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.
CITATION STYLE
Ranea-Sandoval, I. F., Orsaria, M. G., Malfatti, G., Curin, D., Mariani, M., Contrera, G. A., & Guilera, O. M. (2019). Effects of hadron-quark phase transitions in hybrid stars within the NJL model. Symmetry, 11(3). https://doi.org/10.3390/sym11030425
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