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 …

We study the dark matter (DM) effects on the nuclear matter (NM) parameters characterizing
the equation of states of super dense neutron-rich nucleonic matter. The observables of the …

The effects of dark matter (DM) on the curvatures of the neutron star (NS) are examined by
using the stiff and soft relativistic mean-field equation of states. The curvatures of the NSs …

Background: Isotopes of Z= 107–118 have been synthesized using cold fusion at GSI,
Darmstadt, and hot fusion reactions at JINR, Dubna. Recently theoretical models have …

Background: Heavy-ion fusion reactions play a crucial role in various aspects of nuclear
physics and astrophysics. The nuclear interaction potential and hence the fusion barrier …

The ground-state properties such as binding energy, root-mean-square radius, pairing
energy, nucleons density distribution, symmetry energy, and single-particle energies are …

A simple form of nonlinear self-coupling of the scalar meson field is introduced and suggests
a new nucleon-nucleon (NN) potential in relativistic mean field theory (RMFT) analogous to …

The aspect of structural evolution and the correlation of the properties of the ground state
with the effective symmetry energy and its coefficients is examined for neutron-rich even …

Starting from light to superheavy nuclei, we have calculated the effective surface properties
such as the symmetry energy, neutron pressure, and symmetry energy curvature using the …

We revisit the studies of the isotopic shift in the charge radii of even–even isotopes of Sn and
Pb nuclei at N= 82, and 126, respectively, within the relativistic mean-field (RMF) and …