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The Cosmogony of Super-Massive Black Holes

We report results of a project investigating the growth of super-massive black holes (BHs) by disk accretion. We find that the BH mass growth is quick enough to account for the inferred masses in the highest-redshift quasars, and the growth time is an inverse function of the final BH mass as seems to be required by recent X-ray surveys.

preprint2006arXivOpen access
Wolfgang J. DuschlPeter A. Strittmatter
astro-ph
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Wolfgang J. DuschlPeter A. Strittmatter

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