GModelSpectralPlawEnergyFlux.cpp

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/***************************************************************************
 *   GModelSpectralPlawEnergyFlux.cpp - Spectral power law model class     *
 * ----------------------------------------------------------------------- *
 *  copyright (C) 2016-2021 by Michael Mayer                               *
 * ----------------------------------------------------------------------- *
 *                                                                         *
 *  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 GModelSpectralPlawEnergyFlux.cpp
 * @brief Energy flux normalized power law spectral model class implementation
 * @author Michael Mayer
 */
 
/* __ Includes ___________________________________________________________ */
#ifdef HAVE_CONFIG_H
#include <config.h>
#endif
#include <cmath>
#include "GException.hpp"
#include "GTools.hpp"
#include "GMath.hpp"
#include "GRan.hpp"
#include "GModelSpectralPlawEnergyFlux.hpp"
#include "GModelSpectralRegistry.hpp"
 
/* __ Constants __________________________________________________________ */
 
/* __ Globals ____________________________________________________________ */
const GModelSpectralPlawEnergyFlux g_spectral_plaw_eflux_seed("PowerLaw",
                                                              "EnergyFlux",
                                                              "Index",
                                                              "LowerLimit",
                                                              "UpperLimit");
const GModelSpectralRegistry       g_spectral_plaw_eflux_registry(&g_spectral_plaw_eflux_seed);
 
/* __ Method name definitions ____________________________________________ */
#define G_FLUX       "GModelSpectralPlawEnergyFlux::flux(GEnergy&, GEnergy&)"
#define G_EFLUX     "GModelSpectralPlawEnergyFlux::eflux(GEnergy&, GEnergy&)"
#define G_MC  "GModelSpectralPlawEnergyFlux::mc(GEnergy&, GEnergy&, GTime&, "\
                                                                     "GRan&)"
#define G_READ             "GModelSpectralPlawEnergyFlux::read(GXmlElement&)"
#define G_WRITE           "GModelSpectralPlawEnergyFlux::write(GXmlElement&)"
 
/* __ Macros _____________________________________________________________ */
 
/* __ Coding definitions _________________________________________________ */
 
/* __ Debug definitions __________________________________________________ */
 
 
/*==========================================================================
 =                                                                         =
 =                        Constructors/destructors                         =
 =                                                                         =
 ==========================================================================*/
 
/***********************************************************************//**
 * @brief Void constructor
 ***************************************************************************/
GModelSpectralPlawEnergyFlux::GModelSpectralPlawEnergyFlux(void) :
                              GModelSpectral()
{
    // Initialise members
    init_members();
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Model type and parameter name constructor
 *
 * @param[in] type Model type.
 * @param[in] eflux Name of energy flux parameter.
 * @param[in] index Name of index parameter.
 * @param[in] emin Name of emin parameter.
 * @param[in] emax Name of emax parameter.
 ***************************************************************************/
GModelSpectralPlawEnergyFlux::GModelSpectralPlawEnergyFlux(const std::string& type,
                                                           const std::string& eflux,
                                                           const std::string& index,
                                                           const std::string& emin,
                                                           const std::string& emax) :
                              GModelSpectral()
{
    // Initialise members
    init_members();
 
    // Set model type
    m_type = type;
 
    // Set parameter names
    m_eflux.name(eflux);
    m_index.name(index);
    m_emin.name(emin);
    m_emax.name(emax);
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Constructor
 *
 * @param[in] eflux Energy flux (erg/cm2/s).
 * @param[in] index Power law index.
 * @param[in] emin Minimum energy.
 * @param[in] emax Maximum energy.
 *
 * Construct a spectral power law from the
 * - energy flux (in erg/cm2/s),
 * - spectral index,
 * - minimum energy and
 * - maximum energy.
 ***************************************************************************/
GModelSpectralPlawEnergyFlux::GModelSpectralPlawEnergyFlux(const double&  eflux,
                                                           const double&  index,
                                                           const GEnergy& emin,
                                                           const GEnergy& emax) :
                              GModelSpectral()
{
    // Initialise members
    init_members();
 
    // Set parameters
    m_eflux.value(eflux);
    m_index.value(index);
    m_emin.value(emin.MeV());
    m_emax.value(emax.MeV());
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief XML constructor
 *
 * @param[in] xml XML element.
 *
 * Constructs energy flux normalized power law spectral model by extracting
 * information from an XML element.
 ***************************************************************************/
GModelSpectralPlawEnergyFlux::GModelSpectralPlawEnergyFlux(const GXmlElement& xml) :
                              GModelSpectral()
{
    // Initialise members
    init_members();
 
