Holographic Thermodynamics of Accelerating Black Holes


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


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


          @misc{ 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},
            year = {2018},
            month = {nov},
            note = {PIRSA:18110091 see, \url{https://pirsa.org}}

David Kubiznak Perimeter Institute for Theoretical Physics

Talk Type Scientific Series


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.