The extreme orbital period in scalar hairy Kerr black holes
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Publication:2316110
DOI10.1016/j.physletb.2019.03.022zbMath1416.83060arXiv1901.02601OpenAlexW2909107054WikidataQ64296004 ScholiaQ64296004MaRDI QIDQ2316110
Publication date: 26 July 2019
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1901.02601
Related Items (6)
On instabilities of stationary scalar field configurations supported by reflecting compact stars ⋮ Hair distributions in noncommutative Einstein-Born-Infeld black holes ⋮ Lower bound on the radii of light rings in traceless black-hole spacetimes ⋮ Stationary scalar hairy configurations supported by Neumann compact stars ⋮ No-go theorem for static boson stars with negative cosmological constants ⋮ No hair theorem for spherically symmetric regular compact stars with Dirichlet boundary conditions
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