Infinitesimally thin static scalar shells surrounding charged Gauss-Bonnet black holes

Abstract

We reveal the existence of a new form of spontaneously scalarized black-hole configurations. In particular, it is proved that Reissner-Nordström black holes in the highly charged regime $Q/M>(Q/M{)}_{\text{crit}}=\sqrt{21}/5$ can support {\it thin} matter shells that are made of massive scalar fields with a non-minimal coupling to the Gauss-Bonnet invariant of the curved spacetime. These static scalar shells, which become infinitesimally thin in the dimensionless large-mass $M\mu \gg 1$ regime, hover a finite proper distance above the black-hole horizon [here $\{M,Q\}$ are respectively the mass and electric charge of the central supporting black hole, and $\mu$ is the proper mass of the supported scalar field]. In addition, we derive a remarkably compact analytical formula for the discrete resonance spectrum $\{\eta (Q/M,M\mu ;n){\}}_{n=0}^{n=\infty }$ of the non-trivial coupling parameter which characterizes the bound-state charged-black-hole-thin-massive-scalar-shell cloudy configurations of the composed Einstein-Maxwell-scalar field theory.

arXiv comment17 pages

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Cited by in corpus (4)

• Spin-charge induced scalarization of Kerr-Newman black-hole spacetimes
• Nontrivial spatial behavior of the Gauss-Bonnet curvature invariant of rapidly-rotating Kerr black holes
• Non-equatorial scalar rings supported by magnetized Schwarzschild-Melvin black holes
• Higher dimensional Reissner-Nordström black holes supporting static scalar shells