Core-Halo Mass Relation in Cosmological Vector Dark Matter
Jiajun Chen, Yonghao Yao, David J. E. Marsh
astro-ph.CO
Submitted: 2026-07-20
Comments: 9 pages, 8 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- A Review on the Scalar Field/ Bose-Einstein Condensate Dark Matter Model
- Do Dark Matter Axions Form a Condensate with Long-Range Correlation?
- Schr\"odinger method as N-body double and UV completion of dust
- Ultralight scalars as cosmological dark matter
- Formation of Solitonic Stars Through Gravitational Cooling
- Dynamical Boson Stars
- Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
- Formation and mass growth of axion stars in axion miniclusters
- Gravitational Bose-Einstein condensation in the kinetic regime
- Landau equation for self-gravitating classical and quantum particles: Application to dark matter
- Kinetic relaxation and Bose-star formation in multicomponent dark matter- I
- The Diversity of Core Halo Structure in the Fuzzy Dark Matter Model
- Core-halo mass relation of ultralight axion dark matter from merger history
- Galactic Rotation Curves vs. Ultra-Light Dark Matter: Implications of the Soliton -- Host Halo Relation
- Looking for ultralight dark matter near supermassive black holes
- Soliton Merger Rates and Enhanced Axion Dark Matter Decay
- Axion Star Explosions: A New Source for Axion Indirect Detection
- Ultra-Light Dark Matter Simulations and Stellar Dynamics: Tension in Dwarf Galaxies for $m < 5\times10^{-21} $ eV
- WISPy Cold Dark Matter
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