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dc.contributor.authorBorsten, Leron
dc.contributor.authorJonsson, David Simon Henrik
dc.contributor.authorKim, Hyungrok
dc.date.accessioned2024-08-16T12:30:01Z
dc.date.available2024-08-16T12:30:01Z
dc.date.issued2024-08-08
dc.identifier.citationBorsten , L , Jonsson , D S H & Kim , H 2024 , ' Out-of-time-order asymptotic observables are quasi-isomorphic to time-ordered amplitudes ' , Journal of High Energy Physics (JHEP) . https://doi.org/10.1007/JHEP08(2024)074
dc.identifier.issn1126-6708
dc.identifier.otherArXiv: http://arxiv.org/abs/2405.11110v1
dc.identifier.otherORCID: /0000-0001-9008-7725/work/165661860
dc.identifier.urihttp://hdl.handle.net/2299/28101
dc.description© The Authors. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0). https://creativecommons.org/licenses/by/4.0/
dc.description.abstractAsymptotic observables in quantum feld theory beyond the familiar S-matrixhave recently attracted much interest, for instance in the context of gravity waveforms. Suchobservables can be understood in terms of Schwinger-Keldysh-type ‘amplitudes’ computedby a set of modifed Feynman rules involving cut internal legs and external legs labelledby time-folds.In parallel, a homotopy-algebraic understanding of perturbative quantum feld theoryhas emerged in recent years. In particular, passing through homotopy transfer, the S-matrixof a perturbative quantum feld theory can be understood as the minimal model of anassociated (quantum) L∞-algebra.Here we bring these two developments together. In particular, we show that SchwingerKeldysh amplitudes are naturally encoded in an L∞-algebra, similar to ordinary scatteringamplitudes. As before, they are computed via homotopy transfer, but using deformationretract data that are not canonical (in contrast to the conventional S-matrix). We furthershow that the L∞-algebras encoding Schwinger-Keldysh amplitudes and ordinary amplitudesare quasi-isomorphic (meaning, in a suitable sense, equivalent). This entails a set of recursionrelations that enable one to compute Schwinger-Keldysh amplitudes in terms of ordinaryamplitudes or vice versa.en
dc.format.extent28
dc.format.extent519010
dc.language.isoeng
dc.relation.ispartofJournal of High Energy Physics (JHEP)
dc.subjecthep-th
dc.subjectmath-ph
dc.subjectmath.MP
dc.subject81T18 (Primary) 17B55, 18G50 (Secondary)
dc.titleOut-of-time-order asymptotic observables are quasi-isomorphic to time-ordered amplitudesen
dc.contributor.institutionMathematics and Theoretical Physics
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1007/JHEP08(2024)074
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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