Black holes in scalar-tensor gravity

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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v1: 4 pages; v2: typos corrected, published version

Scientific paper

10.1103/PhysRevLett.108.081103

Hawking has proven that black holes which are stationary as the endpoint of
gravitational collapse in Brans--Dicke theory (without a potential) are no
different than in general relativity. We extend this proof to the much more
general class of scalar-tensor and f(R) gravity theories, without assuming any
symmetries apart from stationarity.

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