Stationary bound-state scalar configurations supported by rapidly-spinning exotic compact objects

DOI10.1016/J.PHYSLETB.2017.04.065zbMath1403.83021arXiv1803.07093OpenAlexW2608316787MaRDI QIDQ1631730

Shahar Hod

Publication date: 6 December 2018

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1803.07093

Mathematics Subject Classification ID

Black holes (83C57) Gravitational interaction in quantum theory (81V17)

Related Items (10)

Spontaneous scalarization of Gauss-Bonnet black holes surrounded by massive scalar fields ⋮ On instabilities of scalar hairy regular compact reflecting stars ⋮ Ultra-spinning exotic compact objects supporting static massless scalar field configurations ⋮ On instabilities of stationary scalar field configurations supported by reflecting compact stars ⋮ The longlived charged massive scalar field in the higher-dimensional Reissner-Nordström spacetime ⋮ No hair for spherically symmetric neutral reflecting stars: nonminimally coupled massive scalar fields ⋮ Isotropic compact stars in 4D Einstein–Gauss–Bonnet gravity ⋮ Quasibound states of the Dirac field in Schwarzschild and Reissner–Nordström black hole backgrounds ⋮ Scalarization of compact stars in the scalar-Gauss-Bonnet gravity ⋮ No hair theorem for bound-state massless static scalar fields outside horizonless Neumann compact stars

Cites Work

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• Ergosphere instability
• How to tell a gravastar from a black hole
• The fuzzball proposal for black holes: an elementary review

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