The early growth of the first black holes

Johnson, Jarrett L.; Haardt, Francesco

doi:10.1017/pasa.2016.4

Title: The early growth of the first black holes

Journal Article · Fri Mar 04 00:00:00 EST 2016 · Publications of the Astronomical Society of Australia

DOI:https://doi.org/10.1017/pasa.2016.4· OSTI ID:1304824

Johnson, Jarrett L. ^[1]; Haardt, Francesco ^[2]

Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Univ. dell'Insubria, Como (Italy)

With detections of quasars powered by increasingly massive black holes at increasingly early times in cosmic history over the past decade, there has been correspondingly rapid progress made on the theory of early black hole formation and growth. Here, we review the emerging picture of how the first massive black holes formed from the primordial gas and then grew to supermassive scales. We discuss the initial conditions for the formation of the progenitors of these seed black holes, the factors dictating the initial masses with which they form, and their initial stages of growth via accretion, which may occur at super-Eddington rates. Lastly, we briefly discuss how these results connect to large-scale simulations of the growth of supermassive black holes in the first billion years after the Big Bang.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE (originally DOE/LANL)

Grant/Contract Number:: AC52-06NA25396

OSTI ID:: 1304824

Report Number(s):: LA-UR-15-20293; applab

Journal Information:: Publications of the Astronomical Society of Australia, Vol. 33; ISSN 1323-3580

Publisher:: CSIROCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 39 works

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