scholarly journals Scalar, electromagnetic, and Weyl perturbations of BTZ black holes: Quasinormal modes

2001 ◽  
Vol 63 (12) ◽  
Author(s):  
Vitor Cardoso ◽  
José P. S. Lemos
Keyword(s):  
Black Holes ◽  
Quasinormal Modes ◽  
Btz Black Holes

scholarly journals Dirac quasinormal modes of Chern-Simons and BTZ black holes with torsion

2014 ◽  
Vol 89 (2) ◽  
Author(s):  
Ramón Bécar ◽  
P. A. González ◽  
Y. Vásquez
Keyword(s):  
Black Holes ◽  
Quasinormal Modes ◽  
Btz Black Holes ◽  
Chern Simons

scholarly journals Massive Dirac quasinormal modes in Schwarzschild–de Sitter black holes: Anomalous decay rate and fine structure

2021 ◽  
Vol 103 (6) ◽  
Author(s):  
Almendra Aragón ◽  
Ramón Bécar ◽  
P. A. González ◽  
Yerko Vásquez
Keyword(s):  
Black Holes ◽  
Fine Structure ◽  
Decay Rate ◽  
Quasinormal Modes ◽  
De Sitter

scholarly journals Quasinormal modes of growing dirty black holes

2021 ◽  
Vol 103 (12) ◽  
Author(s):  
Jamie Bamber ◽  
Oliver J. Tattersall ◽  
Katy Clough ◽  
Pedro G. Ferreira
Keyword(s):  
Black Holes ◽  
Quasinormal Modes

scholarly journals Slow scrambling in extremal BTZ and microstate geometries

2021 ◽  
Vol 2021 (3) ◽  
Author(s):  
Ben Craps ◽  
Marine De Clerck ◽  
Philip Hacker ◽  
Kévin Nguyen ◽  
Charles Rabideau
Keyword(s):  
Field Theory ◽  
Black Holes ◽  
Degrees Of Freedom ◽  
Average Power ◽  
Nonzero Temperature ◽  
Time Intervals ◽  
Conformal Field ◽  
Btz Black Holes ◽  
The Right ◽  
Extremal Black Holes

Abstract Out-of-time-order correlators (OTOCs) that capture maximally chaotic properties of a black hole are determined by scattering processes near the horizon. This prompts the question to what extent OTOCs display chaotic behaviour in horizonless microstate geometries. This question is complicated by the fact that Lyapunov growth of OTOCs requires nonzero temperature, whereas constructions of microstate geometries have been mostly restricted to extremal black holes.In this paper, we compute OTOCs for a class of extremal black holes, namely maximally rotating BTZ black holes, and show that on average they display “slow scrambling”, characterized by cubic (rather than exponential) growth. Superposed on this average power-law growth is a sawtooth pattern, whose steep parts correspond to brief periods of Lyapunov growth associated to the nonzero temperature of the right-moving degrees of freedom in a dual conformal field theory.Next we study the extent to which these OTOCs are modified in certain “superstrata”, horizonless microstate geometries corresponding to these black holes. Rather than an infinite throat ending on a horizon, these geometries have a very deep but finite throat ending in a cap. We find that the superstrata display the same slow scrambling as maximally rotating BTZ black holes, except that for large enough time intervals the growth of the OTOC is cut off by effects related to the cap region, some of which we evaluate explicitly.

scholarly journals Quasinormal modes of (anti-)de Sitter black holes in the 1/D expansion

2015 ◽  
Vol 2015 (4) ◽  
Author(s):  
Roberto Emparan ◽  
Ryotaku Suzuki ◽  
Kentaro Tanabe
Keyword(s):  
Black Holes ◽  
Quasinormal Modes ◽  
De Sitter
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