This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

Formation of the First Supermassive Black Holes

and

© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Volker Bromm and Abraham Loeb 2003 ApJ 596 34 DOI 10.1086/377529

0004-637X/596/1/34

Abstract

We consider the physical conditions under which supermassive black holes could have formed inside the first galaxies. Our smoothed particle hydrodynamics simulations indicate that metal-free galaxies with a virial temperature of ~104 K and suppressed H2 formation (due to an intergalactic UV background) tend to form a binary black hole system that contains a substantial fraction (≳10%) of the total baryonic mass of the host galaxy. Fragmentation into stars is suppressed without substantial H2 cooling. Our simulations follow the condensation of ~5 × 106 M around the two centers of the binary down to a scale of ≲0.1 pc. Low-spin galaxies form a single black hole instead. These early black holes lead to quasar activity before the epoch of reionization. Primordial black hole binaries lead to gravitational radiation emission at redshifts z ≳ 10 that would be detectable by Laser Interferometer Space Antenna.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/377529