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    Large-scale calculations of β-decay rates and implications for r-process nucleosynthesis

    A. Ravlić1,2,*, Y. Saito1,3,4,†, and W. Nazarewicz1,5,‡

    • *Contact author: ravlic@frib.msu.edu
    • †Contact author: saitoy@frib.msu.edu
    • ‡Contact author: witek@frib.msu.edu

    Phys. Rev. C 113, 045802 – Published 2 April, 2026

    DOI: https://doi.org/10.1103/pm1t-9qlb

    Abstract

    Nuclear β decay is a key element of the astrophysical rapid neutron capture process (r process). In this work, we present state-of-the-art global β-decay calculations based on the quantified relativistic nuclear energy density functional theory and the deformed proton-neutron quasiparticle random-phase approximation. Our analysis considers contributions from allowed and first-forbidden transitions. We used two point-coupling functionals with carefully calibrated time-odd terms and isoscalar pairing strength. The new calculations display consistent results for both employed functionals, especially near the neutron drip line, suggesting slower β decays past the N=126 neutron shell closure than in commonly used β-decay models. The new rates, along with the existing rates based on the recent nonrelativistic global calculations, are found to slow down the synthesis of heavy elements in the r process and significantly reduce the contribution of neutron-induced fission.

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