High-redshift supermassive black hole population from core-collapse in self-interacting dark matter halos

arXiv:2609.13041 · astro-ph.GA, astro-ph.CO, hep-ph · Submitted 2026-09-11 · Read on arXiv

astro-ph.GA, astro-ph.CO, hep-ph

Submitted: 2026-09-11

Updated: 2026-09-11

Comments: 22 pages and 6 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 5× in this paper · explained in 2 episodes

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