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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On the Time Dependence of Holographic Complexity
Dean Carmi,Dean Carmi,Shira Chapman,Hugo Marrochio,Hugo Marrochio,Robert C. Myers,Sotaro Sugishita,Sotaro Sugishita +7 more
TL;DR: In this paper, the authors evaluate the full time dependence of holographic complexity in various eternal black hole backgrounds using both the complexity=action (CA) and the complexity-volume (CV) conjectures and conclude that the rate of change of complexity is a monotonically increasing function of time, which saturates from below to a positive constant in the late time limit.
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Black Hole Microstate Cosmology
TL;DR: In this paper, the authors explore the possibility that certain high-energy holographic CFT states correspond to black hole microstates with a geometrical behind-the-horizon region, modelled by a portion of a second asymptotic region terminating at an end-of-theworld (ETW) brane.
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Brane-antibrane systems at finite temperature and the entropy of black branes
TL;DR: In this article, a microscopic brane-antibrane model for D-brane-anti-Dbrane systems at T > 0 was proposed, where the negative specific heat and pressure of the black brane have a simple interpretation in terms of brane antibrane annihilation.
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Measuring Black Hole Formations by Entanglement Entropy via Coarse-Graining
TL;DR: In this article, it was shown that the total von-Neumann entropy remains vanishing even when a black hole is created in a gravity dual, being consistent with the fact that its corresponding CFT is described by a time-dependent pure state.
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Flat entanglement spectra in fixed-area states of quantum gravity
TL;DR: In this paper, the authors use the Einstein-Hilbert path integral to investigate gravitational entanglement at leading order $O(1/G) and show that the reduced density matrix can be approximated as proportional to the identity to the extent that its Renyi entropies $S_n$ are independent of $n$ at this order.
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.
Journal ArticleDOI
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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