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advanced radiative transfer for astrophysics
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PlanckFunction Class Reference

#include <PlanckFunction.hpp>

Public Member Functions

 PlanckFunction (double T)
 
double cdf (Array &lambdav, Array &pv, Array &Pv, Range lambdaRange) const
 
double operator() (double lambda) const
 
double value (double lambda) const
 

Private Attributes

double _f1
 
double _f2
 
double _T
 

Detailed Description

This class represents the Planck function

Bλ(λ,T)=2hc2λ51exp(hcλkT)1.

The temperature T is specified in the constructor.

Constructor & Destructor Documentation

◆ PlanckFunction()

PlanckFunction::PlanckFunction ( double  T)
explicit

The constructor for the PlanckFunction class accepts the temperature T and precalculates some constants for later use.

Member Function Documentation

◆ cdf()

double PlanckFunction::cdf ( Array lambdav,
Array pv,
Array Pv,
Range  lambdaRange 
) const

This function constructs a tabulated normalized probability density function (pdf) and the corresponding normalized cumulative distribution function (cdf) for the Planck function with temperature T (specified in the constructor) within the given wavelength range. As the basis for the tabulation, the function constructs a logarithmic wavelength grid with approximately 1000 wavelength points for each order of magitude in the wavelength range. The integration to determine the cdf is performed using a mechanism that assumes that the pdf behaves as a power-law between any two grid points.

◆ operator()()

double PlanckFunction::operator() ( double  lambda) const
inline

This function call operator returns the value of the Planck function Bλ(λ,T) for a given wavelength λ and for the temperature T specified in the constructor. It is equivalent to the value() function.

◆ value()

double PlanckFunction::value ( double  lambda) const

This function returns the value of the Planck function Bλ(λ,T) for a given wavelength λ and for the temperature T specified in the constructor.


The documentation for this class was generated from the following file: