The SKIRT project
advanced radiative transfer for astrophysics
SersicGeometry Class Reference

#include <SersicGeometry.hpp>

Inheritance diagram for SersicGeometry:

Public Member Functions

 ~SersicGeometry ()
double density (double r) const override
double effectiveRadius () const
double index () const
double randomRadius () const override
double Sigmar () const override
Public Member Functions inherited from SpheGeometry
double density (Position bfr) const override
int dimension () const override
Position generatePosition () const override
double SigmaX () const override
double SigmaY () const override
double SigmaZ () const override
Public Member Functions inherited from SimulationItem
template<class T>
T * find (bool setup=true) const
template<class T>
T * interface (int levels=-999999, bool setup=true) const
virtual string itemName () const
void setup ()
string typeAndName () const
Public Member Functions inherited from Item
 Item (const Item &)=delete
virtual ~Item ()
void addChild (Item *child)
const vector< Item * > & children () const
virtual void clearItemListProperty (const PropertyDef *property)
void destroyChild (Item *child)
virtual bool getBoolProperty (const PropertyDef *property) const
virtual vector< double > getDoubleListProperty (const PropertyDef *property) const
virtual double getDoubleProperty (const PropertyDef *property) const
virtual string getEnumProperty (const PropertyDef *property) const
virtual int getIntProperty (const PropertyDef *property) const
virtual vector< Item * > getItemListProperty (const PropertyDef *property) const
virtual ItemgetItemProperty (const PropertyDef *property) const
virtual string getStringProperty (const PropertyDef *property) const
int getUtilityProperty (string name) const
virtual void insertIntoItemListProperty (const PropertyDef *property, int index, Item *item)
Itemoperator= (const Item &)=delete
Itemparent () const
virtual void removeFromItemListProperty (const PropertyDef *property, int index)
virtual void setBoolProperty (const PropertyDef *property, bool value)
virtual void setDoubleListProperty (const PropertyDef *property, vector< double > value)
virtual void setDoubleProperty (const PropertyDef *property, double value)
virtual void setEnumProperty (const PropertyDef *property, string value)
virtual void setIntProperty (const PropertyDef *property, int value)
virtual void setItemProperty (const PropertyDef *property, Item *item)
virtual void setStringProperty (const PropertyDef *property, string value)
void setUtilityProperty (string name, int value)
virtual string type () const

Protected Member Functions

 SersicGeometry ()
void setupSelfBefore () override
Protected Member Functions inherited from SpheGeometry
 SpheGeometry ()
Protected Member Functions inherited from Geometry
 Geometry ()
Randomrandom () const
Protected Member Functions inherited from SimulationItem
 SimulationItem ()
virtual bool offersInterface (const std::type_info &interfaceTypeInfo) const
virtual void setupSelfAfter ()
Protected Member Functions inherited from Item
 Item ()

Private Types

using BaseType
using ItemType

Private Attributes

double _b
double _effectiveRadius
double _index
const double & _n
const double & _reff
double _rho0
SersicFunction_sersicfunction

Friends

class ItemRegistry

Detailed Description

The SersicGeometry class is a subclass of the SpheGeometry class, and describes spherically symmetric stellar geometries characterized by the density distribution

\[ \rho(r) = \rho_0\, {\cal{S}}_n \left(\frac{r}{r_{\text{eff}}}\right), \]

with \({\cal{S}}_n(s)\) the Sersic function of order \(n\) (see SersicFunction). It is defined in such a way that the projected surface brightness profile has the form

\[ I(r_p) = I_0 \exp \left[ -b_n\left( \frac{r_p}{r_{\text{eff}}} \right)^{1/n} \right]. \]

Two parameters characterize a SersicGeometry class object: the Sersic index \(n\) and the effective radius \(r_{\text{eff}}\). Internally, the SersicGeometry class has a SersicFunction object as one of its data members. See Sersic (1963) and Ciotti & Bertin (1999, A&A 352, 447–451).

Constructor & Destructor Documentation

◆ SersicGeometry()

SersicGeometry::SersicGeometry ( )
inlineprotected

Default constructor for concrete Item subclass SersicGeometry: "a Sérsic geometry".

◆ ~SersicGeometry()

SersicGeometry::~SersicGeometry ( )

The destructor; it deallocates the sersic function object created during setup.

Member Function Documentation

◆ density()

double SersicGeometry::density ( double r) const
overridevirtual

This function returns the density \(\rho(r)\) at a radius \(r\). It just implements the analytical formula.

Implements SpheGeometry.

◆ effectiveRadius()

double SersicGeometry::effectiveRadius ( ) const
inline

This function returns the value of the discoverable double property effectiveRadius: "the effective radius".

This property represents a physical quantity of type "length".

The minimum value for this property is "]0".

◆ index()

double SersicGeometry::index ( ) const
inline

This function returns the value of the discoverable double property index: "the Sérsic index n".

The minimum value for this property is "]0.5".

The maximum value for this property is "10]".

The default value for this property is given by the conditional value expression "1".

◆ randomRadius()

double SersicGeometry::randomRadius ( ) const
overridevirtual

This function returns the radius of a random position drawn from the Sersic density distribution. This is accomplished by generating a uniform deviate \({\cal{X}}\), and solving the equation

\[ {\cal{X}} = M(r) = 4\pi \int_0^r \rho(r')\, r'{}^2\, {\text{d}}r' \]

for \(r\). For the Sersic model, we use the SersicFunction::inversemass() function to solve this equation.

Implements SpheGeometry.

◆ setupSelfBefore()

void SersicGeometry::setupSelfBefore ( )
overrideprotectedvirtual

This function creates a SersicFunction class object. The central density \(\rho_0\) is set by the normalization condition that the total mass is equal to one. Since the Sersic function satisfies the normalization

\[ 4\pi \int_0^\infty {\cal{S}}_n(s)\, s^2\, {\text{d}}s = 1, \]

we easily find

\[ \rho_0 = \frac{1}{r_{\text{eff}}^3} \]

This function also caches the value of the dimensionless constant \(b_n\) that appears in the definition of the Sersic profile. A suitable approximation is

\[ b_n = 2n -\frac{1}{3} + \frac{4}{405n} + \frac{46}{25515n^2} + \frac{131}{1148175n^3}. \]

Reimplemented from Geometry.

◆ Sigmar()

double SersicGeometry::Sigmar ( ) const
overridevirtual

This function returns the radial surface density, i.e. the integration of the density along a line starting at the centre of the coordinate system,

\[ \Sigma_r = \int_0^\infty \rho(r)\,{\text{d}}r. \]

For the Sersic geometry, one finds

\[ \Sigma_r = \frac{1}{r_{\text{eff}}^2}\, \frac{b_n^{2n}}{ 2\pi\, \Gamma(2n+1)}. \]

Implements SpheGeometry.


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