Class Shakura-Sunyeav disk, inherited from Radiation.hpp.
More...
#include <ShSDisk.hpp>
|
double | Tin |
| Disk temperature at R=Rin in Kev.
|
|
double | Mbh |
|
double | Rg |
| Black hole mass in solar masses.
|
|
double | Ldisk |
| Disk luminosity in Eddington units.
|
|
double | Hratio |
|
std::vector< double > | en_phot |
| array of photon energies
|
|
std::vector< double > | num_phot |
| array of number of photons in units of erg/s/Hz
|
|
std::vector< double > | en_phot_obs |
| same as above but in observer frame
|
|
std::vector< double > | num_phot_obs |
| same as above but in observer frame
|
|
double | r |
|
double | z |
| Dimensions of emitting region.
|
|
double | vol |
| Volume of emitting region.
|
|
double | beta |
| speed of the emitting region
|
|
double | dopfac |
|
double | angle |
| Viewing angle/Doppler factor of emitting region.
|
|
double | dopnum |
| Doppler boosting exponent, depends on geometry.
|
|
bool | counterjet |
| boolean switch if user wants to include counterjet emission
|
|
std::string | geometry |
| string to track geometry of emitting region
|
|
Class Shakura-Sunyeav disk, inherited from Radiation.hpp.
◆ ShSDisk()
kariba::ShSDisk::ShSDisk |
( |
size_t |
size = 50 | ) |
|
Constructor for the disk. No input parameters because the sized of the arrays is set automatically, and every other property needs to be handled by the setters below
◆ cover_disk()
void kariba::ShSDisk::cover_disk |
( |
double |
f | ) |
|
this method removes a fraction f from the observed disk luminosity, assuming that it was absorbed and reprocessed into some other unspecified radiative mechanism
◆ disk_spectrum()
void kariba::ShSDisk::disk_spectrum |
( |
| ) |
|
◆ hdisk()
double kariba::ShSDisk::hdisk |
( |
| ) |
const |
|
inline |
◆ lum()
double kariba::ShSDisk::lum |
( |
| ) |
const |
|
inline |
◆ rin()
double kariba::ShSDisk::rin |
( |
| ) |
const |
|
inline |
◆ set_luminosity()
void kariba::ShSDisk::set_luminosity |
( |
double |
L | ) |
|
NOTE: the constant factor to go between inner temperature Tin and disk lunminosity Ldisk is 2 because the model uses the zero torque inner boundary condition, Kubota et al. 1998, hence the factor 2 rather than 4pi when converting between luminosity and temperature
◆ set_mbh()
void kariba::ShSDisk::set_mbh |
( |
double |
M | ) |
|
◆ set_rin()
void kariba::ShSDisk::set_rin |
( |
double |
R | ) |
|
Note: for disk r is inner radius, z is the outer radius, both are input in cm.
◆ set_rout()
void kariba::ShSDisk::set_rout |
( |
double |
R | ) |
|
◆ set_tin_k()
void kariba::ShSDisk::set_tin_k |
( |
double |
T | ) |
|
◆ set_tin_kev()
void kariba::ShSDisk::set_tin_kev |
( |
double |
T | ) |
|
◆ test()
void kariba::ShSDisk::test |
( |
| ) |
|
◆ tin()
double kariba::ShSDisk::tin |
( |
| ) |
const |
|
inline |
◆ total_luminosity()
double kariba::ShSDisk::total_luminosity |
( |
| ) |
|
Simple integration method to integrate num_phot_obs and get the total luminosity of the disk
◆ disk_int
double disk_int |
( |
double |
nu, |
|
|
void * |
p |
|
) |
| |
|
friend |
return SD spectrum over a given radius, frequency to be integrated over radius
◆ Hratio
double kariba::ShSDisk::Hratio |
|
protected |
Disk aspect ratio; TODO test with constant hbb or with hbb varying with disk size. Also test with just one Comptonization zone, and with one up to hbb(Rin) and another up to the end of the nozzle
◆ Ldisk
double kariba::ShSDisk::Ldisk |
|
protected |
Disk luminosity in Eddington units.
◆ Mbh
double kariba::ShSDisk::Mbh |
|
protected |
◆ Rg
double kariba::ShSDisk::Rg |
|
protected |
Black hole mass in solar masses.
◆ Tin
double kariba::ShSDisk::Tin |
|
protected |
Disk temperature at R=Rin in Kev.
The documentation for this class was generated from the following files: