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dc.contributor.authorAdhikari, Prabal
dc.contributor.authorAndersen, Jens Oluf
dc.contributor.authorKneschke, Patrick
dc.date.accessioned2020-01-15T10:16:33Z
dc.date.available2020-01-15T10:16:33Z
dc.date.created2019-10-28T14:01:09Z
dc.date.issued2019
dc.identifier.citationEuropean Physical Journal C. 2019, 79 (10), .nb_NO
dc.identifier.issn1434-6044
dc.identifier.urihttp://hdl.handle.net/11250/2636379
dc.description.abstractIn this paper, we calculate the equation of state of two-flavor finite isospin chiral perturbation theory at next-to-leading order in the pion-condensed phase at zero temperature. We show that the transition from the vacuum phase to a Bose-condensed phase is of second order. While the tree-level result has been known for some time, surprisingly quantum effects have not yet been incorporated into the equation of state. We find that the corrections to the quantities we compute, namely the isospin density, pressure, and equation of state, increase with increasing isospin chemical potential. We compare our results to recent lattice simulations of 2 + 1 flavor QCD with physical quark masses. The agreement with the lattice results is generally good and improves somewhat as we go from leading order to next-to-leading order in χPT.nb_NO
dc.language.isoengnb_NO
dc.publisherSpringernb_NO
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleTwo-flavor chiral perturbation theory at nonzero isospin: Pion condensation at zero temperaturenb_NO
dc.typeJournal articlenb_NO
dc.typePeer reviewednb_NO
dc.description.versionpublishedVersionnb_NO
dc.source.pagenumber13nb_NO
dc.source.volume79nb_NO
dc.source.journalEuropean Physical Journal Cnb_NO
dc.source.issue10nb_NO
dc.identifier.doi10.1140/epjc/s10052-019-7381-4
dc.identifier.cristin1741219
dc.description.localcode© The Author(s) 2019. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.nb_NO
cristin.unitcode194,66,20,0
cristin.unitnameInstitutt for fysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1


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