Grand Unified Model of Accretion Disks Around Black Holes: the Sub-Keplerian Paradigm
| dc.creator | Chakrabarti, Sandip K. | |
| dc.date | 1995-02-06 | |
| dc.date.accessioned | 2026-07-07T02:19:40Z | |
| dc.date.available | 2026-07-07T02:19:40Z | |
| dc.description | We show that viscous, transonic accretion disks which start with sub-Keplerian angular momentum at the outer boundary reproduce the features of the so-called thick, thin, slim and other accretion disk models depending upon the accretion rates and viscosity parameters. These disks are advection dominated in the pre-shock region and rotation dominated in the post-shock region when viscosity is less than a critical value. For a higher viscosity the shock disappears, and the flow has significant radial velocity only close to the black hole. | |
| dc.description | 4 pages, Latex. Two figures available upon request. Proceedings of 17th Texas Symposium (Munich, Dec. 1994) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9502040 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9502040 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/9955 | |
| dc.subject | Astrophysics | |
| dc.title | Grand Unified Model of Accretion Disks Around Black Holes: the Sub-Keplerian Paradigm | |
| dc.type | text |