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Growing Supermassive Black Holes in Cosmological Simulations of Structure Formation

Published online by Cambridge University Press:  03 June 2010

Debora Sijacki ,
Volker Springel  and
Martin G. Haehnelt
Debora Sijacki
Affiliation:
Kavli Institute for Cosmology, Cambridge and Institute of Astronomy Madingley Road, Cambridge, CB3 0HA, UK Email: [email protected], [email protected]
Volker Springel
Affiliation:
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Straße 1, 85740 Garching bei München, Germany Email: [email protected]
Martin G. Haehnelt
Affiliation:
Kavli Institute for Cosmology, Cambridge and Institute of Astronomy Madingley Road, Cambridge, CB3 0HA, UK Email: [email protected], [email protected]
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Abstract

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We discuss a numerical model for black hole (BH) growth and feedback that allows simultaneous tracking of the evolution of galaxies and their central BHs in fully cosmological simulations. After describing the main features of the numerical model adopted, we show how BHs in these simulations affect the properties of their host halos and how this in turn impacts the growth of the BHs themselves. We also present results from a set of simulations specifically designed to address the issue of BH assembly in the early Universe and discuss whether or not different extensions of the model, in particular rapidly spinning BHs and gravitational recoils, can hamper the formation of the first bright quasars.

Keywords

black hole physicsmethods: numericalcosmology: theory
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S267: Co-Evolution of Central Black Holes and Galaxies , August 2009 , pp. 445 - 450
Copyright
Copyright © International Astronomical Union 2010

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