Dynamical friction in gravitational atoms
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Publication:6175033
DOI10.1088/1475-7516/2023/07/070arXiv2305.15460MaRDI QIDQ6175033
Unnamed Author, Unnamed Author, Gianfranco Bertone
Publication date: 17 August 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2305.15460
Black holes (83C57) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35)
Cites Work
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- Testing string vacua in the lab: from a hidden CMB to dark forces in flux compactifications
- The impact of realistic models of mass segregation on the event rate of extreme-mass ratio inspirals and cusp re-growth
- Axion clouds may survive the perturbative tidal interaction over the early inspiral phase of black hole binaries
- The spectra of gravitational atoms
- Axion cloud evaporation during inspiral of black hole binaries: The effects of backreaction and radiation
- Gravitational Radiation from Point Masses in a Keplerian Orbit
- Dynamical Friction. I. General Considerations: the Coefficient of Dynamical Friction.
- Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals
- Impact of multiple modes on the evolution of self-interacting axion condensate around rotating black holes
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