Galaxy and Halo Assembly Bias in Alternative Dark Matter Models

arXiv:2609.32086 · astro-ph.CO · Submitted 2026-09-25 · Read on arXiv

astro-ph.CO

Submitted: 2026-09-25

Updated: 2026-09-25

Project page: https://gdespali.github.io/AIDA

Terminology

• Clustering — 44× in this paper · explained in 2 episodes
• AIDA-TNG — 23× in this paper · explained in 1 episode
• Abundance — 8× in this paper · explained in 1 episode
• Robustness — 7× in this paper · explained in 5 episodes
• Core — 3× in this paper · explained in 2 episodes
• Warm Dark Matter (WDM) — 2× in this paper · explained in 3 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Gravitational Lensing — 1× in this paper · explained in 2 episodes
• Little Red Dots — 1× in this paper · explained in 2 episodes
• N-body simulations — 1× in this paper · explained in 2 episodes
• Velocity Dispersion — 1× in this paper · explained in 2 episodes

Sources

• Survival of the most compact: the life and death of satellite halos in self-interacting dark matter

Related papers

• Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
• A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
• Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
• Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
• Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
• Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation