Regan, John and Wise, John H. and O'Shea, Brian W. and Norman, Michael L. (2020) The emergence of the first star-free atomic cooling haloes in the Universe. Monthly Notices of the Royal Astronomical Society, 492 (2). pp. 3021-3031. ISSN 1365-2966

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Abstract

Using the Renaissance suite of simulations, we examine the emergence of pristine atomic cooling haloes that are both metal free and star free in the early universe. The absence of metals prevents catastrophic cooling, suppresses fragmentation, and may allow for the formation of massive black hole seeds. Here we report on the abundance of pristine atomic cooling haloes found and on the specific physical conditions that allow for the formation of these direct-collapse-black hole (DCBH) haloes. In total, in our simulations we find that 79 DCBH haloes form before a redshift of 11.6. We find that the formation of pristine atomic haloes is driven by the rapid assembly of the atomic cooling haloes with mergers, both minor and/or major, prior to reaching the atomic cooling limit a requirement. However, the ability of assembling haloes to remain free of (external) metal enrichment is equally important and underlines the necessity of following the transport of metals in such simulations. The candidate DCBH-hosting haloes we find have been exposed to mean Lyman–Werner radiation fields of J21 ∼1 and typically lie at least 10 kpc (physical) from the nearest massive galaxy. The growth rates of the haloes reach values of greater than 107M⊙ per unit redshift, leading to significant dynamical heating and the suppression of efficient cooling until the halo crosses the atomic cooling threshold. Finally, we also find five synchronized halo candidates where pairs of pristine atomic cooling haloes emerge that are both spatially and temporally synchronized.

Item Type:	Article
Additional Information:	Cite as: John A Regan, John H Wise, Brian W O’Shea, Michael L Norman, The emergence of the first star-free atomic cooling haloes in the Universe, Monthly Notices of the Royal Astronomical Society, Volume 492, Issue 2, February 2020, Pages 3021–3031, DOI: 10.1093/mnras/staa035
Keywords:	methods: numerical; stars: black holes; large-scale structure of Universe; cosmology: theory;
Academic Unit:	Faculty of Science and Engineering > Research Institutes > Hamilton Institute Faculty of Science and Engineering > Theoretical Physics
Item ID:	14852
Identification Number:	https://doi.org/10.1093/mnras/staa035
Depositing User:	John Regan
Date Deposited:	23 Sep 2021 16:32
Journal or Publication Title:	Monthly Notices of the Royal Astronomical Society
Publisher:	Oxford University Press
Refereed:	Yes
URI:	Publisher Organisation
Use Licence:	This item is available under a Creative Commons Attribution Non Commercial Share Alike Licence (CC BY-NC-SA). Details of this licence are available here

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