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First Light and Reionization Epoch Simulations (FLARES) – XV: The physical properties of super-massive black holes and their impact on galaxies in the early universe

Wilkins, Stephen; Kuusisto, Jussi K.; Irodotou, Dimitrios; Liao, Shihong; Lovell, Christopher C.; Soininen, Sonja; Berger, Sabrina C.; Newman, Sophie L.; Roper, William J.; Seeyave, Louise T. C.; Thomas, Peter A.; Vijayan, Aswin P.

Authors

Stephen Wilkins

Jussi K. Kuusisto

Dimitrios Irodotou

Shihong Liao

Christopher C. Lovell

Sonja Soininen

Sabrina C. Berger

Sophie L. Newman

William J. Roper

Louise T. C. Seeyave

Peter A. Thomas

Aswin P. Vijayan



Abstract

Understanding the co-evolution of super-massive black holes (SMBHs) and their host galaxies remains a key challenge of extragalactic astrophysics, particularly the earliest stages at high-redshift. However, studying SMBHs at high-redshift with cosmological simulations, is challenging due to the large volumes and high-resolution required. Through its innovative simulation strategy, the First Light And Reionisation Epoch Simulations (FLARES) suite of cosmological hydrodynamical zoom simulations allows us to simulate a much wider range of environments which contain SMBHs with masses extending to
at
. In this paper, we use FLARES to study the physical properties of SMBHs and their hosts in the early Universe (
). FLARES predicts a sharply declining density with increasing redshift, decreasing by a factor of 100 over the range
. Comparison between our predicted mass and bolometric luminosity functions and pre-JWST observations yielded a reasonable match. However, recent JWST observations appear to suggest a higher density of SMBHs at
and the presence of more luminous SMBHs at
than predicted by FLARES. Finally, by using a re-simulation with AGN feedback disabled, we explore the impact of AGN feedback on their host galaxies. This reveals that AGN feedback results in a reduction of star formation activity, even at
, but only in the most massive galaxies. A deeper analysis reveals that AGN are also the cause of suppressed star formation in passive galaxies but that the presence of an AGN doesn’t necessarily result in the suppression of star formation.

Citation

Wilkins, S., Kuusisto, J. K., Irodotou, D., Liao, S., Lovell, C. C., Soininen, S., Berger, S. C., Newman, S. L., Roper, W. J., Seeyave, L. T. C., Thomas, P. A., & Vijayan, A. P. (in press). First Light and Reionization Epoch Simulations (FLARES) – XV: The physical properties of super-massive black holes and their impact on galaxies in the early universe. Open Journal of Astrophysics, 8, https://doi.org/10.33232/001c.132374

Journal Article Type Article
Acceptance Date Mar 19, 2025
Online Publication Date Mar 19, 2025
Deposit Date Apr 30, 2025
Journal The Open Journal of Astrophysics
Electronic ISSN 2565-6120
Publisher Maynooth Academic Publishing
Peer Reviewed Peer Reviewed
Volume 8
DOI https://doi.org/10.33232/001c.132374
Public URL https://keele-repository.worktribe.com/output/1202697
Publisher URL https://astro.theoj.org/article/132374-first-light-and-reionization-epoch-simulations-flares-xv-the-physical-properties-of-super-massive-black-holes-and-their-impact-on-galaxies-in-th



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