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dc.contributor.authorGlatthard, J
dc.date.accessioned2024-04-12T13:46:42Z
dc.date.issued2024-04-11
dc.date.updated2024-04-12T13:21:05Z
dc.description.abstractThe entanglement entropy of a black hole and that of its Hawking radiation are expected to follow the socalled Page curve: After an increase in line with Hawking’s calculation, it is expected to decrease back to zero once the black hole has fully evaporated, as demanded by unitarity. Recently, a simple system-plusbath model has been proposed which shows a similar behavior. Here, we make a general argument as to why such a Page-curve-like entanglement dynamics should be expected to hold generally for system-plusbath models at small coupling and low temperatures, when the system is initialized in a pure state far from equilibrium. The interaction with the bath will then generate entanglement entropy, but it eventually has to decrease to the value prescribed by the corresponding mean-force Gibbs state. Under those conditions, it is close to the system ground state. We illustrate this on two paradigmatic open-quantum-system models, the exactly solvable harmonic quantum Brownian motion and the spin-boson model, which we study numerically. In the first example we find that the intermediate entropy of an initially localized impurity is higher for more localized initial states. In the second example, for an impurity initialized in the excited state, the Page time—when the entropy reaches its maximum—occurs when the excitation has half decayed.en_GB
dc.description.sponsorshipUniversity of Exeteren_GB
dc.identifier.citationVol. 109, No. 8, article L081901en_GB
dc.identifier.doihttps://doi.org/10.1103/physrevd.109.l081901
dc.identifier.urihttp://hdl.handle.net/10871/135741
dc.language.isoenen_GB
dc.publisherAmerican Physical Societyen_GB
dc.rights© The Author(s). Open Access. Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.en_GB
dc.subjectExact solutions for many-body systemsen_GB
dc.subjectInformation theoryen_GB
dc.subjectNumerical techniquesen_GB
dc.titlePage-curve-like entanglement dynamics in open quantum systemsen_GB
dc.typeArticleen_GB
dc.date.available2024-04-12T13:46:42Z
dc.identifier.issn2470-0010
exeter.article-numberL081901
dc.descriptionThis is the final version. Available from the American Physical Society via the DOI in this record. en_GB
dc.descriptionThe data that support the findings of this study are available from the author upon reasonable request.en_GB
dc.identifier.eissn2470-0029
dc.identifier.journalPhysical Review D (particles, fields, gravitation, and cosmology)en_GB
dc.relation.ispartofPhysical Review D, 109(8)
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_GB
dcterms.dateAccepted2024-03-11
rioxxterms.versionVoRen_GB
rioxxterms.licenseref.startdate2024-04-11
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2024-04-12T13:40:20Z
refterms.versionFCDVoR
refterms.dateFOA2024-04-12T13:46:49Z
refterms.panelBen_GB
refterms.dateFirstOnline2024-04-11


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© The Author(s). Open Access. Published by the American Physical Society under the terms of
the Creative Commons Attribution 4.0 International license.
Further distribution of this work must maintain attribution to
the author(s) and the published article’s title, journal citation,
and DOI.
Except where otherwise noted, this item's licence is described as © The Author(s). Open Access. Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.