GModelSpectralFunc.cpp
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/***************************************************************************
* GModelSpectralFunc.cpp - Spectral function model class *
* ----------------------------------------------------------------------- *
* copyright (C) 2010-2013 by Juergen Knoedlseder *
* ----------------------------------------------------------------------- *
* *
* 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 GModelSpectralFunc.cpp
* @brief Spectral function model class implementation
* @author Juergen Knoedlseder
*/
/* __ Includes ___________________________________________________________ */
#ifdef HAVE_CONFIG_H
#include <config.h>
#endif
#include <cmath>
#include "GException.hpp"
#include "GTools.hpp"
#include "GCsv.hpp"
#include "GModelSpectralFunc.hpp"
#include "GModelSpectralRegistry.hpp"
/* __ Constants __________________________________________________________ */
/* __ Globals ____________________________________________________________ */
const GModelSpectralFunc g_spectral_func_seed;
const GModelSpectralRegistry g_spectral_func_registry(&g_spectral_func_seed);
/* __ Method name definitions ____________________________________________ */
#define G_FLUX "GModelSpectralFunc::flux(GEnergy&, GEnergy&)"
#define G_EFLUX "GModelSpectralFunc::eflux(GEnergy&, GEnergy&)"
#define G_MC "GModelSpectralFunc::mc(GEnergy&, GEnergy&, GRan&)"
#define G_READ "GModelSpectralFunc::read(GXmlElement&)"
#define G_WRITE "GModelSpectralFunc::write(GXmlElement&)"
#define G_LOAD_NODES "GModelSpectralFunc::load_nodes(std::string&)"
/* __ Macros _____________________________________________________________ */
/* __ Coding definitions _________________________________________________ */
/* __ Debug definitions __________________________________________________ */
/*==========================================================================
= =
= Constructors/destructors =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Void constructor
***************************************************************************/
GModelSpectralFunc::GModelSpectralFunc(void) : GModelSpectral()
{
// Initialise members
init_members();
// Return
return;
}
/***********************************************************************//**
* @brief File constructor
*
* @param[in] filename File name of nodes.
*
* Creates instance of a spectral function model from a list of nodes that is
* found in the specified file. See GModelSpectralFunc::load_nodes() for more
* information about the expected structure of the file.
***************************************************************************/
GModelSpectralFunc::GModelSpectralFunc(const std::string& filename)
: GModelSpectral()
{
// Initialise members
init_members();
// Load nodes
load_nodes(filename);
// Return
return;
}
/***********************************************************************//**
* @brief XML constructor
*
* @param[in] xml XML element.
*
* Creates instance of a spectral function model by extracting information
* from an XML element. See GModelSpectralFunc::read() for more information
* about the expected structure of the XML element.
***************************************************************************/
GModelSpectralFunc::GModelSpectralFunc(const GXmlElement& xml) :
GModelSpectral()
{
// Initialise members
init_members();
// Read information from XML element
read(xml);
// Return
return;
}
/***********************************************************************//**
* @brief Copy constructor
*
* @param[in] model Spectral function model.
***************************************************************************/
GModelSpectralFunc::GModelSpectralFunc(const GModelSpectralFunc& model) :
GModelSpectral(model)
{
// Initialise members
init_members();
// Copy members
copy_members(model);
// Return
return;
}
/***********************************************************************//**
* @brief Destructor
***************************************************************************/
GModelSpectralFunc::~GModelSpectralFunc(void)
{
// Free members
free_members();
// Return
return;
}
/*==========================================================================
= =
= Operators =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Assignment operator
*
* @param[in] model Spectral function model.
***************************************************************************/
GModelSpectralFunc& GModelSpectralFunc::operator= (const GModelSpectralFunc& 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 instance
***************************************************************************/
void GModelSpectralFunc::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 instance
***************************************************************************/
GModelSpectralFunc* GModelSpectralFunc::clone(void) const
{
return new GModelSpectralFunc(*this);
}
/***********************************************************************//**
* @brief Evaluate model
*
* @param[in] srcEng True photon energy.
* @param[in] srcTime True photon arrival time.
* @return Model value (ph/cm2/s/MeV).
