dc.creatorRanea Sandoval, Ignacio Francisco
dc.creatorOrsaria, Milva Gabriela
dc.creatorMalfatti, Germán
dc.creatorCurin, Daniela
dc.creatorMariani, Mauro
dc.creatorContrera, Gustavo Aníbal
dc.creatorGuilera, Octavio Miguel
dc.date2019-03
dc.date2019-09-12T17:29:40Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/81108
dc.identifierissn:2073-8994
dc.descriptionWe 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.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas (FCAG)
dc.descriptionInstituto de Física La Plata (IFLP)
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsCreative Commons Attribution 4.0 International (CC BY 4.0)
dc.subjectCiencias Astronómicas
dc.subjectNJL model
dc.subjectquark matter
dc.subjecthybrid stars
dc.subjectstellar oscillations
dc.titleEffects of Hadron-Quark Phase Transitions in Hybrid Stars within the NJL Model
dc.typeArticulo
dc.typeArticulo


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