Even though the crystallized nature of the neutron star crust plays a pivotal role in describing
various fascinating astrophysical observations, its microscopic structure is not fully …

In this paper, we employ the density dependent relativistic hadron (DDRH) field theoretical
model in a Bayesian analysis to investigate the equation of state (EOS) of dense matter …

We use the effective relativistic mean-field (E-RMF) model to study the crustal properties of
the neutron star. The unified equations of state (EoS) are constructed using recently …

We study the properties of pasta structures and their influence on the neutron star
observables employing the effective relativistic mean-field (E-RMF) model. The …

In this study, my main goal is to examine the nuclear matter properties across a wide range
of conditions, such as temperature, density, asymmetry, pressure, and magnetic field …

This work aims to study the various thermal characteristics of nuclei in view of the saturation
and critical behavior of infinite nuclear matter. The free energy of a nucleus is parametrized …

The first-order phase transition in nuclear matter plays a crucial role in the heavy-ion
collision experiments. This phase transition is characterized by a critical point (CP) in the …