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In mimetic gravity, we derive $D$-dimension charged black hole solutions having flat or cylindrical horizons with zero curvature boundary.
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Irina Dymnikova and Michal Korpusik, “Regular black hole remnants in de Sitter space,” Phys. Lett. , 12–18 (2010)
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Salvatore Capozziello and Mariafelicia De Laurentis, “Extended Theories of Gravity,” Phys. Rept. 509
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2011
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2011
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2011
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Valerio Faraoni and Salvatore Capozziello, Beyond Einstein Gravity , Vol. 170 (Springer, Dordrecht, 2011)
2011
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2011
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Irina Dymnikova and Michał Korpusik, “Thermodynamics of regular cosmological black holes with the de sitter interior,” Entropy 13
2011
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M. I. Wanas, “The other side of gravity and geometry: Antigravity and anticurvature,” Adv. High Energy Phys. 2012
2012
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2016
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K. Ghaderi and B. Malakolkalami, “Thermodynamics of the Schwarzschild and the ReissnerNordström black holes with quintessence,” Nucl. Phys. , 10–18 (2016)
2016
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2017
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Andrea Addazi and Antonino Marciano, “Evaporation and Antievaporation instabilities,” Symmetry 9
2017
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Rampei Kimura, Atsushi Naruko, and Daisuke Yoshida, “Extended vector-tensor theories,” JCAP 1701
2017
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Sunny Vagnozzi, “Recovering a MOND-like acceleration law in mimetic gravity,” Class. Quant. Grav. 34
2017
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Irina Dymnikova, “Generic Features of Thermodynamics of Horizons in Regular Spherical Space-Times of the Kerr-Schild Class,” Universe 4
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