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Holographic complexity: stretching the horizon of an evaporating black hole

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dc.contributor Háskóli Íslands
dc.contributor University of Iceland
dc.contributor.author Schneiderbauer, Lukas
dc.contributor.author Sybesma, Watse
dc.contributor.author Thorlacius, Larus
dc.date.accessioned 2021-01-26T12:51:46Z
dc.date.available 2021-01-26T12:51:46Z
dc.date.issued 2020-03
dc.identifier.citation Schneiderbauer, L., Sybesma, W. & Thorlacius, L. Holographic complexity: stretching the horizon of an evaporating black hole. J. High Energ. Phys. 2020, 69 (2020). https://doi.org/10.1007/JHEP03(2020)069
dc.identifier.issn 1029-8479
dc.identifier.uri https://hdl.handle.net/20.500.11815/2412
dc.description Publisher's version (útgefin grein)
dc.description.abstract We obtain the holographic complexity of an evaporating black hole in the semi-classical RST model of two-dimensional dilaton gravity, using a volume prescription that takes into account the higher-dimensional origin of the model. For classical black holes, we recover the expected late time behaviour of the complexity, but new features arise at the semi-classical level. By considering the volume inside the stretched horizon of the evolving black hole, we obtain sensible results for the rate of growth of the complexity, with an early onset of order the black hole scrambling time followed by an extended period where the rate of growth tracks the shrinking area of the stretched horizon as the black hole evaporates.
dc.format.extent 69
dc.language.iso en
dc.publisher Springer Science and Business Media LLC
dc.relation.ispartofseries Journal of High Energy Physics;2020(3)
dc.rights info:eu-repo/semantics/openAccess
dc.subject 2D Gravity
dc.subject Black Holes
dc.subject Classical Theories of Gravity
dc.subject Svarthol (stjörnufræði)
dc.subject Þyngdarafl
dc.title Holographic complexity: stretching the horizon of an evaporating black hole
dc.type info:eu-repo/semantics/article
dcterms.license This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited
dc.description.version Peer Reviewed
dc.identifier.journal Journal of High Energy Physics
dc.identifier.doi 10.1007/JHEP03(2020)069
dc.relation.url http://link.springer.com/content/pdf/10.1007/JHEP03(2020)069.pdf
dc.contributor.department Raunvísindastofnun (HÍ)
dc.contributor.department Science Institute (UI)
dc.contributor.school Verkfræði- og náttúruvísindasvið (HÍ)
dc.contributor.school School of Engineering and Natural Sciences (UI)

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