PIRSA:14050027

Video URL

https://pirsa.org/14050027

Last gasp ‎of a black hole: why unitary evaporation must be non-monotonic

Smerlak, M. (2014). Last gasp ‎of a black hole: why unitary evaporation must be non-monotonic. Perimeter Institute for Theoretical Physics. https://pirsa.org/14050027

Smerlak, Matteo. Last gasp ‎of a black hole: why unitary evaporation must be non-monotonic. Perimeter Institute for Theoretical Physics, May. 29, 2014, https://pirsa.org/14050027 

          @misc{ scivideos_PIRSA:14050027,
            doi = {10.48660/14050027},
            url = {https://pirsa.org/14050027},
            author = {Smerlak, Matteo},
            keywords = {Quantum Gravity},
            language = {en},
            title = {Last gasp ‎of a black hole: why unitary evaporation must be non-monotonic},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2014},
            month = {may},
            note = {PIRSA:14050027 see, \url{https://scivideos.org/pirsa/14050027}}
          }

Matteo Smerlak Capital Fund Management S.A.

Talk numberPIRSA:14050027
DOI10.48660/14050027
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

I will describe the relationship between radiated energy and entanglement entropy of massless fields at future null infinity (the "Page curve") in two-dimensional models of black hole evaporation. ‎I will use this connection to derive a general feature of any unitary-preserving evaporation scenario: the Bondi mass of the hole must be non-monotonic. Time permitting, I will comment on time scales in such scenarios.