    // Read information from XML element
    read(xml);
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Copy constructor
 *
 * @param[in] model Spectral power law model.
 ***************************************************************************/
GModelSpectralPlawEnergyFlux::GModelSpectralPlawEnergyFlux(const GModelSpectralPlawEnergyFlux& model) :
                              GModelSpectral(model)
{
    // Initialise members
    init_members();
 
    // Copy members
    copy_members(model);
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Destructor
 ***************************************************************************/
GModelSpectralPlawEnergyFlux::~GModelSpectralPlawEnergyFlux(void)
{
    // Free members
    free_members();
 
    // Return
    return;
}
 
 
/*==========================================================================
 =                                                                         =
 =                                Operators                                =
 =                                                                         =
 ==========================================================================*/
 
/***********************************************************************//**
 * @brief Assignment operator
 *
 * @param[in] model Spectral power law model.
 * @return Spectral power law model.
 ***************************************************************************/
GModelSpectralPlawEnergyFlux& GModelSpectralPlawEnergyFlux::operator=(const GModelSpectralPlawEnergyFlux& model)
{
    // Execute only if object is not identical
    if (this != &model) {
 
        // Copy base class members
        this->GModelSpectral::operator=(model);
 
        // Free members
        free_members();
 
        // Initialise members
        init_members();
 
        // Copy members
        copy_members(model);
 
    } // endif: object was not identical
 
    // Return
    return *this;
}
 
 
/*==========================================================================
 =                                                                         =
 =                              Public methods                             =
 =                                                                         =
 ==========================================================================*/
 
/***********************************************************************//**
 * @brief Clear power law model
 ***************************************************************************/
void GModelSpectralPlawEnergyFlux::clear(void)
{
    // Free class members (base and derived classes, derived class first)
    free_members();
    this->GModelSpectral::free_members();
 
    // Initialise members
    this->GModelSpectral::init_members();
    init_members();
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Clone power law model
 *
 * @return Pointer to deep copy of power law model
 ***************************************************************************/
GModelSpectralPlawEnergyFlux* GModelSpectralPlawEnergyFlux::clone(void) const
{
    // Clone power law model
    return new GModelSpectralPlawEnergyFlux(*this);
}
 
 
/***********************************************************************//**
 * @brief Evaluate function
 *
 * @param[in] srcEng True photon energy.
 * @param[in] srcTime True photon arrival time.
 * @param[in] gradients Compute gradients?
 * @return Model value (ph/cm2/s/MeV).
 *
 * Computes
 *
 * \f[
 *    S_{\rm E}(E | t) = {\tt m\_eflux}
 *    \frac{{\tt m\_index}+2}
 *         {{\tt e\_max}^{{\tt m\_index}+2} -
 *          {\tt e\_min}^{{\tt m\_index}+2}}
 *    E^{\tt m\_index}
 * \f]
 *
 * for \f${\tt m\_index} \ne -2\f$ and
 *
 * \f[
 *    S_{\rm E}(E | t) = 
 *    \frac{{\tt m\_eflux}}
 *         {\log {\tt e\_max} - \log {\tt e\_min}}
 *    E^{\tt m\_index}
 * \f]
 *
 * for \f${\tt m\_index} = -2\f$, where
 * - \f${\tt e\_min}\f$ is the minimum energy of an interval,
 * - \f${\tt e\_max}\f$ is the maximum energy of an interval,
 * - \f${\tt m\_eflux}\f$ is the energy flux between
 *   \f${\tt e\_min}\f$ and \f${\tt e\_max}\f$, and
 * - \f${\tt m\_index}\f$ is the spectral index.
 *
 * If the @p gradients flag is true the method will also compute the
 * partial derivatives of the model with respect to the parameters using
 *
 * \f[
 *    \frac{\delta S_{\rm E}(E | t)}{\delta {\tt m\_eflux}} =
 *      \frac{S_{\rm E}(E | t)}{{\tt m\_eflux}}
 * \f]
 *
 * \f[
 *    \frac{\delta S_{\rm E}(E | t)}{\delta {\tt m\_index}} =
 *      S_{\rm E}(E | t) \,
 *      \left( \frac{1}{{\tt m\_index}+2} -
 *             \frac{\log({\tt e\_max}) {\tt e\_max}^{{\tt m\_index}+2} -
 *                   \log({\tt e\_min}) {\tt e\_min}^{{\tt m\_index}+2}}
 *                        {{\tt e\_max}^{{\tt m\_index}+2} -
 *                         {\tt e\_min}^{{\tt m\_index}+2}}
 *                 + \ln(E) \right)
 * \f]
 *
 * for \f${\tt m\_index} \ne -2\f$ and
 *
 * \f[
 *    \frac{\delta S_{\rm E}(E | t)}{\delta {\tt m\_index}} =
 *      S_{\rm E}(E | t) \, \ln(E)
 * \f]
 *
 * for \f${\tt m\_index} = -2\f$.
 *
 * No partial derivatives are supported for the energy boundaries.
 ***************************************************************************/
double GModelSpectralPlawEnergyFlux::eval(const GEnergy& srcEng,
                                          const GTime&   srcTime,
                                          const bool&    gradients) const
{
    // Update precomputed values
    update(srcEng);
 
