Stationary bound-state scalar configurations supported by rapidly-spinning exotic compact objects
arXiv:1803.07093 · doi:10.1016/j.physletb.2017.04.065
Abstract
Some quantum-gravity theories suggest that the absorbing horizon of a classical black hole should be replaced by a reflective surface which is located a microscopic distance above the would-be classical horizon. Instead of an absorbing black hole, the resulting horizonless spacetime describes a reflective exotic compact object. Motivated by this intriguing prediction, in the present paper we explore the physical properties of exotic compact objects which are linearly coupled to stationary bound-state massive scalar field configurations. In particular, solving the Klein-Gordon wave equation for a stationary scalar field of proper mass and spheroidal harmonic indices in the background of a rapidly-rotating exotic compact object of mass and angular momentum , we derive a compact analytical formula for the {\it discrete} radii of the exotic compact objects which can support the stationary bound-state massive scalar field configurations. We confirm our analytical results by direct numerical computations.
11 pages. arXiv admin note: text overlap with arXiv:1704.05856
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