Eternal Black Holes in AdS
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In this paper, a dual non-perturbative description for maximally extended Schwarzschild anti-de-Sitter spacetimes is proposed, which involves two copies of the conformal field theory associated to the AdS spacetime and an initial entangled state.Abstract:
We propose a dual non-perturbative description for maximally extended Schwarzschild Anti-de-Sitter spacetimes. The description involves two copies of the conformal field theory associated to the AdS spacetime and an initial entangled state. In this context we also discuss a version of the information loss paradox and its resolution.read more
Citations
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Relaxation in conformal field theory, Hawking-Page transition, and quasinormal or normal modes
TL;DR: In this article, the authors studied the process of relaxation back to thermal equilibrium in a conformal field theory at finite temperature and showed that when the size of the system is much larger than the inverse temperature, perturbations decay exponentially with time.
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Quantum Regge Trajectories and the Virasoro Analytic Bootstrap
TL;DR: In this paper, the authors show that the double-twist data from the Virasoro vacuum module defines a "Virasoro Mean Field Theory" (VMFT), whose spectrum includes a finite number of discrete Regge trajectories whose dimensions obey a simple formula exact in the central charge c and external operator dimensions.
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Typicality versus thermality: an analytic distinction
Vijay Balasubramanian,Bartlomiej Czech,Veronika E. Hubeny,Klaus Larjo,Mukund Rangamani,Joan Simón,Joan Simón +6 more
TL;DR: In this paper, it was shown that the variance between micro-states of black holes will be exponentially suppressed in the entropy, by exploiting the analytic properties of correlation functions, thereby distinguishing pure states from the thermal density matrix.
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Complexity Growth Rate in Lovelock Gravity.
TL;DR: Using the complexity=action framework, the late time growth of complexity for charged black holes in Lovelock gravity is computed, finding in some cases a minimum mass below which complexity remains effectively constant, even if the black hole contains a nondegenerate horizon.
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Correlations in Hawking radiation and the infall problem
TL;DR: In this article, the entanglement entropy is computed numerically in order to find the order unity corrections to low-energy evolution at the horizon (i.e. fuzzballs) to remove entagglement between radiation and the hole.
References
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Anti De Sitter Space And Holography
TL;DR: In this article, it was shown that the Kaluza-Klein modes of Type IIB supergravity on $AdS_5\times {\bf S}^5$ match with the chiral operators of the super Yang-Mills theory in four dimensions.
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Gauge Theory Correlators from Non-Critical String Theory
TL;DR: In this paper, a boundary of the anti-deSitter space analogous to a cut-off on the Liouville coordinate of the two-dimensional string theory is introduced to obtain certain Green's functions in 3+1-dimensional N = 4 supersymmetric Yang-Mills theory with a large number of colors via non-critical string theory.
Book
Quantum Fields in Curved Space
N. D. Birrell,Paul Davies +1 more
TL;DR: A comprehensive review of the subject of gravitational effects in quantum field theory can be found in this paper, where special emphasis is given to the Hawking black hole evaporation effect, and to particle creation processes in the early universe.
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Anti-de Sitter Space, Thermal Phase Transition, And Confinement in Gauge Theories
TL;DR: The correspondence between supergravity and string theory on AdS space and boundary conformal eld theory relates the thermodynamics of N = 4 super Yang-Mills theory in four dimensions to the thermodynamic properties of Schwarzschild black holes in Anti-de Sitter space as mentioned in this paper.
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Breakdown of Predictability in Gravitational Collapse
TL;DR: In this paper, it is shown that the ignorance principle holds for the quantum-mechanical evaporation of black holes, where the black hole creates particles in pairs, with one particle always falling into the hole and the other possibly escaping to infinity.
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