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dc.contributor.authorAndersen, Jens Oluf
dc.contributor.authorZhou, Hua
dc.contributor.authorYu, Qing
dc.date.accessioned2024-02-28T07:41:00Z
dc.date.available2024-02-28T07:41:00Z
dc.date.created2024-02-22T17:06:45Z
dc.date.issued2024
dc.identifier.issn0556-2821
dc.identifier.urihttps://hdl.handle.net/11250/3120201
dc.description.abstractWe consider pion condensation in QCD at finite isospin density μI and zero temperature using two-flavor chiral perturbation theory (χPT). The pressure is calculated to next-to-leading order (NLO) in the low-energy expansion. In the nonrelativistic limit, we recover the classic result by Lee, Huang, and Yang for the energy density of a dilute Bose gas with an s-wave scattering length that includes loop corrections from χPT. In the chiral limit, higher-order calculations are tractable. We calculate the pressure to next-to-next-to-leading order (NNLO) in the low-energy expansion, which is an expansion in powers of μ2I/(4π)2f2, where f is the (bare) pion decay constant. The spontaneous breakdown of the global internal symmetry U(1)I3 gives rise to a massless Goldstone boson or phonon. We discuss the properties of the low-energy effective theory describing this mode. Finally, we compare our results for the pressure and the speed of sound with recent lattice simulations with 2+1 flavors. The agreement is very good for isospin chemical potentials up to 180–200 MeV, depending on the physical 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.titlePion condensation in QCD at finite isospin density, the dilute Bose gas, and speedy Goldstone bosonsen_US
dc.title.alternativePion condensation in QCD at finite isospin density, the dilute Bose gas, and speedy Goldstone bosonsen_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.source.journalPhysical Review D. Particles and fieldsen_US
dc.identifier.doihttps://doi.org/10.1103/PhysRevD.109.034022
dc.identifier.cristin2248945
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode0


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