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dc.contributor.authorGorda, Tyler
dc.contributor.authorKurkela, Eero Aleksi
dc.contributor.authorPaatelainen, Risto
dc.contributor.authorSäppi, Saga
dc.contributor.authorVuorinen, Aleksi
dc.date.accessioned2023-03-15T09:59:30Z
dc.date.available2023-03-15T09:59:30Z
dc.date.created2021-12-06T18:31:44Z
dc.date.issued2021
dc.identifier.citationGorda, T., Kurkela, A., Paatelainen, R., Säppi, S., & Vuorinen, A. (2021). Cold quark matter at N 3 LO: Soft contributions. Physical Review D, 104(7), 074015.en_US
dc.identifier.issn2470-0010
dc.identifier.urihttps://hdl.handle.net/11250/3058314
dc.description.abstractHigh-order perturbative calculations for thermodynamic quantities in QCD are complicated by the physics of dynamical screening that affects the soft, long-wavelength modes of the system. Here, we provide details for the evaluation of this soft contribution to the next-to-next-to-next-to-leading order ( N 3 LO ) pressure of high-density, zero-temperature quark matter (QM), complementing our accompanying Letter [T. Gorda et al., Phys. Rev. Lett. 127, 162003 (2021)]. Our calculation requires the determination of the pressure of the hard-thermal-loop effective theory to full two-loop order at zero temperature, which we go through in considerable detail. In addition to this, we comprehensively discuss the structure of the weak-coupling expansion of the QM pressure, and lay out a roadmap towards the evaluation of the contributions missing from a full N 3 LO result for this quantity.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.titleCold quark matter at N3LO: Soft contributionsen_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.pagenumber1-43en_US
dc.source.volume104en_US
dc.source.journalPhysical Review Den_US
dc.source.issue7en_US
dc.identifier.doi10.1103/PhysRevD.104.074015
dc.identifier.cristin1965274
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1


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