*
* The spectral model is defined as
* \f[I(E)=norm f(E)\f]
* where
* \f$norm\f$ is the normalization of the function.
* Note that the node energies are stored as log10 of energy in units of
* MeV.
***************************************************************************/
double GModelSpectralFunc::eval(const GEnergy& srcEng,
const GTime& srcTime) const
{
// Interpolate function. This is done in log10-log10 space, but the
// linear value is returned.
double arg = m_log_nodes.interpolate(srcEng.log10MeV(), m_log_values);
double func = std::pow(10.0, arg);
// Compute function value
double value = norm() * func;
// Compile option: Check for NaN/Inf
#if defined(G_NAN_CHECK)
if (isnotanumber(value) || isinfinite(value)) {
std::cout << "*** ERROR: GModelSpectralFunc::eval";
std::cout << "(srcEng=" << srcEng << "):";
std::cout << " NaN/Inf encountered";
std::cout << " (value=" << value;
std::cout << ", norm=" << norm();
std::cout << ", func=" << func;
std::cout << ")" << std::endl;
}
#endif
// Return
return value;
}
/***********************************************************************//**
* @brief Evaluate function and gradients
*
* @param[in] srcEng True photon energy.
* @param[in] srcTime True photon arrival time.
* @return Model value (ph/cm2/s/MeV).
*
* The spectral model is defined as
* \f[I(E)=norm f(E)\f]
* where
* \f$norm=n_s n_v\f$ is the normalization of the function.
* Note that the normalization is factorised into a scaling factor and a
* value and that the method is expected to return the gradient with respect
* to the parameter value \f$n_v\f$.
*
* The partial derivative of the normalization value is given by
* \f[dI/dn_v=n_s f(E)\f]
***************************************************************************/
double GModelSpectralFunc::eval_gradients(const GEnergy& srcEng,
const GTime& srcTime)
{
// Interpolate function. This is done in log10-log10 space, but the
// linear value is returned.
double arg = m_log_nodes.interpolate(srcEng.log10MeV(), m_log_values);
double func = std::pow(10.0, arg);
// Compute function value
double value = norm() * func;
// Compute partial derivatives of the parameter values
double g_norm = (m_norm.isfree()) ? m_norm.scale() * func : 0.0;
// Set gradients (circumvent const correctness)
const_cast<GModelSpectralFunc*>(this)->m_norm.factor_gradient(g_norm);
// Compile option: Check for NaN/Inf
#if defined(G_NAN_CHECK)
if (isnotanumber(value) || isinfinite(value)) {
std::cout << "*** ERROR: GModelSpectralFunc::eval_gradients";
std::cout << "(srcEng=" << srcEng << "):";
std::cout << " NaN/Inf encountered";
std::cout << " (value=" << value;
std::cout << ", norm=" << norm();
std::cout << ", func=" << func;
std::cout << ", g_norm=" << g_norm;
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 Maximum photon energy.
* @return Photon flux (ph/cm2/s).
*
* @exception GException::erange_invalid
* Energy range is invalid (emin < emax required).
*
* Computes
* \f[\int_{E_{\rm min}}^{E_{\rm max}} I(E) dE\f]
* where
* \f$E_{\rm min}\f$ and \f$E_{\rm max}\f$ are the minimum and maximum
* energy, respectively, and
* \f$I(E)\f$ is the spectral model (units: ph/cm2/s/MeV).
***************************************************************************/
double GModelSpectralFunc::flux(const GEnergy& emin, const GEnergy& emax) const
{
// Throw an exception if energy range is invalid
if (emin >= emax) {
throw GException::erange_invalid(G_FLUX, emin.MeV(), emax.MeV(),
"Minimum energy < maximum energy required.");
}
// Initialise flux
double flux = 0.0;
// Get energy range in MeV
double e_min = emin.MeV();
double e_max = emax.MeV();
// Continue only if e_max > e_min
if (e_max > e_min) {
// Determine left node index for minimum energy
m_lin_nodes.set_value(e_min);
int inx_emin = m_lin_nodes.inx_left();
// Determine left node index for maximum energy
m_lin_nodes.set_value(e_max);
int inx_emax = m_lin_nodes.inx_left();
// If both energies are within the same nodes then simply
// integrate over the energy interval using the appropriate power
// law parameters
if (inx_emin == inx_emax) {
flux = m_prefactor[inx_emin] *
plaw_photon_flux(e_min,
e_max,
m_epivot[inx_emin],
m_gamma[inx_emin]);
}
// ... otherwise integrate over the nodes where emin and emax
// resides and all the remaining nodes
else {
// If we are requested to extrapolate beyond first node,
// the use the first nodes lower energy and upper energy
// boundary for the initial integration.
