PIRSA:18110091

Video URL

https://pirsa.org/18110091

Holographic Thermodynamics of Accelerating Black Holes

Kubiznak, D. (2018). Holographic Thermodynamics of Accelerating Black Holes. Perimeter Institute for Theoretical Physics. https://pirsa.org/18110091

Kubiznak, David. Holographic Thermodynamics of Accelerating Black Holes. Perimeter Institute for Theoretical Physics, Nov. 22, 2018, https://pirsa.org/18110091 

          @misc{ scivideos_PIRSA:18110091,
            doi = {10.48660/18110091},
            url = {https://pirsa.org/18110091},
            author = {Kubiznak, David},
            keywords = {Strong Gravity},
            language = {en},
            title = {Holographic Thermodynamics of Accelerating Black Holes},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2018},
            month = {nov},
            note = {PIRSA:18110091 see, \url{https://scivideos.org/pirsa/18110091}}
          }

David Kubiznak Charles University

Talk numberPIRSA:18110091
DOI10.48660/18110091
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

I will address a long-standing problem of describing the thermodynamics of an accelerating black hole, concentrating on the special case of slowly accelerating black holes in AdS. The key
ingredient of consistent thermodynamics is to ensure that the system is not over-constrained by including the possibility of varying the string tensions that are responsible for the acceleration of the black hole. The first law assumes the standard form, with the entropy given by one quarter of the horizon area and other quantities identified by standard methods. The dual
energy-momentum tensor can be written as a three-dimensional perfect fluid plus a non-hydrodynamic contribution. Some novel thermodynamic phase behavior related to the black hole acceleration will also be discussed.