The Clustering of Little Red Dots from Ultra-Strongly Self-Interacting Dark Matter
astro-ph.CO, astro-ph.GA, hep-ph
Submitted: 2025-12-19
Updated: 2026-09-24
Terminology
Sources
- Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots
- A Critical Evaluation of the Physical Nature of the Little Red Dots
- Formation of the Little Red Dots from the Core-collapse of Self-interacting Dark Matter Halos
- The Large-scale Environments of Low-luminosity AGNs at $3.9 < z < 6$ and Implications for Their Host Dark Matter Halos from a Complete NIRCam Grism Redshift Survey
- Little Red Dots from Ultra-Strongly Self-Interacting Dark Matter
- Ultra-Strongly Self-Interacting Dark Matter: From Phenomenology to Astrophysical Observables
- Massive Black Holes Seeded by Dark Matter -- Implications for Little Red Dots and Gravitational Wave Signatures
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