PIRSA:23080018

Talk 22 - Microstates of a 2d Black Hole in string theory

APA

Betzios, P. (2023). Talk 22 - Microstates of a 2d Black Hole in string theory. Perimeter Institute for Theoretical Physics. https://pirsa.org/23080018

MLA

Betzios, Panagiotis. Talk 22 - Microstates of a 2d Black Hole in string theory. Perimeter Institute for Theoretical Physics, Aug. 03, 2023, https://pirsa.org/23080018

BibTex

          @misc{ scivideos_PIRSA:23080018,
            doi = {10.48660/23080018},
            url = {https://pirsa.org/23080018},
            author = {Betzios, Panagiotis},
            keywords = {Quantum Fields and Strings, Quantum Information, Quantum Foundations},
            language = {en},
            title = {Talk 22 - Microstates of a 2d Black Hole in string theory},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2023},
            month = {aug},
            note = {PIRSA:23080018 see, \url{https://scivideos.org/index.php/pirsa/23080018}}
          }
          

Panagiotis Betzios University of British Columbia

Talk numberPIRSA:23080018
Source RepositoryPIRSA
Collection

Abstract

We analyse models of Matrix Quantum Mechanics in the double scaling limit that contain non-singlet states. The finite temperature partition function of such systems contains non-trivial winding modes (vortices) and is expressed in terms of a group theoretic sum over representations. We then focus on the model of Kazakov-Kostov-Kutasov when the first winding mode is dominant. In the limit of large representations (continuous Young diagrams), and depending on the values of the parameters of the model such as the compactification radius and the string coupling, the dual geometric background corresponds either to that of a long string (winding mode) condensate or a 2d (non-supersymmetric) semi-classical Black Hole competing with the thermal linear dilaton background. In the matrix model we are free to tune these parameters and explore various regimes of this phase diagram. Our construction allows us to identify the origin of the microstates of the long string condensate/2d Black Hole arising from the non trivial representations.