int i_start = (e_min < m_lin_nodes[0]) ? inx_emin : inx_emin+1;
// Integrate from emin to the node boundary
flux = m_prefactor[inx_emin] *
plaw_photon_flux(e_min,
m_lin_nodes[i_start],
m_epivot[inx_emin],
m_gamma[inx_emin]);
// Integrate over all nodes between
for (int i = i_start; i < inx_emax; ++i) {
flux += m_flux[i];
}
// Integrate from node boundary to emax
flux += m_prefactor[inx_emax] *
plaw_photon_flux(m_lin_nodes[inx_emax],
e_max,
m_epivot[inx_emax],
m_gamma[inx_emax]);
} // endelse: emin and emax not between same nodes
// Multiply flux by normalisation factor
flux *= norm();
} // endif: e_max > e_min
// Return
return flux;
}
/***********************************************************************//**
* @brief Returns model energy flux between [emin, emax] (units: erg/cm2/s)
*
* @param[in] emin Minimum photon energy.
* @param[in] emax Maximum photon energy.
* @return Energy flux (erg/cm2/s).
*
* @exception GException::erange_invalid
* Energy range is invalid (emin < emax required).
*
* Computes
* \f[\int_{E_{\rm min}}^{E_{\rm max}} I(E) E dE\f]
* where
* \f$E_{\rm min}\f$ and \f$E_{\rm max}\f$ are the minimum and maximum
* energy, respectively, and
* \f$I(E)\f$ is the spectral model (units: ph/cm2/s/MeV).
***************************************************************************/
double GModelSpectralFunc::eflux(const GEnergy& emin, const GEnergy& emax) const
{
// Throw an exception if energy range is invalid
if (emin >= emax) {
throw GException::erange_invalid(G_EFLUX, emin.MeV(), emax.MeV(),
"Minimum energy < maximum energy required.");
}
// Initialise flux
double flux = 0.0;
// Get energy range in MeV
double e_min = emin.MeV();
double e_max = emax.MeV();
// Continue only if e_max > e_min
if (e_max > e_min) {
// Determine left node index for minimum energy
m_lin_nodes.set_value(e_min);
int inx_emin = m_lin_nodes.inx_left();
// Determine left node index for maximum energy
m_lin_nodes.set_value(e_max);
int inx_emax = m_lin_nodes.inx_left();
// If both energies are within the same nodes then simply
// integrate over the energy interval using the appropriate power
// law parameters
if (inx_emin == inx_emax) {
flux = m_prefactor[inx_emin] *
plaw_energy_flux(e_min,
e_max,
m_epivot[inx_emin],
m_gamma[inx_emin]) * MeV2erg;
}
// ... otherwise integrate over the nodes where emin and emax
// resides and all the remaining nodes
else {
// If we are requested to extrapolate beyond first node,
// the use the first nodes lower energy and upper energy
// boundary for the initial integration.
int i_start = (e_min < m_lin_nodes[0]) ? inx_emin : inx_emin+1;
// Integrate from emin to the node boundary
flux = m_prefactor[inx_emin] *
plaw_energy_flux(e_min,
m_lin_nodes[i_start],
m_epivot[inx_emin],
m_gamma[inx_emin]) * MeV2erg;
// Integrate over all nodes between
for (int i = i_start; i < inx_emax; ++i) {
flux += m_eflux[i];
}
// Integrate from node boundary to emax
flux += m_prefactor[inx_emax] *
plaw_energy_flux(m_lin_nodes[inx_emax],
e_max,
m_epivot[inx_emax],
m_gamma[inx_emax]) * MeV2erg;
} // endelse: emin and emax not between same nodes
// Multiply flux by normalisation factor
flux *= norm();
} // endif: e_max > e_min
// Return
return flux;
}
/***********************************************************************//**
* @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.
