kerrbb: multi-temperature blackbody model for thin accretion disk around a Kerr black hole

A multi-temperature blackbody model for a thin, steady state, general relativistic accretion disk around a Kerr black hole. The effect of self-irradiation of the disk is considered, and the torque at the inner boundary of the disk is allowed to be non-zero. This model is intended as an extension to grad, which assumes that the black hole is non-rotating. For details see Li et al. (2005).

par1 | eta, ratio of the disk power produced by a torque at the disk inner boundary to the disk power arising from accretion. It must be and . When eta = 0, the solution corresponds to that of a standard Keplerian disk with zero torque at the inner boundary. |

par2 | specific angular momentum of the black hole in units of the black hole mass M (geometrized units G=c=1). Should be and <1. |

par3 | disk's inclination angle (the angle between the axis of the disk and the line of sight). It is expressed in degrees. i=0 is for a "face-on" accretion disk. i should be degree. |

par4 | the mass of the black hole in units of the solar mass. |

par5 | the ``effective'' mass accretion rate of the disk in units of g/s. When eta = 0 (zero torque at the inner boundary), this is just the mass accretion rate of the disk. When eta is nonzero, the effective mass accretion rate = (1+eta) times the true mass accretion rate of the disk. The total disk luminosity is then ``epsilon'' times ``the effective mass accretion rate'' times c, where epsilon is the radiation efficiency of a standard accretion disk around the Kerr black hole |

par6 | the distance from the observer to the black hole in units of kpc. |

par7 | spectral hardening factor, T/T. It should be greater than 1.0, and considered to be 1.5-1.9 for accretion disks around a stellar-mass black hole. See, e.g., Shimura & Takahara (1995) |

par8 | a flag to switch on/off the effect of self-irradiation (never allowed to be free). Self-irradiation is included when > 0. Self-irradiation is not included when . |

par9 | a flag to switch on/off the effect of limb-darkening (never allowed to be free). The disk emission is assumed to be limb-darkened when >0. The disk emission is assumed to be isotropic when lflag is . |

K | normalization. Should be set to 1 if the inclination, mass and distance are frozen. |