Spinning boson stars and Kerr black holes with scalar hair: The effect of self-interactions
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Publication:2826543
DOI10.1142/S0218271816410145zbMath1347.83022arXiv1604.06202WikidataQ59688826 ScholiaQ59688826MaRDI QIDQ2826543
Eugen Radu, Helgi Rúnarsson, Carlos A. R. Herdeiro
Publication date: 17 October 2016
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1604.06202
Related Items (8)
Spinning Kerr black holes with stationary massive scalar clouds: the large-coupling regime ⋮ Proca-Higgs balls and stars in a UV completion for Proca self-interactions ⋮ Rotating black holes with non-Abelian hair ⋮ Gravitating solitons and black holes with synchronised hair in the four dimensional O(3) sigma-model ⋮ Compact objects and the swampland ⋮ Onset of superradiant instabilities in rotating spacetimes of exotic compact objects ⋮ Weak cosmic censorship with self-interacting scalar and bound on charge to mass ratio ⋮ Dynamical boson stars
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