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Seeds don’t sink: even massive black hole ‘seeds’ cannot migrate to galaxy centres efficiently

Ma, Linhao and Hopkins, Philip F. and Ma, Xiangcheng and Anglés-Alcázar, Daniel and Faucher-Giguère, Claude-André and Kelley, Luke Zoltan (2021) Seeds don’t sink: even massive black hole ‘seeds’ cannot migrate to galaxy centres efficiently. Monthly Notices of the Royal Astronomical Society, 508 (2). pp. 1973-1985. ISSN 0035-8711. doi:10.1093/mnras/stab2713. https://resolver.caltech.edu/CaltechAUTHORS:20210309-082003361

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Abstract

Possible formation scenarios of supermassive black holes (BHs) in the early universe include rapid growth from less massive seed BHs via super-Eddington accretion or runaway mergers, yet both of these scenarios would require seed BHs to efficiently sink to and be trapped in the Galactic Centre via dynamical friction. This may not be true for their complicated dynamics in clumpy high-z galaxies. In this work, we study this ‘sinking problem’ with state-of-the-art high-resolution cosmological simulations, combined with both direct N-body integration of seed BH trajectories and post-processing of randomly generated test particles with a newly developed dynamical friction estimator. We find that seed BHs less massive than 10⁸M⊙ (i.e. all but the already-supermassive seeds) cannot efficiently sink in typical high-z galaxies. We also discuss two possible solutions: dramatically increasing the number of seeds such that one seed can end up trapped in the Galactic Centre by chance, or seed BHs being embedded in dense structures (e.g. star clusters) with effective masses above the mass threshold. We discuss the limitations of both solutions.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stab2713DOIArticle
https://arxiv.org/abs/2101.02727arXivDiscussion Paper
ORCID:
AuthorORCID
Ma, Linhao0000-0001-6117-5750
Hopkins, Philip F.0000-0003-3729-1684
Ma, Xiangcheng0000-0001-8091-2349
Anglés-Alcázar, Daniel0000-0001-5769-4945
Faucher-Giguère, Claude-André0000-0002-4900-6628
Kelley, Luke Zoltan0000-0002-6625-6450
Additional Information:© 2021 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Accepted 2021 September 16. Received 2021 August 25; in original form 2021 January 7. Published: 22 September 2021. We thank Zuyi Chen and Alessandro Lupi for their useful discussions. Support for LM and PFH was provided by NSF Research Grants 1911233 & 20009234, NSF CAREER grant 1455342, NASA grants 80NSSC18K0562, HST-AR-15800.001-A. DAA acknowledges support by NSF grant AST-2009687 and by the Flatiron Institute, which is supported by the Simons Foundation. CAFG was supported by NSF through grants AST-1715216 and CAREER award AST-1652522; by NASA through grant 17-ATP17-0067; and by a Cottrell Scholar Award and a Scialog Award from the Research Corporation for Science Advancement. Numerical calculations were run on the Caltech compute cluster ‘Wheeler,’ allocations FTA-Hopkins supported by the NSF and TACC, and NASA HEC SMD-16-7592. Data Availability: The data and source code supporting the plots within this paper are available on reasonable request to the corresponding author.
Group:Astronomy Department, TAPIR
Funders:
Funding AgencyGrant Number
NSFAST-1911233
NSF20009234
NSFAST-1455342
NASA80NSSC18K0562
NASAHST-AR-15800.001-A
NSFAST-2009687
Flatiron InstituteUNSPECIFIED
Simons FoundationUNSPECIFIED
NSFAST-1715216
NSFAST-1652522
NASA17-ATP17-0067
Cottrell Scholar of Research CorporationUNSPECIFIED
NASASMD-16-7592
Subject Keywords:black hole physics – galaxies: evolution – galaxies: formation – galaxies: high-redshift – galaxies: kinematics and dynamics
Issue or Number:2
DOI:10.1093/mnras/stab2713
Record Number:CaltechAUTHORS:20210309-082003361
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210309-082003361
Official Citation:Linhao Ma, Philip F Hopkins, Xiangcheng Ma, Daniel Anglés-Alcázar, Claude-André Faucher-Giguère, Luke Zoltan Kelley, Seeds don’t sink: even massive black hole ‘seeds’ cannot migrate to galaxy centres efficiently, Monthly Notices of the Royal Astronomical Society, Volume 508, Issue 2, December 2021, Pages 1973–1985, https://doi.org/10.1093/mnras/stab2713
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:108359
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:10 Mar 2021 20:06
Last Modified:03 Dec 2021 21:09

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