*
* @exception GException::erange_invalid
* Energy range is invalid (emin < emax required).
*
* Simulates a random energy in the interval [emin, emax] for a spectral
* function.
***************************************************************************/
GEnergy GModelSpectralFunc::mc(const GEnergy& emin,
const GEnergy& emax,
const GTime& time,
GRan& ran) const
{
// Throw an exception if energy range is invalid
if (emin >= emax) {
throw GException::erange_invalid(G_MC, emin.MeV(), emax.MeV(),
"Minimum energy < maximum energy required.");
}
// Allocate energy
GEnergy energy;
// Continue only if emax > emin
if (emax > emin) {
// Update cache
mc_update(emin, emax);
// Determine in which bin we reside
int inx = 0;
if (m_mc_cum.size() > 1) {
double u = ran.uniform();
for (inx = m_mc_cum.size()-1; inx > 0; --inx) {
if (m_mc_cum[inx-1] <= u) {
break;
}
}
}
// Get random energy for specific bin
if (m_mc_exp[inx] != 0.0) {
double e_min = m_mc_min[inx];
double e_max = m_mc_max[inx];
double u = ran.uniform();
double eng = (u > 0.0)
? std::exp(std::log(u * (e_max - e_min) + e_min) / m_mc_exp[inx])
: 0.0;
energy.MeV(eng);
}
else {
double e_min = m_mc_min[inx];
double e_max = m_mc_max[inx];
double u = ran.uniform();
double eng = std::exp(u * (e_max - e_min) + e_min);
energy.MeV(eng);
}
} // endif: emax > emin
// Return energy
return energy;
}
/***********************************************************************//**
* @brief Read model from XML element
*
* @param[in] xml XML element containing power law model information.
*
* @exception GException::model_invalid_parnum
* Invalid number of model parameters found in XML element.
* @exception GException::model_invalid_parnames
* Invalid model parameter name found in XML element.
*
* Read the function information from an XML element and load the nodes
* from the associated file. The XML element is required to have an
* attribute "file" that specifies the function nodes and a parameter
* named "Normalization".
***************************************************************************/
void GModelSpectralFunc::read(const GXmlElement& xml)
{
// Verify that XML element has exactly 1 parameter
if (xml.elements() != 1 || xml.elements("parameter") != 1) {
throw GException::model_invalid_parnum(G_READ, xml,
"Spectral function requires exactly 1 parameter.");
}
// Get parameter element
const GXmlElement* par = xml.element("parameter", 0);
// Get value
if (par->attribute("name") == "Normalization") {
m_norm.read(*par);
}
else {
throw GException::model_invalid_parnames(G_READ, xml,
"Require \"Normalization\" parameter.");
}
// Load nodes from file
load_nodes(xml.attribute("file"));
// Return
return;
}
/***********************************************************************//**
* @brief Write model into XML element
*
* @param[in] xml XML element into which model information is written.
*
* @exception GException::model_invalid_spectral
* Existing XML element is not of type "FileFunction"
* @exception GException::model_invalid_parnum
* Invalid number of model parameters or nodes found in XML element.
* @exception GException::model_invalid_parnames
* Invalid model parameter names found in XML element.
*
* Write the spectral function information into an XML element. The XML
* element has to be of type "FileFunction" and will have 1 parameter leaf
* named "Normalization". Note that the function nodes will not be written
* since they will not be altered by any method.
