Self-interacting dark scalar spikes around black holes via relativistic Bondi accretion

DOI10.1088/1475-7516/2022/08/032OpenAlexW4225716287MaRDI QIDQ5101141

Chian-Shu Chen, Feng-Li Lin, Alessandro Parisi, Wei-Xiang Feng

Publication date: 2 September 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2112.05160

zbMATH Keywords

accretionastrophysical fluid dynamicsdark matter theorymassive black holes

Mathematics Subject Classification ID

Black holes (83C57) Hydro- and aero-acoustics (76Q05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Dark matter and dark energy (83C56)

Cites Work

• Model-independent implications of the \(e^{\pm }\), \(\bar{p}\) cosmic ray spectra on properties of Dark Matter
• Dark matter self-interactions and small scale structure
• THE STRUCTURE AND FORMATION OF BOSON STARS
• Fundamental oscillation modes of self-interacting bosonic dark stars
• Dynamical instability of collapsed dark matter halos
• Dynamical boson stars

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