Background: The microscopic composition and properties of infinite hadronic matter at a
wide range of densities and temperatures have been subjects of intense investigation for …

We carry out the study of finite nuclei, infinite nuclear matter, and neutron star properties with
the newly developed relativistic force, the Institute of Physics Bhubaneswar-I (IOPB-I). Using …

This review presents the status of the field of two-nucleon and multi-nucleon transfer
reactions induced by heavy ions. The role of the pairing interaction in nuclei as a finite …

The fastest and heaviest pulsar, PSR J0952-0607, with a mass of M= 2.35±0.17 M⊙, has
recently been discovered in the disk of the Milky Way Galaxy. In response to this discovery, a …

The density dependence of the symmetry energy, instrumental in understanding the
behavior of the asymmetric nuclear matter, is investigated within the extended relativistic …

Abstract The Hartree-Fock-Bogoliubov (HFB) equations in coordinate representation are
solved exactly, ie, with correct asymptotic boundary conditions for the continuous spectrum …

A new parameter set is generated for finite and infinite nuclear system within the effective
field theory motivated relativistic mean field (ERMF) formalism. The isovector part of the …

The correlation between the charge radii differences in mirror nuclei pairs and the neutron
skin thickness has been studied with the so-called finite range simple effective interaction …

A Shell-model-like approach suggested to treat the pairing correlations in relativistic mean
field theory is introduced, in which the occupancies thus obtained have been iterated back …

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 …