***************************************************************************/
void GModelSpectralFunc::write(GXmlElement& xml) const
{
// Set model type
if (xml.attribute("type") == "") {
xml.attribute("type", "FileFunction");
}
// Verify model type
if (xml.attribute("type") != "FileFunction") {
throw GException::model_invalid_spectral(G_WRITE, xml.attribute("type"),
"Spectral model is not of type \"FileFunction\".");
}
// If XML element has 0 nodes then append 1 parameter node
if (xml.elements() == 0) {
xml.append(GXmlElement("parameter name=\"Normalization\""));
}
// Verify that XML element has exactly 1 parameter
if (xml.elements() != 1 || xml.elements("parameter") != 1) {
throw GException::model_invalid_parnum(G_WRITE, xml,
"Spectral function requires exactly 1 parameter.");
}
// Get parameter element
GXmlElement* par = xml.element("parameter", 0);
// Set parameyter
if (par->attribute("name") == "Normalization") {
m_norm.write(*par);
}
else {
throw GException::model_invalid_parnames(G_WRITE, xml,
"Require \"Normalization\" parameter.");
}
// Return
return;
}
/***********************************************************************//**
* @brief Print powerlaw information
***************************************************************************/
std::string GModelSpectralFunc::print(void) const
{
// Initialise result string
std::string result;
// Append header
result.append("=== GModelSpectralFunc ===");
result.append("\n"+parformat("Function file")+m_filename);
result.append("\n"+parformat("Number of nodes")+str(m_lin_nodes.size()));
result.append("\n"+parformat("Number of parameters")+str(size()));
for (int i = 0; i < size(); ++i) {
result.append("\n"+m_pars[i]->print());
}
// Append node information
for (int i = 0; i < m_prefactor.size(); ++i) {
result.append("\n"+parformat("Node "+str(i+1)));
result.append("Epivot="+str(m_epivot[i]));
result.append(" Prefactor="+str(m_prefactor[i]));
result.append(" Gamma="+str(m_gamma[i]));
result.append(" Flux="+str(m_flux[i]));
result.append(" EFlux="+str(m_eflux[i]));
}
// Return result
return result;
}
/*==========================================================================
= =
= Private methods =
= =
==========================================================================*/
/***********************************************************************//**
* @brief Initialise class members
***************************************************************************/
void GModelSpectralFunc::init_members(void)
{
// Initialise powerlaw normalisation
m_norm.clear();
m_norm.name("Normalization");
m_norm.scale(1.0);
m_norm.value(1.0);
m_norm.range(0.0,1000.0);
m_norm.free();
m_norm.gradient(0.0);
m_norm.hasgrad(true);
// Set parameter pointer(s)
m_pars.clear();
m_pars.push_back(&m_norm);
// Initialise members
m_lin_nodes.clear();
m_log_nodes.clear();
m_lin_values.clear();
m_log_values.clear();
m_filename.clear();
// Initialise cache
m_mc_emin.clear();
m_mc_emax.clear();
m_mc_cum.clear();
m_mc_min.clear();
m_mc_max.clear();
m_mc_exp.clear();
// Return
return;
}
/***********************************************************************//**
* @brief Copy class members
*
* @param[in] model Spectral function model.
***************************************************************************/
void GModelSpectralFunc::copy_members(const GModelSpectralFunc& model)
{
// Copy members
m_norm = model.m_norm;
m_lin_nodes = model.m_lin_nodes;
m_log_nodes = model.m_log_nodes;
m_lin_values = model.m_lin_values;
m_log_values = model.m_log_values;
m_filename = model.m_filename;
// Copy pre-computation cache
m_prefactor = model.m_prefactor;
m_gamma = model.m_gamma;
m_epivot = model.m_epivot;
m_flux = model.m_flux;
m_eflux = model.m_eflux;
// Copy MC cache
m_mc_emin = model.m_mc_emin;
m_mc_emax = model.m_mc_emax;
m_mc_cum = model.m_mc_cum;
m_mc_min = model.m_mc_min;
m_mc_max = model.m_mc_max;
m_mc_exp = model.m_mc_exp;
// Set parameter pointer(s)
m_pars.clear();
m_pars.push_back(&m_norm);
// Return
return;
}
/***********************************************************************//**
* @brief Delete class members
***************************************************************************/
void GModelSpectralFunc::free_members(void)
{
// Return
return;
}
/***********************************************************************//**
* @brief Load nodes from file
*
* @param[in] filename File name.
