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Anti-Evaporation of Black Holes in Bigravity

Department of Physics, Nagoya University, Nagoya 464-8602, Japan
Academic Editors: Kazuharu Bamba and Sergei D. Odintsov
Universe 2015, 1(2), 158-172;
Received: 26 March 2015 / Revised: 10 July 2015 / Accepted: 22 July 2015 / Published: 3 August 2015
(This article belongs to the Special Issue Modified Gravity Cosmology: From Inflation to Dark Energy)
We review properties of solutions in bigravity theory for a specific case where two metric tensors, \(g_{\mu \nu}\) and \(f_{\mu \nu}\), satisfy proportional relation \(f_{\mu \nu}=C^{2}g_{\mu \nu}\). For this condition, we find that the solutions describing the asymptotically de Sitter space-time can be obtained and investigate the perturbation around the Schwarzschild–de Sitter solutions and corresponding anti-evaporation. We discuss the stability under special perturbations related to the anti-evaporation and the importance of the non-diagonal components of the metric in bigravity. View Full-Text
Keywords: modified gravity; bigravity; quantum field theory modified gravity; bigravity; quantum field theory
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Katsuragawa, T. Anti-Evaporation of Black Holes in Bigravity. Universe 2015, 1, 158-172.

AMA Style

Katsuragawa T. Anti-Evaporation of Black Holes in Bigravity. Universe. 2015; 1(2):158-172.

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Katsuragawa, Taishi. 2015. "Anti-Evaporation of Black Holes in Bigravity" Universe 1, no. 2: 158-172.

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