    // Compute function value
    double value = m_eflux.value() * gammalib::erg2MeV * m_norm * m_power;
 
    // Optionally compute gradients
    if (gradients) {
 
        // Compute partial derivatives of the parameter values
        double g_eflux = (m_eflux.is_free() && m_eflux.factor_value() != 0.0)
                         ? g_eflux = value / m_eflux.factor_value()
                         : 0.0;
        double g_index = (m_index.is_free())
                         ? value * (m_g_norm + gammalib::ln10 *
                                    srcEng.log10MeV()) * m_index.scale()
                         : 0.0;
 
        // Set gradients
        m_eflux.factor_gradient(g_eflux);
        m_index.factor_gradient(g_index);
 
    } // endif: gradient computation was requested
 
    // Compile option: Check for NaN/Inf
    #if defined(G_NAN_CHECK)
    if (gammalib::is_notanumber(value) || gammalib::is_infinite(value)) {
        std::cout << "*** ERROR: GModelSpectralPlawEnergyFlux::eval";
        std::cout << "(srcEng=" << srcEng;
        std::cout << ", srcTime=" << srcTime << "):";
        std::cout << " NaN/Inf encountered";
        std::cout << " (value=" << value;
        std::cout << ", eflux=" << eflux();
        std::cout << ", m_norm=" << m_norm;
        std::cout << ", m_power=" << m_power;
        std::cout << ")" << std::endl;
    }
    #endif
 
    // Return
    return value;
}
 
 
/***********************************************************************//**
 * @brief Returns model photon flux between [emin, emax] (units: ph/cm2/s)
 *
 * @param[in] emin Minimum photon energy.
 * @param[in] emax Minimum photon energy.
 * @return Photon flux (ph/cm2/s).
 *
 * Computes
 *
 * \f[
 *    \int_{\tt emin}^{\tt emax} S_{\rm E}(E | t) dE
 * \f]
 *
 * where
 * - [@p emin, @p emax] is an energy interval, and
 * - \f$S_{\rm E}(E | t)\f$ is the spectral model (ph/cm2/s/MeV).
 ***************************************************************************/
double GModelSpectralPlawEnergyFlux::flux(const GEnergy& emin,
                                          const GEnergy& emax) const
{
    // Initialise flux
    double flux = 0.0;
 
    // Compute only if integration range is valid
    if (emin < emax) {
 
        // Compute power law normalization
        double norm = 0.0;
        if (index() != -2.0) {
            double gamma        = m_index.value() + 2.0;
            double pow_ref_emin = std::pow(this->emin().MeV(), gamma);
            double pow_ref_emax = std::pow(this->emax().MeV(), gamma);
            norm = m_eflux.value() * gammalib::erg2MeV * gamma /
                   (pow_ref_emax - pow_ref_emin);
        }
        else {
            double log_ref_emin = std::log(this->emin().MeV());
            double log_ref_emax = std::log(this->emax().MeV());
            norm = m_eflux.value() * gammalib::erg2MeV /
                   (log_ref_emax - log_ref_emin);
        }
 
        // Compute photon flux
        if (index() != -1.0) {
            double gamma    = m_index.value() + 1.0;
            double pow_emin = std::pow(emin.MeV(), gamma);
            double pow_emax = std::pow(emax.MeV(), gamma);
            flux = norm / gamma * (pow_emax - pow_emin);
        }
 
