SUPERMASSIVE BLACK HOLES OR BOSON STARS? HAIR COUNTING WITH GRAVITATIONAL WAVE DETECTORS

DOI10.1142/S0218271806009637zbMath1112.83021arXivgr-qc/0605101OpenAlexW2126325759MaRDI QIDQ3434359

Emanuele Berti, Vitor Cardoso

Publication date: 25 April 2007

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0605101

zbMATH Keywords

black holegravitational wavesboson starsquasinormal modesno-hair theoremgravitational wave sources

Mathematics Subject Classification ID

Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75) Galactic and stellar structure (85A15) Gravitational waves (83C35)

Related Items (5)

Proca-Higgs balls and stars in a UV completion for Proca self-interactions ⋮ Tests for the existence of horizon through gravitational waves from a small binary in the vicinity of a massive object ⋮ Rotating boson stars using finite differences and global Newton methods ⋮ Dynamical boson stars ⋮ Dynamical boson stars

Cites Work

• General relativistic boson stars
• No observational proof of the black-hole event-horizon
• Evolution of 3D boson stars with waveform extraction
• Mapping spacetimes with LISA: inspiral of a test body in a ‘quasi-Kerr’ field

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