Results 21 to 30 of about 729,890 (281)
Black hole thermodynamics without a black hole? [PDF]
20 pages, it will be submitted to Phys.Lett ...
openaire +4 more sources
Black holes and the multiverse [PDF]
49 pages, 15 figures, matches version to appear in ...
Jaume Garriga+3 more
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The Thermodynamics of Black Holes [PDF]
46 pages, no figures, plain latex file; submitted to Living Reviews in Relativity.
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We present novel asymptotically global AdS4 solutions, constructed by turning on a dipolar differential rotation at the conformal boundary. At fixed energy and boundary profile, we find two different geometries: a horizonless spacetime, and a deformed, hourglass shaped black hole with zero net angular momentum.
Markeviciute, Julija, Santos, Jorge E
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Thermodynamics of third order Lovelock anti-de Sitter black holes revisited
We compute the mass and the temperature of third order Lovelock black holes with negative Gauss-Bonnet coefficient ...
D. Birmingham+7 more
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Black hole masking and black hole thermodynamics [PDF]
Masking of black holes means that, for given total mass and Hawking temperatures, these data may correspond to either "pure" black hole or a black hole of a lesser mass surrounded by a massive shell. It is shown that there is one-to one correspondence between this phenomenon and thermodynamics of a black hole in a finite size cavity: masking of black ...
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Do stringy corrections stabilize coloured black holes? [PDF]
We consider hairy black hole solutions of Einstein-Yang-Mills-Dilaton theory, coupled to a Gauss-Bonnet curvature term, and we study their stability under small, spacetime-dependent perturbations. We demonstrate that the stringy corrections do not remove
A. Messiah+32 more
core +2 more sources
Holographic complexity of Born-Infeld black holes
In this paper, according to CA duality, we study complexity growth of Born-Infeld (BI) black holes. As a comparison, we study action growth of dyonic black holes in Einstein-Maxwell gravity at the beginning.
Meng, Kun
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We study six-dimensional rotating black holes with bumpy horizons: these are topologically spherical, but the sizes of symmetric cycles on the horizon vary non-monotonically with the polar angle. We construct them numerically for the first three bumpy families, and follow them in solution space until they approach critical solutions with localized ...
Roberto Emparan+3 more
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On Universal Black Holes [PDF]
4 pages. Short summary of arXiv:1907.08788. Presented at the 6th Conference of the Polish Society on Relativity, Szczecin, Poland, September 23--26 ...
Hervik, S., Ortaggio, M. (Marcello)
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