        // Case B: Index is -1
        else {
            double log_emin = std::log(emin.MeV());
            double log_emax = std::log(emax.MeV());
            flux = norm * (log_emax - log_emin);
        }
 
    } // endif: integration range was valid
 
    // Return flux
    return flux;
}
 
 
/***********************************************************************//**
 * @brief Returns model energy flux between [emin, emax] (units: erg/cm2/s)
 *
 * @param[in] emin Minimum photon energy.
 * @param[in] emax Minimum photon energy.
 * @return Energy flux (erg/cm2/s).
 *
 * Computes
 *
 * \f[
 *    \int_{\tt emin}^{\tt emax} S_{\rm E}(E | t) E \, dE
 * \f]
 *
 * where
 * - [@p emin, @p emax] is an energy interval, and
 * - \f$S_{\rm E}(E | t)\f$ is the spectral model (ph/cm2/s/MeV).
 ***************************************************************************/
double GModelSpectralPlawEnergyFlux::eflux(const GEnergy& emin,
                                           const GEnergy& emax) const
{
    // Initialise flux
    double eflux = 0.0;
 
    // Compute only if integration range is valid
    if (emin < emax) {
 
        // Compute power law normalization
        if (index() != -2.0) {
            double gamma        = m_index.value() + 2.0;
            double pow_ref_emin = std::pow(this->emin().MeV(), gamma);
            double pow_ref_emax = std::pow(this->emax().MeV(), gamma);
            double pow_emin     = std::pow(emin.MeV(), gamma);
            double pow_emax     = std::pow(emax.MeV(), gamma);
            double factor       = (pow_emax - pow_emin) /
                                  (pow_ref_emax - pow_ref_emin);
            eflux               = m_eflux.value() * factor;
        }
        else {
            double log_emin     = std::log(emin.MeV());
            double log_emax     = std::log(emax.MeV());
            double log_ref_emin = std::log(this->emin().MeV());
            double log_ref_emax = std::log(this->emax().MeV());
            double factor       = (log_emax - log_emin) /
                                  (log_ref_emax - log_ref_emin);
            eflux               = m_eflux.value() * factor;
        }
 
    } // endif: integration range was valid
 
    // Return flux
    return eflux;
}
 
 
/***********************************************************************//**
 * @brief Returns MC energy between [emin, emax]
 *
 * @param[in] emin Minimum photon energy.
 * @param[in] emax Maximum photon energy.
 * @param[in] time True photon arrival time.
 * @param[in,out] ran Random number generator.
 * @return Energy.
 *
 * Returns Monte Carlo energy by randomly drawing from a power law.
 ***************************************************************************/
GEnergy GModelSpectralPlawEnergyFlux::mc(const GEnergy& emin,
                                         const GEnergy& emax,
                                         const GTime&   time,
                                         GRan&          ran) const
{
    // Check energy interval
    gammalib::check_energy_interval(G_MC, emin, emax);
 
    // Allocate energy
    GEnergy energy;
 
    // Case A: Index is not -1
    if (index() != -1.0) {
        double exponent = index() + 1.0;
        double e_max    = std::pow(emax.MeV(), exponent);
        double e_min    = std::pow(emin.MeV(), exponent);
        double u        = ran.uniform();
        double eng      = (u > 0.0) 
                          ? std::exp(std::log(u * (e_max - e_min) + e_min) / exponent)
                          : 0.0;
        energy.MeV(eng);
    }
 
    // Case B: Index is -1
    else {
        double e_max = std::log(emax.MeV());
        double e_min = std::log(emin.MeV());
        double u     = ran.uniform();
        double eng   = std::exp(u * (e_max - e_min) + e_min);
        energy.MeV(eng);
    }
 
    // Return energy
    return energy;
}
 
 
/***********************************************************************//**
 * @brief Read model from XML element
 *
 * @param[in] xml XML element.
 *
 * Reads the spectral information from an XML element.
 ***************************************************************************/
void GModelSpectralPlawEnergyFlux::read(const GXmlElement& xml)
{
    // Verify number of model parameters
    gammalib::xml_check_parnum(G_READ, xml, 4);
 
