Can bosenovae deplete the galactic dark matter?
astro-ph.HE, astro-ph.CO, astro-ph.GA, hep-ph
Submitted: 2026-10-14
Updated: 2026-10-14
Comments: 16 pages, 11 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Sources
- Ultralight scalars as cosmological dark matter
- String Axiverse
- Gravitational Bose-Einstein condensation in the kinetic regime
- Searching for Earth/Solar Axion Halos
- Probing Ultralight Bosons with Binary Black Holes
- A Generic Formation Mechanism of Ultralight Dark Matter Solar Halos
- Relativistic axions from collapsing Bose stars
- Collapse of Axion Stars
- Kinetic relaxation and nucleation of Bose stars in self-interacting wave dark matter
- Dynamical Boson Stars
- Recurrent Axinovae and their Cosmological Constraints
- Detectability of accretion-induced bosenovae in the Milky Way
- Condensation and Evaporation of Boson Stars
- Axion Star Bosenova in Axion Miniclusters
- Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: I. Analytical results
- Analysis of Dark Matter Axion Clumps with Spherical Symmetry
- A galaxy lacking dark matter
- The massive relic galaxy NGC 1277 is dark matter deficient. From dynamical models of integral-field stellar kinematics out to five effective radii
- Strong bound on canonical ultra-light axion dark matter from the Lyman-alpha forest
- Axion Kinetic Misalignment Mechanism
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