We report a new equation of state (EoS) of cold and hot hyperonic matter constructed in the
framework of the quark–meson-coupling (QMC-A) model. The QMC-A EoS yields results …

We analyze the role played by a mixed vector-isoscalar/vector-isovector meson interaction
in dense matter present in the interior of neutron stars in the light of new measurements …

A neutron star was first detected as a pulsar in 1967. It is one of the most mysterious
compact objects in the universe, with a radius of the order of 10 km and masses that can …

Using six different parametrizations of the quantum hadrodynamics (one of which is
original), I study how different values of the symmetry energy slope L affect some …

We investigate possible traces of the nuclear symmetry energy slope (L) in the gravitational
wave emission of neutron stars. For fixed stellar mass values, we examine how the slope …

In this work we introduce an extended version of the formalism proposed originally by
Taurines et al. that considers the effects of many-body forces simulated by nonlinear self …

In this work we revisit the quantum hadrodynamics (QHD) formalism to investigate hyperonic
and hybrid stars with hyperon-meson couplings fixed via broken SU (6) group, in favor of a …

We study how the nuclear symmetry energy slope (L) can affect the hadron-quark phase
transition and neutron star properties. We show that the main physical quantities as the …

Abstract In 2023 December, the Fermi Large Area Telescope Catalog announced the
discovery of 33 new millisecond pulsars. Motivated by that, in this work, I study how different …

Motivated by the recent gravitational wave detection by the LIGO–VIRGO observatories, we
study the Love number and dimensionless tidal polarizability of highly magnetized stars. We …