Spherically Symmetric Fluid Simulations of Black Hole Accretion in Self-Interacting Dark Matter Halos
Zhe Meng, Tan Chen, Bocheng Zhu, Fan Zhou, Bin Hu, Liang Gao, Rong-Gen Cai
astro-ph.CO
Submitted: 2026-07-02
Comments: 15 pages, 7 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Waning of the WIMP? A Review of Models, Searches, and Constraints
- Dark Matter Search Results from 4.2 Tonne-Years of Exposure of the LUX-ZEPLIN (LZ) Experiment
- First Search for Light Dark Matter in the Neutrino Fog with XENONnT
- Observational evidence for self-interacting cold dark matter
- Subhaloes in Self-Interacting Galactic Dark Matter Haloes
- Dark Matter Self-interactions and Small Scale Structure
- A semi-analytic study of self-interacting dark-matter haloes with baryons
- A Parametric Model for Self-Interacting Dark Matter Halos
- The impact of baryonic potentials on the gravothermal evolution of self-interacting dark matter haloes
- Distinctive GWBs from eccentric inspiraling SMBH binaries with a DM spike
- An Enhanced Isothermal Jeans Approach to Constraining Dark Matter Self-Interactions from Galactic Kinematics
- Testing the isothermal Jeans model for self-interacting dark matter halos in the collapse phase
- Dark Matter Halos as Particle Colliders: A Unified Solution to Small-Scale Structure Puzzles from Dwarfs to Clusters
- Small-Scale Challenges to the $\Lambda$CDM Paradigm
- The Core-Cusp Problem
- Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses
- Too big to fail? The puzzling darkness of massive Milky Way subhaloes
- Constraining Self-Interacting Dark Matter with the Milky Way's dwarf spheroidals
- The unexpected diversity of dwarf galaxy rotation curves
- How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves
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