PIRSA:13070011

Black hole evaporation and unitarity: a semi-classical resolution?

Bardeen, J. (2013). Black hole evaporation and unitarity: a semi-classical resolution?. Perimeter Institute. https://pirsa.org/13070011

Bardeen, James. Black hole evaporation and unitarity: a semi-classical resolution?. Perimeter Institute, Jul. 10, 2013, https://pirsa.org/13070011 

          @misc{ pirsa_PIRSA:13070011,
            doi = {10.48660/13070011},
            url = {https://pirsa.org/13070011},
            author = {Bardeen, James},
            keywords = {},
            language = {en},
            title = {Black hole evaporation and unitarity: a semi-classical resolution?},
            publisher = {Perimeter Institute},
            year = {2013},
            month = {jul},
            note = {PIRSA:13070011 see, \url{https://pirsa.org}}
          }

James Bardeen

Talk number
PIRSA:13070011
Collection
Talk Type
Abstract

I explore the possibility that semi-classical back-reaction, due to the partners of the Hawking radiation quanta accumulating over the time for the black hole to lose about one half of its mass (the Page time), might cause the trapped surfaces to disappear, permitting unitary evolution without any cloning of quantum information.