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Page curve for an evaporating black hole
by
Sybesma, Watse
, Thorlacius, Lárus
, Gautason, Friðrik Freyr
, Schneiderbauer, Lukas
in
2D Gravity
/ AdS-CFT Correspondence
/ Black Holes
/ Classical and Quantum Gravitation
/ Dilatons
/ Elementary Particles
/ Energy dissipation
/ Entropy
/ Evaporation
/ Gravity
/ High energy physics
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Radiation
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ Spacetime
/ String Theory
/ Two dimensional analysis
2020
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Page curve for an evaporating black hole
by
Sybesma, Watse
, Thorlacius, Lárus
, Gautason, Friðrik Freyr
, Schneiderbauer, Lukas
in
2D Gravity
/ AdS-CFT Correspondence
/ Black Holes
/ Classical and Quantum Gravitation
/ Dilatons
/ Elementary Particles
/ Energy dissipation
/ Entropy
/ Evaporation
/ Gravity
/ High energy physics
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Radiation
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ Spacetime
/ String Theory
/ Two dimensional analysis
2020
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Page curve for an evaporating black hole
by
Sybesma, Watse
, Thorlacius, Lárus
, Gautason, Friðrik Freyr
, Schneiderbauer, Lukas
in
2D Gravity
/ AdS-CFT Correspondence
/ Black Holes
/ Classical and Quantum Gravitation
/ Dilatons
/ Elementary Particles
/ Energy dissipation
/ Entropy
/ Evaporation
/ Gravity
/ High energy physics
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Radiation
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ Spacetime
/ String Theory
/ Two dimensional analysis
2020
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Journal Article
Page curve for an evaporating black hole
2020
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Overview
A
bstract
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.
Publisher
Springer Berlin Heidelberg,Springer Nature B.V,SpringerOpen
Subject
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