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dc.contributor.authorKurkela, Aleksi
dc.contributor.authorvan der Schee, Wilke
dc.contributor.authorWiedemann, Urs Achim
dc.contributor.authorWu, Bin
dc.date.accessioned2023-01-06T12:14:16Z
dc.date.available2023-01-06T12:14:16Z
dc.date.created2020-11-12T10:40:45Z
dc.date.issued2020
dc.identifier.citationKurkela, A., van der Schee, W., Wiedemann, U. A., & Wu, B. (2020). Early-and late-time behavior of attractors in heavy-ion collisions. Physical Review Letters, 124(10), 102301.en_US
dc.identifier.issn0031-9007
dc.identifier.urihttps://hdl.handle.net/11250/3041573
dc.description.abstractWhether, how, and to what extent solutions of Bjorken-expanding systems become insensitive to aspects of their initial conditions is of importance for heavy-ion collisions. Here we study 1+1D and phenomenologically relevant boost-invariant 3+1D systems in which initial conditions approach a universal attractor. In Israel-Stewart theory (IS) and kinetic theory where the universal attractor extends to arbitrarily early times, we show that all initial conditions approach the attractor at early times by a power law while their approach is exponential at late times. In these theories, the physical mechanisms of hydrodynamization operational at late times do not drive the approach to the attractor at early times, and the early-time attractor is reached prior to hydrodynamization. In marked contrast, the attractor in strongly coupled systems is realized concurrent with hydrodynamization. This qualitative difference may offer a basis for discriminating weakly and strongly coupled scenarios of heavy-ion collisions.en_US
dc.language.isoengen_US
dc.publisherAmerican Physical Societyen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleEarly- and Late-Time Behavior of Attractors in Heavy-Ion Collisionsen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.rights.holderthe authorsen_US
dc.subject.nsiVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430en_US
dc.source.volume124en_US
dc.source.journalPhysical Review Lettersen_US
dc.source.issue10en_US
dc.identifier.doi10.1103/PhysRevLett.124.102301
dc.identifier.cristin1847307
dc.source.articlenumber102301en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2


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