PIRSA:19100054

Evaporating Black-to-White Hole

APA

Martin-Dussaud, P. (2019). Evaporating Black-to-White Hole. Perimeter Institute for Theoretical Physics. https://pirsa.org/19100054

MLA

Martin-Dussaud, Pierre. Evaporating Black-to-White Hole. Perimeter Institute for Theoretical Physics, Oct. 10, 2019, https://pirsa.org/19100054

BibTex

          @misc{ scivideos_PIRSA:19100054,
            doi = {10.48660/19100054},
            url = {https://pirsa.org/19100054},
            author = {Martin-Dussaud, Pierre},
            keywords = {Quantum Gravity},
            language = {en},
            title = {Evaporating Black-to-White Hole},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2019},
            month = {oct},
            note = {PIRSA:19100054 see, \url{https://scivideos.org/index.php/pirsa/19100054}}
          }
          

Pierre Martin-Dussaud Aix-Marseille University

Talk numberPIRSA:19100054
Source RepositoryPIRSA
Collection

Abstract

What is the ultimate fate of black holes? Since the discovery of Hawking evaporation process, the issue has been much discussed. Loop quantum gravity suggests that black hole could ultimately turn into white holes. In this talk, we investigate several possible mixed scenario where black holes first evaporate to a Planckian size before tunnelling to white holes. We build various spacetime models, taking Hawking backreaction into account, and we discuss some aspects of the expected phenomenology. Finally, we will draw the path for a full LQG amplitude computation that could lead to observational predictions.