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Steady states of holographic interfaces

TLDR
In this article, the authors show that the thermal conductivity of a pair of interfaces jumps at the Hawking-Page phase transition from a regime described by classical scatterers to a quantum regime in which heat flows unobstructed.
Abstract
We find stationary thin-brane geometries that are dual to far-from-equilibrium steady states of two-dimensional holographic interfaces. The flow of heat at the boundary agrees with the result of CFT and the known energy-transport coefficients of the thin-brane model. We argue that by entangling outgoing excitations the interface produces thermodynamic entropy at a maximal rate, and point out similarities and differences with double-sided black funnels. The non-compact, non-Killing and far-from-equilibrium event horizon of our solutions coincides with the local (apparent) horizon on the colder side, but lies behind it on the hotter side of the interface. We also show that the thermal conductivity of a pair of interfaces jumps at the Hawking-Page phase transition from a regime described by classical scatterers to a quantum regime in which heat flows unobstructed.

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Sailing past the End of the World and discovering the Island

TL;DR: In this article , the authors explore a family of models obtained by coupling two holographic CFTs along a shared interface (ICFTs), where the bulk solution is characterized by a thin brane separating the two individual duals.
Journal ArticleDOI

Sailing past the End of the World and discovering the Island

- 30 Sep 2022 - 
TL;DR: In this paper , the authors explore a family of models obtained by coupling two holographic CFTs along a shared interface (ICFTs), where the bulk solution is characterized by a thin brane separating the two individual duals.
Journal ArticleDOI

Reflected entropy in boundary and interface conformal field theory

Yuya Kusuki
- 12 Sep 2022 - 
TL;DR: In this article , the authors introduce the left-right reflected entropy (LRRE) in BCFT and show that its holographic dual is given by the area of the entanglement wedge cross section (EWCS) through AdS/BCFT.
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Energy Transport for Thick Holographic Branes

TL;DR: In this paper , the authors developed a method that allows them to extend previous results based on thin-brane holographic models to smooth domain-wall solutions of 3D gravity, and compute the transmission coefficient of a Janus interface in terms of its deformation parameter.
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Energy Transport for Thick Holographic Branes

TL;DR: In this article , the authors use results for the energy transmission in thin-brane holographic models to compute the transmission coefficient of a Janus interface in terms of its deformation parameter.
References
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Journal ArticleDOI

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.
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Holographic Derivation of Entanglement Entropy from the anti de Sitter Space/Conformal Field Theory Correspondence

TL;DR: It is argued that the entanglement entropy in d + 1 dimensional conformal field theories can be obtained from the area of d dimensional minimal surfaces in AdS(d+2), analogous to the Bekenstein-Hawking formula for black hole entropy.
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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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Black hole in three-dimensional spacetime.

TL;DR: The standard Einstein-Maxwell equations in 2+1 spacetime dimensions, with a negative cosmological constant, admit a black hole solution that appears as a negative energy state separated by a mass gap from the continuous black hole spectrum.
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