Theory of disk accretion onto supermassive black holes

Author
Abstract

Accretion onto supermassive black holes produces both the dramatic phenomena associated with active galactic nuclei and the underwhelming displays seen in the Galactic Center and most other nearby galaxies. I review selected aspects of the current theoretical understanding of black hole accretion, emphasizing the role of magnetohydrodynamic turbulence and gravitational instabilities in driving the actual accretion and the importance of the efficacy of cooling in determining the structure and observational appearance of the accretion flow. Ongoing investigations into the dynamics of the plunging region, the origin of variability in the accretion process, and the evolution of warped, twisted, or eccentric disks are summarized.

Year of Publication
2004
Book Title
Supermassive Black Holes in the Distant Universe
Start Page (old)
3
Start Page or ID
89
Date Published
2004-01
Publisher
Kluwer Academic Publishers
URL
https://link.springer.com/chapter/10.1007/978-1-4020-2471-9_3
DOI
10.1007/978-1-4020-2471-9_3
Download citation
JILA PI
Book Chapter
JILA Topics
Group Name & Research Topics