    // Get parameter pointers
    const GXmlElement* eflux = gammalib::xml_get_par(G_READ, xml, m_eflux.name());
    const GXmlElement* index = gammalib::xml_get_par(G_READ, xml, m_index.name());
    const GXmlElement* emin  = gammalib::xml_get_par(G_READ, xml, m_emin.name());
    const GXmlElement* emax  = gammalib::xml_get_par(G_READ, xml, m_emax.name());
 
    // Read parameters
    m_eflux.read(*eflux);
    m_index.read(*index);
    m_emin.read(*emin);
    m_emax.read(*emax);
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Write model into XML element
 *
 * @param[in] xml XML element.
 *
 * Writes the spectral information into an XML element.
 ***************************************************************************/
void GModelSpectralPlawEnergyFlux::write(GXmlElement& xml) const
{
    // Verify model type
    gammalib::xml_check_type(G_WRITE, xml, type());
 
    // Get XML parameters
    GXmlElement* eflux = gammalib::xml_need_par(G_WRITE, xml, m_eflux.name());
    GXmlElement* index = gammalib::xml_need_par(G_WRITE, xml, m_index.name());
    GXmlElement* emin  = gammalib::xml_need_par(G_WRITE, xml, m_emin.name());
    GXmlElement* emax  = gammalib::xml_need_par(G_WRITE, xml, m_emax.name());
 
    // Write parameters
    m_eflux.write(*eflux);
    m_index.write(*index);
    m_emin.write(*emin);
    m_emax.write(*emax);
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Print power law information
 *
 * @param[in] chatter Chattiness.
 * @return String containing power law information.
 ***************************************************************************/
std::string GModelSpectralPlawEnergyFlux::print(const GChatter& chatter) const
{
    // Initialise result string
    std::string result;
 
    // Continue only if chatter is not silent
    if (chatter != SILENT) {
 
        // Append header
        result.append("=== GModelSpectralPlawEnergyFlux ===");
 
        // Append information
        result.append("\n"+gammalib::parformat("Number of parameters"));
        result.append(gammalib::str(size()));
        for (int i = 0; i < size(); ++i) {
            result.append("\n"+m_pars[i]->print(chatter));
        }
 
    } // endif: chatter was not silent
 
    // Return result
    return result;
}
 
 
/*==========================================================================
 =                                                                         =
 =                             Private methods                             =
 =                                                                         =
 ==========================================================================*/
 
/***********************************************************************//**
 * @brief Initialise class members
 ***************************************************************************/
void GModelSpectralPlawEnergyFlux::init_members(void)
{
    // Initialise model type
    m_type = "PowerLaw";
 
    // Initialise energy flux
    m_eflux.clear();
    m_eflux.name("EnergyFlux");
    m_eflux.unit("erg/cm2/s");
    m_eflux.scale(1.0);
    m_eflux.value(1.0);       // default: 1.0
    m_eflux.range(0.0, 10.0); // range:   [0,10]
    m_eflux.free();
    m_eflux.gradient(0.0);
    m_eflux.has_grad(true);
 
    // Initialise powerlaw index
    m_index.clear();
    m_index.name("Index");
    m_index.scale(1.0);
    m_index.value(-2.0);        // default: -2.0
    m_index.range(-10.0,+10.0); // range:   [-10,+10]
    m_index.free();
    m_index.gradient(0.0);
    m_index.has_grad(true);
 
    // Initialise lower limit
    m_emin.clear();
    m_emin.name("LowerLimit");
    m_emin.unit("MeV");
    m_emin.scale(1.0);
    m_emin.value(100.0);         // default: 100
    m_emin.range(0.001, 1.0e15); // range:   [0.001, 1e15]
    m_emin.fix();
    m_emin.gradient(0.0);
    m_emin.has_grad(false);
 
    // Initialise upper limit
    m_emax.clear();
    m_emax.name("UpperLimit");
    m_emax.unit("MeV");
    m_emax.scale(1.0);
    m_emax.value(500000.0);      // default: 500000
    m_emin.range(0.001, 1.0e15); // range:   [0.001, 1e15]
    m_emax.fix();
    m_emax.gradient(0.0);
    m_emax.has_grad(false);
 
    // Set parameter pointer(s)
    m_pars.clear();
    m_pars.push_back(&m_eflux);
    m_pars.push_back(&m_index);
    m_pars.push_back(&m_emin);
    m_pars.push_back(&m_emax);
 
