Results 31 to 40 of about 9,198 (296)
Rotating topological black holes
Physical Review D, 1998 25 pages, LateX, five ps figures added, minor errors corrected, addition of new references, improved discussion of the conserved ...
Moretti, Valter +2 more
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Uniqueness of near-horizon geometries of rotating extremal AdS(4) black holes [PDF]
, 2009 We consider stationary extremal black hole solutions of the Einstein-Maxwell equations with a negative cosmological constant in four dimensions. We determine all non-static axisymmetric near-horizon geometries and all static near-horizon geometries for ...
Lucietti, James, Kunduri, Hari K.
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Thermodynamics, stability and Hawking–Page transition of Kerr black holes from Rényi statistics
European Physical Journal C: Particles and Fields, 2017 Thermodynamics of rotating black holes described by the Rényi formula as equilibrium and zeroth law compatible entropy function is investigated. We show that similarly to the standard Boltzmann approach, isolated Kerr black holes are stable with respect ...
Viktor G. Czinner, Hideo Iguchi
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Black hole shadow of a rotating scale-dependent black hole [PDF]
Physical Review D, 2020 In this work, starting from a spherically symmetric scale--dependent black hole, a rotating solution is obtained by following the Newman--Janis algorithm without complexification. Besides studying the horizon, the static conditions and causality issues of the rotating solution, we get and discuss the shape of its shadow.
Ernesto Contreras +4 more
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Applications of Thermodynamic Geometries to Conformal Regular Black Holes: A Comparative Study
Universe, 2023 In this paper, we investigate the thermal stability and thermodynamic geometries of non-rotating/rotating charged black holes. For these black holes, we apply barrow entropy to determine the physical quantities such as mass and temperature of the system ...
Abdul Jawad +2 more
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ROTATING BRANEWORLD BLACK HOLES [PDF]
The Eleventh Marcel Grossmann Meeting, 2008 We present a Kerr-Newman type stationary and axisymmetric solution that describes rotating black holes with a tidal charge in the Randall-Sundrum braneworld. The tidal charge appears as an imprint of nonlocal gravitational effects from the bulk space.
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Black hole vacua and rotation [PDF]
Nuclear Physics B, 2011 Recent developments suggest that the near-region of rotating black holes behaves like a CFT. To understand this better, I propose to study quantum fields in this region. An instructive approach for this might be to put a large black hole in AdS and to think of the entire geometry as a toy model for the ``near-region".
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Holographic probes of inner horizons
Journal of High Energy Physics, 2020 We study the inner horizons of rotating and charged black holes in anti-de Sitter space. These black holes have a classical analytic extension through the inner horizon to additional asymptotic regions.
Vijay Balasubramanian +2 more
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Rotating Kaluza–Klein black holes [PDF]
Nuclear Physics B, 2000 All regular four-dimensional black holes are constructed in the theory obtained by Kaluza-Klein reduction of five-dimensional Einstein gravity. They are interpreted in string theory as rotating bound states of D0- and D6-branes. Conservation of angular momentum is important for the stability of the bound states.
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Accretion Into and Emission from Black Holes [PDF]
, 1976 Analyses are given of various processes involving matter falling into or coming out of black holes. A significant amount of matter may fall into a black hole in a galactic nucleus or in a binary system.
Page, Don Nelson
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