Primary
kerrbb ⚬ˣˢᵖᵉᶜ｜Documentation｜1st｜20251021193231-00-⌔
kerrbb, zkerrbb: multi-temperature blackbody model for thin accretion disk around a Kerr black hole
kerrbb, zkerrbb: multi-temperature blackbody model for thin accretion disk around a Kerr black holeA 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).
The redshift version zkerrbb has the mass accretion rate parameter in units of Solar masses per year and the distance parameter replaced by redshift.
Parameters for kerrbb:
Parameters for zkerrbb:
Printed 2026-06-28.
(echo:: @ ᯤ)
Link to original
Secondary
• • •