*
* @exception GException::file_function_data
* File contains less than 2 nodes
* @exception GException::file_function_columns
* File contains less than 2 columns
* @exception GException::file_function_value
* File contains invalid value
*
* The file function is stored as a column separated value table (CSV) in an
* ASCII file with (at least) 2 columns. The first column specifies the
* energy in MeV while the second column specifies the intensity at this
* energy in units of ph/cm2/s/MeV.
* The node energies and values will be stored both linearly and as log10.
* The log10 storing requires that node energies and node values are
* positive. Also, at least 2 nodes and 2 columns are required in the file
* function.
***************************************************************************/
void GModelSpectralFunc::load_nodes(const std::string& filename)
{
// Clear nodes and values
m_lin_nodes.clear();
m_log_nodes.clear();
m_lin_values.clear();
m_log_values.clear();
// Set filename
m_filename = filename;
// Load file
GCsv csv = GCsv(filename);
// Check if there are at least 2 nodes
if (csv.nrows() < 2) {
throw GException::file_function_data(G_LOAD_NODES, filename,
csv.nrows());
}
// Check if there are at least 2 columns
if (csv.ncols() < 2) {
throw GException::file_function_columns(G_LOAD_NODES, filename,
csv.ncols());
}
// Setup nodes
double last_energy = 0.0;
for (int i = 0; i < csv.nrows(); ++i) {
// Get log10 of node energy and value. Make sure they are valid.
double log10energy;
double log10value;
if (csv.real(i,0) > 0) {
log10energy = std::log10(csv.real(i,0));
}
else {
throw GException::file_function_value(G_LOAD_NODES, filename,
csv.real(i,0), "Energy value must be positive.");
}
if (csv.real(i,1) > 0) {
log10value = std::log10(csv.real(i,1));
}
else {
throw GException::file_function_value(G_LOAD_NODES, filename,
csv.real(i,1), "Intensity value must be positive.");
}
// Make sure that energies are increasing
if (csv.real(i,0) <= last_energy) {
throw GException::file_function_value(G_LOAD_NODES, filename,
csv.real(i,0), "Energy values must be monotonically increasing.");
}
// Append log10 of node energy and value
m_lin_nodes.append(csv.real(i,0));
m_log_nodes.append(log10energy);
m_lin_values.push_back(csv.real(i,1));
m_log_values.push_back(log10value);
// Store last energy for monotonically increasing check
last_energy = csv.real(i,0);
} // endfor: looped over nodes
// Set pre-computation cache
set_cache();
// Return
return;
}
/***********************************************************************//**
* @brief Set pre-computation cache
***************************************************************************/
void GModelSpectralFunc::set_cache(void) const
{
// Clear any existing values
m_prefactor.clear();
m_gamma.clear();
m_epivot.clear();
m_flux.clear();
m_eflux.clear();
// Loop over all nodes-1
for (int i = 0; i < m_lin_nodes.size()-1; ++i) {
// Get energies and function values
double emin = m_lin_nodes[i];
double emax = m_lin_nodes[i+1];
double fmin = m_lin_values[i];
double fmax = m_lin_values[i+1];
// Compute pivot energy (MeV). We use here the geometric mean of
// the node boundaries.
double epivot = std::sqrt(emin*emax);
// Compute spectral index
double gamma = std::log(fmin/fmax) / std::log(emin/emax);
// Compute power law normalisation
double prefactor = fmin / std::pow(emin/epivot, gamma);
// Compute photon flux between nodes
double flux = prefactor*plaw_photon_flux(emin, emax, epivot, gamma);
// Compute energy flux between nodes
double eflux = prefactor*plaw_energy_flux(emin, emax, epivot, gamma);
// Convert energy flux from MeV/cm2/s to erg/cm2/s
eflux *= MeV2erg;
// Push back values on pre-computation cache
m_prefactor.push_back(prefactor);
m_gamma.push_back(gamma);
m_epivot.push_back(epivot);
m_flux.push_back(flux);
m_eflux.push_back(eflux);
} // endfor: looped over all nodes
// Return
return;
}
/***********************************************************************//**
* @brief Set MC pre-computation cache
*
* @param[in] emin Minimum energy.
* @param[in] emax Maximum energy.
