Impact of multiple modes on the evolution of self-interacting axion condensate around rotating black holes

DOI10.1088/1475-7516/2023/06/016zbMath1528.83081arXiv2211.01949MaRDI QIDQ6173863

Hirotaka Yoshino, Hidetoshi Omiya, Takahiro Tanaka, Takuya Takahashi

Publication date: 13 July 2023

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

Full work available at URL: https://arxiv.org/abs/2211.01949

zbMATH Keywords

axionsastrophysical black holesgravitational waves/sources

Mathematics Subject Classification ID

Other elementary particle theory in quantum theory (81V25) Black holes (83C57) Signal detection and filtering (aspects of stochastic processes) (60G35) Phase transitions (general) in equilibrium statistical mechanics (82B26) Gravitational waves (83C35) Motion of the gyroscope (70E05) Derivations, dissipations and positive semigroups in (C^*)-algebras (46L57)

Related Items (1)

Dynamical friction in gravitational atoms

Cites Work

• The type IIB string axiverse and its low-energy phenomenology
• Aspects of nonlinear effect on black hole superradiance
• Black holes as particle detectors: evolution of superradiant instabilities
• The bosenova and axiverse
• Bosenova Collapse of Axion Cloud around a Rotating Black Hole
• Axion clouds may survive the perturbative tidal interaction over the early inspiral phase of black hole binaries
• Axion cloud evaporation during inspiral of black hole binaries: The effects of backreaction and radiation
• Adiabatic evolution of the self-interacting axion field around rotating black holes
• Renormalization group analysis of superradiant growth of self-interacting axion cloud

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