Video URL
https://pirsa.org/13070011Black hole evaporation and unitarity: a semi-classical resolution?
APA
Bardeen, J. (2013). Black hole evaporation and unitarity: a semi-classical resolution?. Perimeter Institute for Theoretical Physics. https://pirsa.org/13070011
MLA
Bardeen, James. Black hole evaporation and unitarity: a semi-classical resolution?. Perimeter Institute for Theoretical Physics, Jul. 10, 2013, https://pirsa.org/13070011
BibTex
@misc{ scivideos_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 for Theoretical Physics}, year = {2013}, month = {jul}, note = {PIRSA:13070011 see, \url{https://scivideos.org/pirsa/13070011}} }
Source RepositoryPIRSA
Talk Type
Conference
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.