Page curve for an evaporating black hole
Page curve for an evaporating black hole
A Page curve for an evaporating black hole in asymptotically flat spacetime is computed by adapting the Quantum Ryu-Takayanagi (QRT) proposal to an analytically solvable semi-classical two-dimensional dilaton gravity theory. The Page time is found to be one third of the black hole lifetime, at leading order in semi-classical corrections. A Page curve is also obtained for a semi-classical eternal black hole, where energy loss due to Hawking evaporation is balanced by an incoming energy flux.
Gautason, Fridrik Freyr
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Schneiderbauer, Lukas
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Sybesma, Watse
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Thorlacius, Larus
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20 May 2020
Gautason, Fridrik Freyr
0c48d448-e092-48bf-a310-45862bd6fc5f
Schneiderbauer, Lukas
868368ac-aad0-4561-9d8b-a01020777f2d
Sybesma, Watse
2dab8872-b422-4452-bf91-6cd008c398ab
Thorlacius, Larus
0f6d184d-5a34-4f6d-838f-f6a8105cd668
Gautason, Fridrik Freyr, Schneiderbauer, Lukas, Sybesma, Watse and Thorlacius, Larus
(2020)
Page curve for an evaporating black hole.
JHEP, 2020 (91), [91].
(doi:10.1007/JHEP05(2020)091).
Abstract
A Page curve for an evaporating black hole in asymptotically flat spacetime is computed by adapting the Quantum Ryu-Takayanagi (QRT) proposal to an analytically solvable semi-classical two-dimensional dilaton gravity theory. The Page time is found to be one third of the black hole lifetime, at leading order in semi-classical corrections. A Page curve is also obtained for a semi-classical eternal black hole, where energy loss due to Hawking evaporation is balanced by an incoming energy flux.
Text
JHEP05(2020)091
- Version of Record
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Accepted/In Press date: 29 April 2020
Published date: 20 May 2020
Identifiers
Local EPrints ID: 497167
URI: http://eprints.soton.ac.uk/id/eprint/497167
ISSN: 1126-6708
PURE UUID: 9192d764-902f-435f-8902-bb6fc6be79ec
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Date deposited: 15 Jan 2025 17:40
Last modified: 22 Aug 2025 02:43
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Contributors
Author:
Fridrik Freyr Gautason
Author:
Lukas Schneiderbauer
Author:
Watse Sybesma
Author:
Larus Thorlacius
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