Influence of tides and self-gravity on Ultra-Light Dark Matter Bounds from Dwarf Galaxies
hep-ph, astro-ph.CO, astro-ph.GA
Submitted: 2026-04-01
Updated: 2026-09-01
Terminology
Sources
- Ultralight scalars as cosmological dark matter
- Wave Dark Matter
- Ultra-Light Dark Matter
- Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
- Understanding the Core-Halo Relation of Quantum Wave Dark Matter, $\psi$DM, from 3D Simulations
- Simulations of solitonic core mergers in ultra-light axion dark matter cosmologies
- Cosmological particle-in-cell simulations with ultralight axion dark matter
- Galaxy Formation with BECDM: I. Turbulence and relaxation of idealised haloes
- Formation and structure of ultralight bosonic dark matter halos
- Formation and mass growth of axion stars in axion miniclusters
- New insights into the formation and growth of boson stars in dark matter halos
- AxioNyx: Simulating Mixed Fuzzy and Cold Dark Matter
- Cosmological Simulation for Fuzzy Dark Matter Model
- Strong Constraints on Fuzzy Dark Matter from Ultrafaint Dwarf Galaxy Eridanus II
- Soliton Oscillations and Revised Constraints from Eridanus II of Fuzzy Dark Matter
- Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: I. Analytical results
- Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: II. Numerical results
- Gravitational Bose-Einstein condensation in the kinetic regime
- Do Dark Matter Axions Form a Condensate with Long-Range Correlation?
- Relaxation in a Fuzzy Dark Matter Halo
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