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 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 …

In this theoretical study, we establish a correlation between the neutron skin thickness and
the nuclear symmetry energy for the even-even isotopes of Fe, Ni, Zn, Ge, Se, and Kr within …

We have studied the effect of density and the nucleus-nucleus interaction potential on the
fusion reaction cross section for the synthesis of heavy and superheavy nuclei within the …

In this theoretical study, we establish an interrelationship between the nucleon-nucleon
potential and the nuclear fusion reaction cross sections at low energies. The axially …

The effect of δ-and ω-ρ-meson cross couplings on asymmetry nuclear systems are analyzed
in the framework of an effective field theory motivated relativistic mean field formalism. The …

The secondary component of the GW190814 event left us with a question,“whether it is a
supermassive neutron star or lightest black-hole?” Recently, Fattoyev et al. obtained an …

In this theoretical study, we establish a correlation between the neutron skin thickness and
the nuclear symmetry energy for the even–even isotones for magic neutron N= 20, 40, 82 …

Density-dependent nuclear symmetry energy is directly related to isospin asymmetry for
finite and infinite nuclear systems. It is critical to determine the coefficients of symmetry …