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 …

Background: The central depression of nucleonic density, ie, a reduction of density in the
nuclear interior, has been attributed to many factors. For instance, bubble structures in …

It is important to study the different decay modes of superheavy nuclei such as spontaneous
fission, ternary fission and cluster decay. We studied the spontaneous fission, ternary fission …

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 …

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 …

We have studied the fusion cross section, evaporation residue cross secion, compound
nucleus formation probability (P_CN PCN) and survival probability (P_sur P sur) of different …

We employ the relativistic mean-field plus BCS (RMF+ BCS) approach to study the behavior
of sd-shell by investigating in detail the single particle energies, and proton and neutron …

The decay properties of the isotopes of Z= 125 within the range 303≤ A≤ 339 are
investigated. The calculation of proton separation energies reveals that isotopes 125 303 …

The ground state properties of Z= 125 and 126 nuclei are investigated, taking the isotopic
series from the proton to neutron drip-lines. This analysis uses the relativistic mean-field …

We have employed the RMF+ BCS (relativistic mean-field plus BCS) approach to study the
behaviour of the pf shell with the help of the ground state properties of even-even nuclei. Our …