Black Holes in Scalar-Tensor Gravity

Type: Article

Publication Date: 2012-02-24

Citations: 350

DOI: https://doi.org/10.1103/physrevlett.108.081103

Abstract

Hawking has proven that black holes which are stationary as the end point 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.

Locations

  • Physical Review Letters - View
  • arXiv (Cornell University) - View - PDF
  • PubMed - View
  • DataCite API - View

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