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Exact Schwarzschild-de Sitter black holes in a family of massive gravity models

Th. M. Nieuwenhuizen*

  • Center for Cosmology and Particle Physics, New York University, 4 Washington Place, New York, New York 10003, USA
  • Institute for Theoretical Physics, University of Amsterdam, Science Park 904, P.O. Box 94485, Amsterdam, The Netherlands

  • *t.m.nieuwenhuizen@uva.nl URL: http://staff.science.uva.nl/~nieuwenh/
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Phys. Rev. D 84, 024038 – Published 20 July, 2011

DOI: https://doi.org/10.1103/PhysRevD.84.024038

Abstract

The Schwarzschild–de Sitter and Reissner-Nordström–de Sitter black hole metrics appear as exact solutions in the recently formulated massive gravity of de Rham, Gabadadze and Tolley, where the mass term sets the curvature scale. They occur within a two-parameter family of de Rham, Gabadadze and Tolley mass terms. They show no trace of a cloud of scalar graviton modes, and in the limit of vanishing graviton mass they go smoothly to the Schwarzschild and Reissner-Nordström metrics.

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Outline

Information

Phys. Rev. D 84, 024038– Published 20 July, 2011
  • Received 29 March 2011

© 2011 American Physical Society

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