const GXmlElement& xml);
GModelSpectralPlaw(const GModelSpectralPlaw& model);
virtual ~GModelSpectralPlaw(void);
// Operators
virtual GModelSpectralPlaw& operator=(const GModelSpectralPlaw& model);
// Implemented pure virtual methods
virtual void clear(void);
virtual GModelSpectralPlaw* clone(void) const;
virtual std::string type(void) const { return "PowerLaw"; }
virtual double eval(const GEnergy& srcEng) const;
virtual double eval_gradients(const GEnergy& srcEng) const;
virtual double flux(const GEnergy& emin, const GEnergy& emax) const;
virtual double eflux(const GEnergy& emin, const GEnergy& emax) const;
virtual GEnergy mc(const GEnergy& emin, const GEnergy& emax, GRan& ran) const;
virtual void read(const GXmlElement& xml);
virtual void write(GXmlElement& xml) const;
virtual std::string print(void) const;
// Other methods
void autoscale(void);
double norm(void) const { return m_norm.real_value(); }
double index(void) const { return m_index.real_value(); }
double pivot(void) const { return m_pivot.real_value(); }
protected:
// Protected methods
void init_members(void);
void copy_members(const GModelSpectralPlaw& model);
void free_members(void);
// Protected members
GModelPar m_norm; //!< Normalization factor
GModelPar m_index; //!< Spectral index
GModelPar m_pivot; //!< Pivot energy
};
#endif /* GMODELSPECTRALPLAW_HPP */