Variability in Supermassive Black-Hole Accretion Rates in Fuzzy Dark Matter Cores due to Black-Hole Wandering
Eric Ludwig, Philip Mocz, Victor Robles
astro-ph.CO
Submitted: 2026-07-01
Comments: 11 pages, 5 figures
Code: https://github.com/pmocz/quantum-jax
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- An 800-million-solar-mass black hole in a significantly neutral Universe at redshift 7.5
- P\={o}niu\={a}'ena: A Luminous $z=7.5$ Quasar Hosting a 1.5 Billion Solar Mass Black Hole
- A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars
- UNCOVER: A NIRSpec Identification of a Broad Line AGN at z = 8.50
- Evidence for heavy seed origin of early supermassive black holes from a z~10 X-ray quasar
- A candidate supermassive black hole in a gravitationally-lensed galaxy at $z\approx10$
- A recently quenched galaxy 700 million years after the Big Bang
- Formation of the First Stars
- The Birth of a Massive First-Star Binary
- Formation of massive black holes in rapidly growing pre-galactic gas clouds
- Light, medium-weight or heavy? The nature of the first supermassive black hole seeds
- Direct formation of massive black holes via dynamical collapse in metal-enriched merging galaxies at $z \sim 10$: fully cosmological simulations
- Can Supermassive Black Holes Form in Metal-Enriched High-Redshift Protogalaxies ?
- Formation of the first nuclear clusters and massive black holes at high redshift
- SMBH growth parameters in the early Universe of Millennium and Millennium-II simulations
- Hyper-Eddington accretion flows onto massive black holes
- The sustainable growth of the first black holes
- Observability of Low-Luminosity AGN in the Early Universe with JWST
- Physical Pathways for JWST-Observed Supermassive Black Holes in the Early Universe
- Energy input from quasars regulates the growth and activity of black holes and their host galaxies
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