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Paper detail

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.

preprint2020arXivOpen access
Friðrik Freyr GautasonLukas SchneiderbauerWatse SybesmaLárus Thorlacius
hep-th
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Friðrik Freyr GautasonLukas SchneiderbauerWatse SybesmaLárus Thorlacius

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