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 …

We present an analysis of hot and dilute isospin-asymmetric nuclear matter employing the
temperature-dependent effective-relativistic mean-field theory (E-RMF). We consider nuclear …

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 …

The critical parameters of the liquid-gas phase transition of symmetric nuclear matter are
computed using the Brueckner-Hartree-Fock method at finite temperature by employing …

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 …