Please use this identifier to cite or link to this item: https://hdl.handle.net/10316/106064
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dc.contributor.authorPereira, Renan Câmara-
dc.contributor.authorStiele, Rainer-
dc.contributor.authorCosta, Pedro-
dc.date.accessioned2023-03-17T10:23:00Z-
dc.date.available2023-03-17T10:23:00Z-
dc.date.issued2020-
dc.identifier.issn1434-6044-
dc.identifier.issn1434-6052-
dc.identifier.urihttps://hdl.handle.net/10316/106064-
dc.description.abstractThe critical region of the two flavour quarkmeson model with vector interactions is explored using the Functional Renormalization Group, a non-perturbative method that takes into account quantum and thermal fluctuations. Special attention is given to the low temperature and high density region of the phase diagram, which is very important to construct the equation of state of compact stars. As in previous studies, without repulsive vector interaction, an unphysical region of negative entropy density is found near the first order chiral phase transition. We explore the connection between this unphysical region and the chiral critical region, especially the first order line and spinodal lines, using also different values for vector interactions. We find that the unphysical negative entropy density region appears because the s = 0 isentropic line, near the critical region, is displaced from its T = 0 location. For certain values of vector interactions this region is pushed to lower temperatures and high chemical potentials in such way that the negative entropy density region on the phase diagram can even disappear. In the case of finite vector interactions, the location of the critical end point has a non-trivial behaviour in the T −μB plane, which differs from that in mean field calculations.pt
dc.description.sponsorshipThis work was supported by national funds from FCT (Fundação para a Ciência e a Tecnologia, I.P, Portugal) under the IDPASC Ph.D. program (International Doctorate Network in Particle Physics, Astrophysics and Cosmology), with the Grant No. PD/- BD/128234/2016 (R.C.P.), and under the ProjectsNo. UID/FIS/04564/- 2019, No. UID/04564/2020, and No. POCI-01-0145-FEDER-029912 with financial support from POCI “Programa Operacional Competitividade e Internacionalização (COMPETE 2020)”, in its FEDER component, as well as by an INFN Post Doctoral Fellowship (competition INFN notice n. 18372/2016, RS). We wish to thank Constanaça Providência for useful comments. One of the authors (R.C.P.) would like to thankKonstantin Otto for useful email correspondence regarding the numerical approach andMarcos Gouveia for help with the OpenMP interface.We acknowledge the Laboratory for Advanced Computing at the University of Coimbra for providing CPU time with the Navigator cluster. The authors also acknowledge the INFN (Istituto Nazionale di Fisica Nucleare) – Sezione di Torino and the COST Action CA16214 “PHAROS: The multi-messenger physics and astrophysics of neutron stars” for funding a Short Term Scientific Mission (STSM) at the INFN – Sezione di Torino.-
dc.language.isoengpt
dc.publisherSpringer Naturept
dc.rightsopenAccesspt
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/pt
dc.titleFunctional renormalization group study of the critical region of the quark-meson model with vector interactionspt
dc.typearticlept
degois.publication.firstPage712pt
degois.publication.issue8pt
degois.publication.titleEuropean Physical Journal Cpt
dc.peerreviewedyespt
dc.identifier.doi10.1140/epjc/s10052-020-8296-9-
degois.publication.volume80pt
dc.date.embargo2020-01-01*
uc.date.periodoEmbargo0pt
item.grantfulltextopen-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.openairetypearticle-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextCom Texto completo-
crisitem.author.researchunitCFisUC – Center for Physics of the University of Coimbra-
crisitem.author.orcid0000-0003-4809-6542-
Appears in Collections:I&D CFis - Artigos em Revistas Internacionais
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