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• W2809817570 abstract "We study the superradiant instability of a massive boson around a spinning black hole in full general relativity without assuming spatial symmetries. We focus on the case of a rapidly spinning black hole in the presence of a vector boson with a Compton wavelength comparable to the black hole radius, which is the regime where relativistic effects are maximized. We follow the growth of the boson cloud through superradiance into the nonlinear regime as it spins down the black hole, reaches a maximum energy, and begins to dissipate through the emission of gravitational waves. We find that the superradiant instability can efficiently convert a significant fraction of a black hole's rotational energy into gravitational radiation." @default.
• W2809817570 created "2018-07-10" @default.
• W2809817570 creator A5086245101 @default.
• W2809817570 date "2018-09-26" @default.
• W2809817570 modified "2023-10-15" @default.
• W2809817570 title "Massive Boson Superradiant Instability of Black Holes: Nonlinear Growth, Saturation, and Gravitational Radiation" @default.
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• W2809817570 doi "https://doi.org/10.1103/physrevlett.121.131104" @default.
• W2809817570 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/30312089" @default.
• W2809817570 hasPublicationYear "2018" @default.
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