PIRSA:23110049

Video URL

https://pirsa.org/23110049

Black holes in cosmological settings: thermodynamics, semi-classical models, and applications - VIRTUAL

Simovic, F. (2023). Black holes in cosmological settings: thermodynamics, semi-classical models, and applications - VIRTUAL. Perimeter Institute for Theoretical Physics. https://pirsa.org/23110049

Simovic, Filip. Black holes in cosmological settings: thermodynamics, semi-classical models, and applications - VIRTUAL. Perimeter Institute for Theoretical Physics, Nov. 08, 2023, https://pirsa.org/23110049 

          @misc{ scivideos_PIRSA:23110049,
            doi = {10.48660/23110049},
            url = {https://pirsa.org/23110049},
            author = {Simovic, Filip},
            keywords = {Cosmology},
            language = {en},
            title = {Black holes in cosmological settings: thermodynamics, semi-classical models, and applications - VIRTUAL},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2023},
            month = {nov},
            note = {PIRSA:23110049 see, \url{https://scivideos.org/index.php/pirsa/23110049}}
          }

Filip Simovic University of Waterloo

Talk numberPIRSA:23110049
DOI10.48660/23110049
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Black hole thermodynamics plays a central role in the theoretical landscape, acting as both synthesizer and sieve for concepts in field theory, quantum gravity, information theory, and more. While its formulation and applications are well understood in asymptotically flat and anti-de Sitter spaces, significant difficulties arise when generalizing to cosmological settings. In this talk, I will discuss how the thermodynamic properties of black holes can be understood in such scenarios through the Euclidean path integral. I will also discuss black holes in a more generalized, semi-classical setting, and suggest a consistent framework for describing a wide variety of dynamical black hole models and ultracompact objects, with consequences for horizon formation, back-reaction, and the growth of astrophysical black holes.

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Zoom link https://pitp.zoom.us/j/97647270696?pwd=bXhFYWYyYUlrTEUyVXhtOUNDakhhQT09