Alpha decay of thermally excited nuclei
arXiv:2212.03983 · doi:10.1088/1361-6471/aca03c
Abstract
One of the prominent decay modes of heavy nuclei which are produced in astrophysical environments at temperatures of the order of K is the (He) decay. Thermally enhanced decay rates are evaluated within the standard scheme of a tunneling decay where the particle tunnels through the potential barrier formed by its interaction with the daughter nucleus. Following the observation that there exist several excited levels with the possibility of an decay when the daughter nucleus is at a shell closure, we focus in particular on decays producing daughter nuclei with the neutron number, N = 126. Within a statistical approach we find that the half-lives, , for temperatures ranging from = 0 to 2.4 GK can decrease by 1 - 2 orders of magnitude with the exception of the decay of Po which decays to the doubly magic daughter Pb, where decreases by 5 orders of magnitude. The effect of these thermally enhanced decays on the -process nucleosynthesis can be significant in view of the mass build up at the waiting point nuclei with closed neutron shells.
18 pages, 1 figure
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