Feedback Limits Rapid Growth of Seed Black Holes at High Redshift
- 18 January 2006
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 637 (2), L85-L88
- https://doi.org/10.1086/500557
Abstract
Seed black holes formed in the collapse of Population III stars have been invoked to explain the presence of supermassive black holes at high redshift. It has been suggested that a seed black hole can grow up to 105-106 M☉ through highly super-Eddington accretion for a period of ~106-107 yr at redshift z = 20-24. We studied the feedback of radiation pressure, Compton heating, and outflow during the seed black hole growth. It is found that its surrounding medium fueled to the seed hole is greatly heated by Compton heating. For a supercritical accretion onto a 103 M☉ seed hole, a Compton sphere (with a temperature ~106 K) will be formed on a timescale of 1.6 × 103 yr so that the hole is only supplied by a rate of 10-3 of the Eddington limit from the Compton sphere. The kinetic feedback of the strong outflow will heat the medium at a large distance from the black hole; this leads to a dramatic decrease of the outer Bondi accretion onto the black hole and avoids the accumulation of the matter. The highly supercritical accretion will be rapidly halted by the strong feedback. The seed black hole hardly grows up at the very early universe unless the strong feedback can be avoided.Keywords
This publication has 38 references indexed in Scilit:
- Slim Disks with Transition Regions and Applications to Microquasars and Narrow‐Line Seyfert 1 GalaxiesThe Astrophysical Journal, 2004
- Iron Emission in the z = 6.4 Quasar SDSS J114816.64+525150.3The Astrophysical Journal, 2003
- A Variable Ultraluminous Supersoft X‐Ray Source in “The Antennae”: Stellar‐Mass Black Hole or White Dwarf?The Astrophysical Journal, 2003
- Super-Eddington Fluxes from Thin Accretion Disks?The Astrophysical Journal, 2002
- A Survey of [CLC][ITAL]z[/ITAL][/CLC] > 5.8 Quasars in the Sloan Digital Sky Survey. I. Discovery of Three New Quasars and the Spatial Density of Luminous Quasars at [CLC][ITAL]z[/ITAL][/CLC] ∼ 6The Astronomical Journal, 2001
- Slim accretion disksThe Astrophysical Journal, 1988
- Angular momentum from tidal torquesThe Astrophysical Journal, 1987
- Monte Carlo simulations of the evolution of galactic nuclei containing massive, central black holesThe Astrophysical Journal, 1983
- Thick accretion disks - Self-similar, supercritical modelsThe Astrophysical Journal, 1982
- On Spherically Symmetrical AccretionMonthly Notices of the Royal Astronomical Society, 1952