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dc.date.accessioned 2019-09-12T17:29:40Z
dc.date.available 2019-09-12T17:29:40Z
dc.date.issued 2019-03
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/81108
dc.description.abstract We study local and non-local Polyakov Nambu-Jona-Lasinio models and analyze their respective phase transition diagram. We construct hybrid stars using the zero temperature limit of the local and non-local versions of Nambu-Jona-Lasinio model for quark matter and the modern GM1(L) parametrization of the non-linear relativistic mean field model for hadronic matter. We compare our models with data from PSR J1614-2230 and PSR J0343+0432 and also from GW170817 and its electromagnetic counterpart GRB170817A and AT2017gfo. We study observational signatures of the appearance of a mixed phase as a result of modeling a phase transition that mimics the Gibbs formalism and compare the results with the sharp first-order phase transition obtained using the Maxwell construction. We also study in detail the g-mode associated with discontinuities in the equation of state, and calculate non-radial oscillation modes using relativistic Cowling approximation. en
dc.language en es
dc.subject NJL model es
dc.subject quark matter es
dc.subject hybrid stars es
dc.subject stellar oscillations es
dc.title Effects of Hadron-Quark Phase Transitions in Hybrid Stars within the NJL Model en
dc.type Articulo es
sedici.identifier.other https://doi.org/10.3390/sym11030425 es
sedici.identifier.issn 2073-8994 es
sedici.creator.person Ranea Sandoval, Ignacio Francisco es
sedici.creator.person Orsaria, Milva Gabriela es
sedici.creator.person Malfatti, Germán es
sedici.creator.person Curin, Daniela es
sedici.creator.person Mariani, Mauro es
sedici.creator.person Contrera, Gustavo Aníbal es
sedici.creator.person Guilera, Octavio Miguel es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas (FCAG) es
mods.originInfo.place Instituto de Física La Plata (IFLP) es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Symmetry es
sedici.relation.journalVolumeAndIssue vol. 11, no. 3 es


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Creative Commons Attribution 4.0 International (CC BY 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution 4.0 International (CC BY 4.0)