Reissner–Nordström Anti-de Sitter Black Holes in Mimetic F(R) Gravity
Departement of of Physics, Tomsk State Pedagogical University, Tomsk 634061, Russia
Laboratory of Theoretical Cosmology, Tomsk State University of Control Systems and Radioelectronics (TUSUR), Tomsk 634050, Russia
Academic Editor: Gonzalo J. Olmo
Received: 18 April 2016 / Revised: 11 May 2016 / Accepted: 18 May 2016 / Published: 30 May 2016
In this paper, we study under which conditions the Reissner–Nordström anti-de Sitter black hole can be a solution of the vacuum mimetic
gravity with Lagrange multiplier and mimetic scalar potential. As the author demonstrates, the resulting picture in the mimetic
gravity case is a trivial extension of the standard
approach, and in effect, the metric perturbations in the mimetic
gravity case, for the Reissner–Nordström anti-de Sitter black hole metric, at the first order of the perturbed variables are the same at the leading order.
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MDPI and ACS Style
Oikonomou, V.K. Reissner–Nordström Anti-de Sitter Black Holes in Mimetic F(R) Gravity. Universe 2016, 2, 10.
Oikonomou VK. Reissner–Nordström Anti-de Sitter Black Holes in Mimetic F(R) Gravity. Universe. 2016; 2(2):10.
Oikonomou, V. K. 2016. "Reissner–Nordström Anti-de Sitter Black Holes in Mimetic F(R) Gravity." Universe 2, no. 2: 10.
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