Vis enkel innførsel

dc.contributor.authorFolkestad, Åsmund
dc.contributor.authorAndersen, Jens Oluf
dc.date.accessioned2019-04-23T08:37:13Z
dc.date.available2019-04-23T08:37:13Z
dc.date.created2019-03-11T15:10:52Z
dc.date.issued2019
dc.identifier.issn0556-2821
dc.identifier.urihttp://hdl.handle.net/11250/2594986
dc.description.abstractWe study the thermodynamics and phase diagrams of two-flavor quantum chromodynamics using the Polyakov-loop extended quark-meson (PQM) model and the Pisarski-Skokov chiral matrix (χM) model [1]. At temperatures up to T≈2Tc and baryon chemical potentials up to μB=400 MeV, both models show reasonable agreement with the pressure, energy density, and interaction measure as calculated on the lattice. The Polyakov loop is found to rise significantly faster with temperature in models than on the lattice. In the low-temperature and high baryon density regime, the two models predict different states of matter; The PQM model predicts a confined and chirally restored phase, while the χM model predicts a deconfined and chirally restored phase. At finite isospin density and zero baryon density, the onset of pion condensation at T=0 is at μI=12mπ, and the transition is second order at all temperatures. The transition temperature for pion condensation coincides with that of the chiral transition for values of the isospin chemical potential larger than approximately 110 MeV. In the χM model, they also coincide with the transition temperature for deconfinement. The results are in good overall agreement with recent lattice simulations of the μI–T phase diagram.nb_NO
dc.language.isoengnb_NO
dc.publisherAmerican Physical Societynb_NO
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleThermodynamics and phase diagrams of Polyakov-loop extended chiral modelsnb_NO
dc.typeJournal articlenb_NO
dc.typePeer reviewednb_NO
dc.description.versionpublishedVersionnb_NO
dc.source.journalPhysical Review D. Particles and fieldsnb_NO
dc.identifier.doihttps://doi.org/10.1103/PhysRevD.99.054006
dc.identifier.cristin1683818
dc.description.localcodePublished 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. Funded by SCOAP3.nb_NO
cristin.unitcode194,66,20,0
cristin.unitnameInstitutt for fysikk
cristin.ispublishedtrue
cristin.fulltextpostprint
cristin.qualitycode0


Tilhørende fil(er)

Thumbnail

Denne innførselen finnes i følgende samling(er)

Vis enkel innførsel

Navngivelse 4.0 Internasjonal
Med mindre annet er angitt, så er denne innførselen lisensiert som Navngivelse 4.0 Internasjonal