*
* This method sets up an array of indices and the cumulative distribution
* function needed for MC simulations.
*
***************************************************************************/
void GModelSpectralFunc::mc_update(const GEnergy& emin, const GEnergy& emax) const
{
// Check if we need to update the cache
if (emin != m_mc_emin || emax != m_mc_emax) {
// Store new energy interval
m_mc_emin = emin;
m_mc_emax = emax;
// Initialise cache
m_mc_cum.clear();
m_mc_min.clear();
m_mc_max.clear();
m_mc_exp.clear();
// Get energy range in MeV
double e_min = emin.MeV();
double e_max = emax.MeV();
// Continue only if e_max > e_min
if (e_max > e_min) {
// Allocate flux
double flux;
// Determine left node index for minimum energy
m_lin_nodes.set_value(e_min);
int inx_emin = m_lin_nodes.inx_left();
// Determine left node index for maximum energy
m_lin_nodes.set_value(e_max);
int inx_emax = m_lin_nodes.inx_left();
// If both energies are within the same node then just
// add this one node on the stack
if (inx_emin == inx_emax) {
flux = m_prefactor[inx_emin] *
plaw_photon_flux(e_min,
e_max,
m_epivot[inx_emin],
m_gamma[inx_emin]);
m_mc_cum.push_back(flux);
m_mc_min.push_back(e_min);
m_mc_max.push_back(e_max);
m_mc_exp.push_back(m_gamma[inx_emin]);
}
// ... otherwise integrate over the nodes where emin and emax
// resides and all the remaining nodes
else {
// If we are requested to extrapolate beyond first node,
// the use the first nodes lower energy and upper energy
// boundary for the initial integration.
int i_start = (e_min < m_lin_nodes[0]) ? inx_emin : inx_emin+1;
// Add emin to the node boundary
flux = m_prefactor[inx_emin] *
plaw_photon_flux(e_min,
m_lin_nodes[i_start],
m_epivot[inx_emin],
m_gamma[inx_emin]);
m_mc_cum.push_back(flux);
m_mc_min.push_back(e_min);
m_mc_max.push_back(m_lin_nodes[i_start]);
m_mc_exp.push_back(m_gamma[inx_emin]);
// Add all nodes between
for (int i = i_start; i < inx_emax; ++i) {
flux = m_flux[i];
m_mc_cum.push_back(flux);
m_mc_min.push_back(m_lin_nodes[i]);
m_mc_max.push_back(m_lin_nodes[i+1]);
m_mc_exp.push_back(m_gamma[i]);
}
// Add node boundary to emax
flux = m_prefactor[inx_emax] *
plaw_photon_flux(m_lin_nodes[inx_emax],
e_max,
m_epivot[inx_emax],
m_gamma[inx_emax]);
m_mc_cum.push_back(flux);
m_mc_min.push_back(m_lin_nodes[inx_emax]);
m_mc_max.push_back(e_max);
m_mc_exp.push_back(m_gamma[inx_emax]);
} // endelse: emin and emax not between same nodes
// Build cumulative distribution
for (int i = 1; i < m_mc_cum.size(); ++i) {
m_mc_cum[i] += m_mc_cum[i-1];
}
double norm = m_mc_cum[m_mc_cum.size()-1];
for (int i = 0; i < m_mc_cum.size(); ++i) {
m_mc_cum[i] /= norm;
}
// Set MC values
for (int i = 0; i < m_mc_cum.size(); ++i) {
// Compute exponent
double exponent = m_mc_exp[i] + 1.0;
// Exponent dependend computation
if (std::abs(exponent) > 1.0e-11) {
m_mc_exp[i] = exponent;
m_mc_min[i] = std::pow(m_mc_min[i], exponent);
m_mc_max[i] = std::pow(m_mc_max[i], exponent);
}
else {
m_mc_exp[i] = 0.0;
m_mc_min[i] = std::log(m_mc_min[i]);
m_mc_max[i] = std::log(m_mc_max[i]);
}
} // endfor: set MC values
} // endif: e_max > e_min
} // endif: Update was required
// Return
return;
}
/*==========================================================================
= =
= Friends =
= =
==========================================================================*/