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Thermodynamics of Computation

Difference between revisions of "Holographic Second Laws of Black Hole Thermodynamics"

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(Created page with "{{Reference Material |title=Holographic Second Laws of Black Hole Thermodynamics |reference groups=General Non-equilibrium Statistical Physics |Related videos=Alice Bernamonti...")
 
 
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|title=Holographic Second Laws of Black Hole Thermodynamics
 
|title=Holographic Second Laws of Black Hole Thermodynamics
 
|reference groups=General Non-equilibrium Statistical Physics
 
|reference groups=General Non-equilibrium Statistical Physics
|Related videos=Alice Bernamonti
 
Federico Galli
 
Robert C. Myers
 
Jonathan Oppenheim
 
 
|authors=Alice Bernamonti; Federico Galli; Robert C. Myers; Jonathan Oppenheim
 
|authors=Alice Bernamonti; Federico Galli; Robert C. Myers; Jonathan Oppenheim
 
|primary author last name=Bernamonti
 
|primary author last name=Bernamonti

Latest revision as of 11:15, June 24, 2019

reference groups
General Non-equilibrium Statistical Physics
author-supplied keywords
keywords
authors
Alice Bernamonti
Federico Galli
Robert C. Myers
Jonathan Oppenheim
title
Holographic Second Laws of Black Hole Thermodynamics
type
journal
year
2018
pages
70
volume
2018
issue
6
publisher
Springer Nature
abstract
Recently, it has been shown that for out-of-equilibrium systems, there are additional constraints on thermodynamical evolution besides the ordinary second law. These form a new family of second laws of thermodynamics, which are equivalent to the monotonicity of quantum Rényi divergences. In black hole thermodynamics, the usual second law is manifest as the area increase theorem. Hence one may ask if these additional laws imply new restrictions for gravitational dynamics, such as for out-of-equilibrium black holes? Inspired by this question, we study these constraints within the AdS/CFT correspondence. First, we show that the Rényi divergence can be computed via a Euclidean path integral for a certain class of excited CFT states. Applying this construction to the boundary CFT, the Rényi divergence is evaluated as the renormalized action for a particular bulk solution of a minimally coupled gravity-scalar system. Further, within this framework, we show that there exist transitions which are allowed by the traditional second law, but forbidden by the additional thermodynamical constraints. We speculate on the implications of our findings.


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