Cover Image

Accretion of self-interacting dark matter onto supermassive black holes

Fuente: arXiv

Saved in:

Bibliographic Details
Main Authors:	Sabarish, V. M., Brüggen, Marcus, Schmidt-Hoberg, Kai, Fischer, Moritz S.
Format:	Preprint
Published:	2025
Subjects:	Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

Similar Items

Simulations of galaxy cluster mergers with velocity-dependent, rare and frequent self-interactions
by: Sabarish, V. M., et al.
Published: (2023)

Cosmological and idealized simulations of dark matter haloes with velocity-dependent, rare and frequent self-interactions
by: Fischer, Moritz S., et al.
Published: (2023)

Accretion onto supermassive and intermediate mass black holes in cosmological simulations
by: Weinberger, Rainer, et al.
Published: (2025)

Early formation of supermassive black holes from the collapse of strongly self-interacting dark matter
by: Roberts, M. Grant, et al.
Published: (2024)

Testing the isothermal Jeans model for self-interacting dark matter halos in the collapse phase
by: Li, Shubo, et al.
Published: (2026)

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation
by: Patil, Yashraj, et al.
Published: (2025)

Primordial black holes as supermassive black holes seeds
by: Ziparo, Francesco, et al.
Published: (2024)

Bondi-Hoyle-Lyttleton accretion onto ultra dense dark matter halos and direct collapse black holes
by: Subramanian, Kandaswamy, et al.
Published: (2026)

Primordial black holes in cosmological simulations: growth prospects for supermassive black holes
by: Prole, Lewis R., et al.
Published: (2025)

The large cores of dark matter and globular clusters in AS1063. Possible evidence of self-interacting dark matter. Or not
by: Diego, Jose M.
Published: (2026)

Accurately simulating core-collapse self-interacting dark matter halos
by: Fischer, Moritz S., et al.
Published: (2025)

A two-phase model of galaxy formation: IV. Seeding and growing supermassive black holes in dark matter halos
by: Chen, Yangyao, et al.
Published: (2025)

Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
by: Yesuf, Hassen M., et al.
Published: (2026)

Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter
by: Straight, Maria C., et al.
Published: (2025)

Simulating realistic self-interacting dark matter models including small and large-angle scattering
by: Arido, Cenanda, et al.
Published: (2024)

An attractive model: simulating fuzzy dark matter with attractive self-interactions
by: Painter, Connor A., et al.
Published: (2024)

Scattering of wave dark matter by supermassive black holes
by: Tomaselli, Giovanni Maria
Published: (2024)

Influence of supermassive primordial black holes on ultraviolet luminosity of high-redshift galaxies
by: Li, Yi-Yang, et al.
Published: (2025)

Numerical challenges for energy conservation in N-body simulations of collapsing self-interacting dark matter halos
by: Fischer, Moritz S., et al.
Published: (2024)

Sub-Eddington accreting supermassive primordial black holes explain Little Red Dots
by: Huang, Hai-Long, et al.
Published: (2024)

The overconcentrated dark halo in the strong lens SDSS J0946+1006 is a subhalo: evidence for self interacting dark matter?
by: Enzi, Wolfgang J. R., et al.
Published: (2024)

Dynamical reconstruction of SPARC galactic halos within self-interacting fuzzy dark matter
by: Indjin, Milos, et al.
Published: (2025)

The formation of supermassive black holes from Population III.1 seeds. IV. Self-regulated seeding from supermassive star ionizing feedback
by: Petkova, Maya A., et al.
Published: (2026)

Survival of the most compact: the life and death of satellite halos in self-interacting dark matter
by: Klemmer, David, et al.
Published: (2026)

Dianoga SIDM: galaxy cluster self-interacting dark matter simulations
by: Ragagnin, Antonio, et al.
Published: (2024)

Improved constraints from ultra-faint dwarf galaxies on primordial black holes as dark matter
by: Stegmann, Jakob, et al.
Published: (2019)

A Bayesian approach to the halo galaxy - supermassive black hole connection through cosmic time
by: Boettner, Christopher, et al.
Published: (2023)

Core collapse in resonant self-interacting dark matter across two decades in halo mass
by: Tran, Vinh, et al.
Published: (2025)

Dynamical friction for circular orbits in self-interacting ultralight dark matter and Fornax globular clusters
by: Koo, Hyeonmo, et al.
Published: (2025)

Conditions for Super-Eddington Accretion onto the First Black Holes
by: Gordon, Simone T., et al.
Published: (2024)

Novel method to trace the dark matter density profile around supermassive black holes with AGN reverberation mapping
by: Sharma, Mayank, et al.
Published: (2025)

Where to search for supermassive binary black holes
by: Marziani, Paola, et al.
Published: (2025)

The origin of supermassive black holes at cosmic dawn
by: Sharma, Ritik, et al.
Published: (2023)

DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
by: Harvey, David, et al.
Published: (2025)

Fast rotations in galaxies at cosmic noon indicate central concentration of stars, dark matter or massive black holes
by: Roman-Oliveira, Fernanda, et al.
Published: (2026)

On the evolution of a twisted thin accretion disc in eccentric inclined supermassive binary black holes
by: Ivanov, P. B., et al.
Published: (2024)

Dark-to-black super accretion as a mechanism for early supermassive black hole growth
by: Sanchis-Gual, Nicolas, et al.
Published: (2025)

Galactic and extragalactic probe of dark matter with LISA's binary black holes
by: Ghodla, Sohan
Published: (2024)

Uncertainties in the supermassive black hole abundance and implications for the GW background
by: Sato-Polito, Gabriela, et al.
Published: (2025)

Eccentricity effects on the supermassive black hole gravitational wave background
by: Raidal, Juhan, et al.
Published: (2024)