We review the current status of the research on effective nonlocal NJL-like chiral quark
models with separable interactions, focusing on the application of this approach to the …

A viable model for the dense matter equation of state above the nuclear saturation density
includes a hadron-to-quark phase transition at densities relevant to compact objects. In this …

Three parametrizations DOPS1, DOPS2, and DOPS3 (named after the Department of
Physics Shimla) of the relativistic mean field model have been proposed with the inclusion of …

We study the influence of strong magnetic fields in hybrid stars, composed by hadrons and a
pure quark matter core, and analyse their structure and stability as well as some possible …

Neutron stars are the densest objects in the Universe, with M∼ 1.4 M⊙ and R∼ 12 km, and
the equation of state associated to their internal composition is still unknown. The extreme …

We propose a three-flavor version of the Polyakov-Nambu-Jona-Lasino (PNJL) model at
zero temperature regime, by implementing a traced Polyakov loop (Φ) dependence in the …

We probe the outcomes of the baryon-quark phase transition in the hybrid neutron star
(HNS) structure with the help of the Gibbs and Maxwell constructions, adopting a …

We study the hadron–quark hybrid equation of state (EOS) of compact-star matter. The
Nambu–Jona-Lasinio (NJL) local SU (3) model with vector-type interaction is used to …

We perform an improvement in a thermodynamical consistent model with density-dependent
quark masses (mu, d, s′) by introducing effects of quark confinement/deconfinement phase …

Quasinormal modes of neutron stars are an exciting prospect for analyzing the internal
composition of neutron stars and studying matter at high densities. In this work, we focus on …