Astrophysical simulations require knowledge of a wide array of reaction rates. For a number
of reasons, many of these reaction rates cannot be measured directly and instead are …

The r-process progresses in the neutron-rich region of the nuclear chart and can possibly
encounter nuclei having exotic structures with deformations, halos, and bubbles …

Background: Lying at the lower edge of the “island of inversion,” neutron-rich fluorine
isotopes (F 29–31) provide a curious case to study the configuration mixing in this part of the …

Enhancement, due to constructive interference through the many possible reaction
channels, occurs in two-neutron transfer reactions from a bound system $ A $ to a weakly …

Experimental data on Coulomb breakup and neutron removal indicate that Ne 31 is one of
the heaviest halo nuclei discovered so far. The possible ground state of Ne 31 is either 3/2 …

This study examines the radiative capture of a neutron by 10 Be using the Coulomb
dissociation approach within the FRDWBA theory. We analyze the elastic Coulomb breakup …

Background: Small changes in reaction rates due to neutron capture, α capture, and β decay
by exotic nuclei in the low and medium mass region can direct the r-process path in different …

We give a brief overview of the current status of important nuclear physics inputs, like
reaction rates, in hydrostatic and explosive nucleosynthesis. Recently, it has been proposed …

We calculate the 11 B (n, γ) 12 B reaction rate which is an important constituent in
nucleosynthesis networks and is contributed by resonant as well as non-resonant capture …

We calculate the $^{11} $ B $(n,\gamma)^{12} $ B reaction rate, an important constituent in
nucleosynthesis networks, contributed by resonant as well as non-resonant capture. For the …