Last gasp of a black hole: why unitary evaporation must be non-monotonic
APA
Smerlak, M. (2014). Last gasp of a black hole: why unitary evaporation must be non-monotonic. Perimeter Institute. https://pirsa.org/14050027
MLA
Smerlak, Matteo. Last gasp of a black hole: why unitary evaporation must be non-monotonic. Perimeter Institute, May. 29, 2014, https://pirsa.org/14050027
BibTex
@misc{ pirsa_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}, year = {2014}, month = {may}, note = {PIRSA:14050027 see, \url{https://pirsa.org}} }
Capital Fund Management S.A.
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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.