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

By Theodorus M. Nieuwenhuizen. 2011

146 citations recorded by the source corpus.

The Schwarzschild--de Sitter and Reissner-Nordstr\"om--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-Nordstr\"om metrics.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/5bf5039398cb0382b6b710f4e4530f4a1a79ea9a

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Citations in the corpus

Theoretical Aspects of Massive Gravity (2011, background): “Other solutions, including some analytic solutions in various cases, are claimed in [91, 92, 93, 94, 95, 96].”
Massive Gravity (2014, background): “[478, 105, 61, 413, 277, 160, 38, 37, 39] for other spherically symmetric solutions in massive gravity.”
Massive Cosmologies (2011, background): “[12, 17] exhibit singularities at finite values of the coordinates, and hence, should be matched to other solutions before reaching those points.”
Helicity decomposition of ghost-free massive gravity (2011, background): “The allowed mass terms derived in [2] can be shown to arise as the expansion of the determinant √−g det[gν + λKν ] to fourth order in λ [16, 20, 21].”