Uncertainties in radiative neutron-capture rates relevant to the \(A\sim 80\) \(r\)-process peak

Abstract

The rapid neutron-capture process (\(r\)-process) has for the first time been confirmed to take place in a neutron-star merger event. A detailed understanding of the rapid neutron-capture process is one of the holy grails in nuclear astrophysics. In this work we investigate one aspect of the \(r\)-process modelling: uncertainties in radiative neutron-capture cross sections and astrophysical reaction rates for isotopes of the elements Fe, Co, Ni, Cu, Zn, Ga, Ge, As, and Se. In particular, we study deviations from standard libraries used for astrophysics, and the influence of a very-low \(\gamma\)-energy enhancement in the average, reduced \(\gamma\)-decay probability on the (\(n,\gamma\)) rates. We find that the intrinsic uncertainties are in some cases extremely large, and that the low-energy enhancement, if present in neutron-rich nuclei, may increase the neutron-capture reaction rate significantly.