Compact stars (CS) are stellar remnants of massive stars. Inside CSs the density is so high
that matter is in subatomic form composed of nucleons. With an increase of density of matter …

We calculate the baryon-meson coupling constants for the spin-1/2 baryonic octet and spin-
3/2 decuplet in a unified approach relying on symmetry arguments such as the fact that the …

A recent assessment of the central compact object in the supernova remnant HESS J 1731-
347 [Nat. Astron. 6, 1444 (2022) 2397-3366 10.1038/s41550-022-01800-1] reveals its …

Using a quantum hadrodynamics (QHD) and MIT-based models, we construct hybrid stars
within the Maxwell criteria of hadron-quark phase transition. We are able to produce a hybrid …

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 …

Magnetic fields are ubiquitous across different physical systems of current interest; from the
early Universe, compact astrophysical objects and heavy-ion collisions to condensed matter …

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 …

Strong magnetic fields can modify the microscopic composition of matter with consequences
on stellar macroscopic properties. Within this context, we study, for the first time, the …

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 …