scholarly journals Holographic duals of black holes in five-dimensional minimal supergravity

2010 ◽  
Vol 27 (7) ◽  
pp. 075004 ◽  
Author(s):  
Chiang-Mei Chen ◽  
John E Wang
2010 ◽  
Vol 2010 (3) ◽  
Author(s):  
Chiang-Mei Chen ◽  
Ying-Ming Huang ◽  
Shou-Jyun Zou

2009 ◽  
Vol 2009 (04) ◽  
pp. 061-061 ◽  
Author(s):  
Tatsuo Azeyanagi ◽  
Noriaki Ogawa ◽  
Seiji Terashima

2019 ◽  
Vol 34 (32) ◽  
pp. 1950217 ◽  
Author(s):  
Jun-Jin Peng

In this paper, for the sake of providing a concrete comparison between the usual Abbott–Deser–Tekin (ADT) formalism and its off-shell extension, as well as comparing the latter with the Barnich–Brandt–Compere (BBC) approach, we carry out these methods to compute the mass and angular momentum of the rotating charged Gödel black holes in five-dimensional minimal supergravity. We first present the off-shell ADT potential of the supergravity theories in arbitrary odd dimensions, which is consistent with the superpotential via the BBC approach. Then the off-shell generalized ADT method is applied to evaluate the mass and angular momentum of the Gödel-type black holes by including the contribution from the gauge field. Finally, we strictly obey the rules of the original ADT formalism to incorporate the contribution from the gauge field within the potential. With the help of the modified potential, we try to seek for appropriate reference backgrounds to produce the mass and angular momentum. It is observed that the ADT formalism has to incorporate the contribution from the matter fields to yield physical charges for the Gödel-type black holes.


2017 ◽  
Vol 26 (13) ◽  
pp. 1750140 ◽  
Author(s):  
Alex Buchel

[Formula: see text] Type IIb supergravity compactifications on five-dimensional Einstein manifolds [Formula: see text] realize holographic duals to four-dimensional conformal field theories. Black holes in such geometries are dual to thermal states in these CFTs. When black holes become sufficiently small in (global) [Formula: see text], they are expected to suffer Gregory–Laflamme instability with respect to localization on [Formula: see text]. Previously, the instability was demonstrated for gravitational dual of [Formula: see text] SYM, where [Formula: see text]. We extend stability analysis to arbitrary [Formula: see text]. We point out that the quasinormal mode equation governing the instabilities is universal. The precise onset of the instability is [Formula: see text]-sensitive, as it is governed by the lowest nonvanishing eigenvalue [Formula: see text] of its Laplacian.


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