2012

Exact Hairy Black Holes and their Modification to the Universal Law of Gravitation

Anabalon, Andres, Oliva, Julio

Understand

In this paper two things are done.

First, it is pointed out the existence of exact asymptotically flat, spherically symmetric black holes when a self interacting, minimally coupled scalar field is the source of the energy momentum of the Einstein equations in four dimensions.
The scalar field potential is the recently found to be compatible with the hairy generalization of the Plebanski-Demianski solution of general relativity.
This paper describes the spherically symmetric solutions that smoothly connect the Schwarzschild black hole with its hairy counterpart.

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Cited alongside, same era.
U. Nucamendi and M. Salgado, “Scalar hairy black holes and solitons in asymptotically flat space-times,” Phys. Rev. D 68
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Cited alongside, same era.
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2007
Cited alongside, same era.
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Original
Cited in the paper.
P. Amaro-Seoane, “Stellar dynamics and extreme-mass ratio inspirals,” arXiv:1205.5240 [astro-ph.CO]
Original
Cited in the paper.

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