Formation of super-massive black holes

Wolfgang J. Duschl, Peter A. Strittmatter

Research output: Chapter in Book/Report/Conference proceedingChapter

Abstract

We show that the rapid formation of super-massive black holes in quasars can indeed be understood in terms of major galaxy mergers followed by disk accretion. The necessary short disk evolution time can be achieved provided the disk viscosity is sufficiently large, which, for instance, is the case for hydrodynamic turbulence, unlimited by shock dissipation. We present numerical calculations for a representative case. This general picture can account for (a) the presence of highly luminous quasars at redshifts z > 6; (b) for the peak in quasar activity at z ~ 2; and (c) for a subsequent rapid disappearance of quasars at later epochs.

Original languageEnglish (US)
Title of host publicationThe Tenth Marcel Grossmann Meeting
Subtitle of host publicationOn Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories
PublisherWorld Scientific Publishing Co.
Pages550-558
Number of pages9
Volume1
ISBN (Electronic)9789812704030
ISBN (Print)9789812566676
DOIs
StatePublished - Jan 1 2006

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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