Impact of the first-forbidden decay on the production of r-process peak
Nobuya Nishimura🇬🇧 · Zsolt Podolyák🇬🇧 · Dong-Liang Fang🇨🇳 · Toshio Suzuki🇯🇵
We investigated the effects of first-forbidden transitions in decays on the production of the r-process peak. The theoretical calculated -decay rates with -delayed neutron emission were examined using several astrophysical conditions. As the first-borbidden decay is dominant in neutron-rich nuclei, their inclusion shortens -decay lifetimes and shifts the abundance peak towards higher masses. Additionally, the inclusion of the -delayed neutron emission results in a wider abundance peak, and smoothens the mass distribution by removing the odd-even mass staggering. The effects are commonly seen in the results of all adopted astrophysical models. Nevertheless there are quantitative differences, indicating that remaining uncertainty in the determination of half-lives for nuclei is still significant in order to determine the production of the r-process peak.