The collapse of atomically cooled primordial haloes - I. High Lyman - Werner backgrounds

Patrick, Samuel J., Whalen, Daniel J., Latif, Muhammed A. and Elford, Jacob S. 2023. The collapse of atomically cooled primordial haloes - I. High Lyman - Werner backgrounds. Monthly Notices of the Royal Astronomical Society 522 (3) , pp. 3795-3808. 10.1093/mnras/stad1179

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Abstract

Pristine, atomically cooled haloes may be the sites of primordial quasar formation because atomic cooling triggers rapid baryon collapse that can create 104–105 M⊙ black hole seeds. However, no numerical simulation has ever followed the collapse of these haloes for the times required to form supermassive stars and direct-collapse black holes (DCBHs). We have now modelled baryon collapse in atomically cooled haloes with a wide range of spin parameters and assembly histories for times that are sufficient for DCBH formation. Fragmentation of accretion discs after ∼500 kyr is nearly ubiquitous in these haloes and in most cases leads to the formation of binary or multiple supermassive stellar systems. They also confirm that rapid baryon collapse proceeds for the times required for these stars to form DCBHs. Our simulations suggest that binary or even multiple DCBH formation was the rule rather than the exception in the primordial Universe.

Item Type:	Article
Date Type:	Published Online
Status:	Published
Schools:	Physics and Astronomy
Publisher:	Oxford University Press
ISSN:	0035-8711
Date of First Compliant Deposit:	15 September 2023
Date of Acceptance:	13 April 2023
Last Modified:	14 Nov 2024 11:30
URI:	https://orca.cardiff.ac.uk/id/eprint/162566

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