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Electrovacuum Nearhorizon Geometries in Four and Five Dimensions
"... Associated to every stationary extremal black hole is a unique nearhorizon geometry, itself a solution of the field equations. These latter spacetimes are more tractable to analyze and most importantly, retain properties of the original black hole which are intrinsic to the event horizon. After rev ..."
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Associated to every stationary extremal black hole is a unique nearhorizon geometry, itself a solution of the field equations. These latter spacetimes are more tractable to analyze and most importantly, retain properties of the original black hole which are intrinsic to the event horizon. After
Near horizon geometry and black holes in four dimensions
 Nucl. Phys. B528
, 1998
"... A large class of extremal and nearextremal four dimensional black holes in Mtheory feature near horizon geometries that contain three dimensional asymptotically antide Sitter spaces. Globally, these geometries are derived from AdS3 by discrete identifications. The microstates of such black holes ..."
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Cited by 33 (7 self)
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A large class of extremal and nearextremal four dimensional black holes in Mtheory feature near horizon geometries that contain three dimensional asymptotically antide Sitter spaces. Globally, these geometries are derived from AdS3 by discrete identifications. The microstates of such black holes
Static nearhorizon geometries in five dimensions
, 907
"... We consider the classification of static nearhorizon geometries of stationary extremal (not necessarily BPS) black hole solutions of five dimensional EinsteinMaxwell theory coupled to a ChernSimons term with coupling ξ (with ξ = 1 corresponding to supergravity). Assuming the black holes have two ..."
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We consider the classification of static nearhorizon geometries of stationary extremal (not necessarily BPS) black hole solutions of five dimensional EinsteinMaxwell theory coupled to a ChernSimons term with coupling ξ (with ξ = 1 corresponding to supergravity). Assuming the black holes have two
THE NEARHORIZON GEOMETRY OF DILATONAXION BLACK HOLES
, 2001
"... Static black holes of dilatonaxion gravity become singular in the extreme limit, which prevents a direct determination of their nearhorizon geometry. This is addressed by first taking the nearhorizon limit of extreme rotating NUTless black holes, and then going to the static limit. The resulting ..."
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Static black holes of dilatonaxion gravity become singular in the extreme limit, which prevents a direct determination of their nearhorizon geometry. This is addressed by first taking the nearhorizon limit of extreme rotating NUTless black holes, and then going to the static limit
Nearhorizon geometries of supersymmetric AdS(5) black holes
 JHEP 12 (2007) 015; [arXiv:0708.3695]. 16 Hari K. Kunduri, James Lucietti and Harvey S. Reall, Supersymmetric multicharge AdS5 black holes, JHEP 04 (2006) 036; [hepth/0601156
"... We provide a classification of nearhorizon geometries of supersymmetric, asymptotically antide Sitter, black holes of fivedimensional U(1) 3gauged supergravity which admit two rotational symmetries. We find three possibilities: a topologically spherical horizon, an S 1 × S 2 horizon and a toroida ..."
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Cited by 27 (4 self)
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We provide a classification of nearhorizon geometries of supersymmetric, asymptotically antide Sitter, black holes of fivedimensional U(1) 3gauged supergravity which admit two rotational symmetries. We find three possibilities: a topologically spherical horizon, an S 1 × S 2 horizon and a
Dbranes in some nearhorizon geometries
, 2001
"... Abstract: I review some properties of Dbranes in the SU(2) and SL(2,R) WZW models. I comment on a potential difficulty for the realization of ‘warped brane worlds ’ in string theory. This short note is based on a talk given at the Strings’01 conference in Mumbay. Unité mixte du CNRS et de l’Ecole N ..."
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Cited by 2 (0 self)
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Abstract: I review some properties of Dbranes in the SU(2) and SL(2,R) WZW models. I comment on a potential difficulty for the realization of ‘warped brane worlds ’ in string theory. This short note is based on a talk given at the Strings’01 conference in Mumbay. Unité mixte du CNRS et de l’Ecole Normale Supérieure, UMR 8549. 1
Statistical Entropy of Magnetic Black Holes from NearHorizon Geometry
, 1998
"... Fourdimensional magnetic black holes including dilaton and abelian gauge fields which are solutions of supergravity can also be obtained by dimensional reduction of the EinsteinMaxwell gravity in five dimensions. In the extremal case the fivedimensional solutions have horizon and their nearhorizo ..."
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Cited by 1 (0 self)
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geometry is AdS3 × S 2. In the nonextremal case the nearhorizon geometry is shown to be the product of the threedimensional BañadosTeitelboimZanelli black hole and S 2. This allows to perform microscopic counting of statistical entropy of magnetic black holes. Exact agreement with the geometric
Results 1  10
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6,610