    // Initialise last parameters (for fast computation)
    m_log_emin   = 0.0;
    m_log_emax   = 0.0;
    m_pow_emin   = 0.0;
    m_pow_emax   = 0.0;
    m_norm       = 0.0;
    m_power      = 0.0;
    m_last_index = 1000.0;
    m_last_emin.MeV(0.0);
    m_last_emax.MeV(0.0);
    m_last_energy.MeV(0.0);
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Copy class members
 *
 * @param[in] model Spectral power law model.
 ***************************************************************************/
void GModelSpectralPlawEnergyFlux::copy_members(const GModelSpectralPlawEnergyFlux& model)
{
    // Copy members
    m_type  = model.m_type;
    m_eflux = model.m_eflux;
    m_index = model.m_index;
    m_emin  = model.m_emin;
    m_emax  = model.m_emax;
 
    // Set parameter pointer(s)
    m_pars.clear();
    m_pars.push_back(&m_eflux);
    m_pars.push_back(&m_index);
    m_pars.push_back(&m_emin);
    m_pars.push_back(&m_emax);
 
    // Copy bookkeeping information
    m_log_emin     = model.m_log_emin;
    m_log_emax     = model.m_log_emax;
    m_pow_emin     = model.m_pow_emin;
    m_pow_emax     = model.m_pow_emax;
    m_norm         = model.m_norm;
    m_power        = model.m_power;
    m_last_index   = model.m_last_index;
    m_last_emin    = model.m_last_emin;
    m_last_emax    = model.m_last_emax;
    m_last_energy  = model.m_last_energy;
 
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Delete class members
 ***************************************************************************/
void GModelSpectralPlawEnergyFlux::free_members(void)
{
    // Return
    return;
}
 
 
/***********************************************************************//**
 * @brief Update precomputed values
 *
 * @param[in] srcEng Source energy
 ***************************************************************************/
void GModelSpectralPlawEnergyFlux::update(const GEnergy& srcEng) const
{
    // Compute index+1
    double gamma = index() + 2.0;
 
    // Change in spectral index?
    if (index() != m_last_index) {
 
        // Save actual spectral index
        m_last_index = index();
 
        // Change in energy boundaries?
        if (emin() != m_last_emin || emax() != m_last_emax) {
            m_log_emin  = std::log(emin().MeV());
            m_last_emin = emin();
            m_log_emax  = std::log(emax().MeV());
            m_last_emax = emax();
        }
 
        // Compute normalization factors
        if (gamma != 0.0) {
            m_pow_emin  = std::pow(emin().MeV(), gamma);
            m_pow_emax  = std::pow(emax().MeV(), gamma);
            double d    = m_pow_emax - m_pow_emin;
            m_norm      = gamma / d;
            m_g_norm    = 1.0/gamma -
                          (m_pow_emax*m_log_emax - m_pow_emin*m_log_emin)/d;
        }
        else {
            m_norm   = 1.0 / (m_log_emax - m_log_emin);
            m_g_norm = 0.0;
        }
 
        // Update power law factor
        m_power       = std::pow(srcEng.MeV(), index());
        m_last_energy = srcEng;
 
    } // endif: change in spectral index
 
    // ... no change in spectral index
    else {
 
        // Change in energy boundaries?
        if (emin() != m_last_emin || emax() != m_last_emax) {
 
            // Update energy boundaries
            m_log_emin  = std::log(emin().MeV());
            m_last_emin = emin();
            m_log_emax  = std::log(emax().MeV());
            m_last_emax = emax();
        
            // Compute power law normalization
            if (gamma != 0.0) {
                m_pow_emin  = std::pow(emin().MeV(), gamma);
                m_pow_emax  = std::pow(emax().MeV(), gamma);
                double d    = m_pow_emax - m_pow_emin;
                m_norm      = gamma / d;
                m_g_norm    = 1.0/gamma -
                              (m_pow_emax*m_log_emax - m_pow_emin*m_log_emin)/d;
            }
            else {
                m_norm = 1.0 / (m_log_emax - m_log_emin);
                m_g_norm = 0.0;
            }
 
        } // endif: change in energy boundaries
 
        // Change in energy?
        if (srcEng != m_last_energy) {
            m_power       = std::pow(srcEng.MeV(), index());
            m_last_energy = srcEng;
        }
 
    } // endelse: no change in spectral index
 
    // Return
    return;
}