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dc.contributor.authorKurkela, Aleksi
dc.contributor.authorMazeliauskas, Aleksas
dc.contributor.authorPaquet, Jean-Francois
dc.contributor.authorSchlichting, Sören
dc.contributor.authorTeaney, Derek
dc.date.accessioned2021-05-10T07:24:27Z
dc.date.available2021-05-10T07:24:27Z
dc.date.created2019-07-25T12:51:03Z
dc.date.issued2019-03
dc.identifier.citationKurkela, A., Mazeliauskas, J.F.P. et al. (2019) Matching the Nonequilibrium Initial Stage of Heavy Ion Collisions to Hydrodynamics with QCD Kinetic Theory Physical Review Letters, 122 (12)en_US
dc.identifier.issn0031-9007
dc.identifier.urihttps://hdl.handle.net/11250/2754481
dc.description.abstractHigh-energy nuclear collisions produce a nonequilibrium plasma of quarks and gluons which thermalizes and exhibits hydrodynamic flow. There are currently no practical frameworks to connect the early particle production in classical field simulations to the subsequent hydrodynamic evolution. We build such a framework using nonequilibrium Green’s functions, calculated in QCD kinetic theory, to propagate the initial energy-momentum tensor to the hydrodynamic phase. We demonstrate that this approach can be easily incorporated into existing hydrodynamic simulations, leading to stronger constraints on the energy density at early times and the transport properties of the QCD medium. Based on (conformal) scaling properties of the Green’s functions, we further obtain pragmatic bounds for the applicability of hydrodynamics in nuclear 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.subjectfysikken_US
dc.titleMatching the Nonequilibrium Initial Stage of Heavy Ion Collisions to Hydrodynamics with QCD Kinetic Theoryen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.subject.nsiVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430en_US
dc.source.volume122en_US
dc.source.journalPhysical Review Lettersen_US
dc.source.issue12en_US
dc.identifier.doi10.1103/PhysRevLett.122.122302
dc.identifier.cristin1712697
dc.source.articlenumber122302en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2


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