β-Delayed Neutron and Fission Calculations with Relativistic QRPA and Statistical Model
Abstract
A role of β-delayed neutron emission and fission in r-process nucleosynthesis attracts a high interest. Although the number of study on them covering r-process nuclei is increasing recently, uncertainties of β-delayed neutron and fission are still large for r-process simulations. Our purpose is to make a new database on β-delayed neutron emission and fission rates. To this end, the data that are not investigated experimentally have to be predicted. Microscopic theoretical approaches based on a nuclear energy density functional and statistical models are one of the competent tools for the prediction. To obtain β strength function, p-n relativistic QRPA is adopted. Particle evaporations and fission from nuclear highly excited states are estimated by the Hauser-Feshbach statistical model. β-delayed neutron branching ratios (Pn) are calculated and compared with experimental data. β-delayed fission branching ratio (Pf) are also assessed by using four different fission barrier data. Calculated Pn values are in a good agreement with experimental data. It is found that energy withdrawal by β-delayed neutron emission sensitively varies Pn values for nuclei near the neutron drip line. Pf are sensitively dependent on fission barrier data. Newly calculated data on β-delayed neutron emission and fission are summarized as a table in supplement material. They are provided for studies of r-process as well as other fields such as nuclear engineering.
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