Effect of scalar field mass on gravitating charged scalar solitons and black holes in a cavity

DOI10.1016/j.physletb.2016.10.073zbMath1369.83082arXiv1610.00135OpenAlexW2528321145WikidataQ62476399 ScholiaQ62476399MaRDI QIDQ2399098

Elizabeth Winstanley, Supakchai Ponglertsakul

Publication date: 21 August 2017

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

Full work available at URL: https://arxiv.org/abs/1610.00135

zbMATH Keywords

solitonsblack holesEinstein charged scalar field theory

Mathematics Subject Classification ID

Black holes (83C57) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (15)

Final state of instabilities in Born-Infeld black holes ⋮ On instabilities of scalar hairy regular compact reflecting stars ⋮ On the dual relation in the Hawking-Page phase transition of the black holes in a cavity ⋮ Hairy black holes in a box ⋮ Spinning Kerr black holes with stationary massive scalar clouds: the large-coupling regime ⋮ Studies of a general flat space/boson star transition model in a box through a language similar to holographic superconductors ⋮ Dynamical formation of a hairy black hole in a cavity from the decay of unstable solitons ⋮ No-go theorem for static boson stars ⋮ Scalar field configurations supported by charged compact reflecting stars in a curved spacetime ⋮ Boson stars and solitons confined in a Minkowski box ⋮ Phase diagram of the charged black hole bomb system ⋮ Einstein-Charged Scalar Field Theory: Black Hole Solutions and Their Stability ⋮ Thermodynamics and phase transition of a nonlinear electrodynamics black hole in a cavity ⋮ Superradiant instability and asymptotically AdS hairy black holes in \(F(R)\)-charged scalar field theory ⋮ Charged black hole bombs in a Minkowski cavity

Cites Work

• The charged black-hole bomb: a lower bound on the charge-to-mass ratio of the explosive scalar field

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