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Black holes in scalar-tensor gravity
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Black holes in scalar-tensor gravity
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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.
Forward citations
Cited by 14 Pith papers
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