Unique first-forbidden $\beta$-decay rates for neutron-rich nickel isotopes in stellar environment
Jameel-Un Nabi, Sabin Stoica

TL;DR
This paper calculates the first-forbidden beta-decay rates for neutron-rich nickel isotopes in stellar environments using pn-QRPA, highlighting their importance in astrophysical processes like supernovae and improving upon previous models.
Contribution
It provides the first calculation of total beta-decay half-lives and unique first-forbidden rates for neutron-rich nickel isotopes in stellar conditions using pn-QRPA.
Findings
pn-QRPA results agree better with experimental data
First-forbidden transitions significantly affect decay rates in neutron-rich nuclei
Inclusion of rank 0 and 1 operators improves theoretical predictions
Abstract
In astrophysical environments, allowed Gamow-Teller (GT) transitions are important, particularly for -decay rates in presupernova evolution of massive stars, since they contribute to the fine-tuning of the lepton-to-baryon content of the stellar matter prior to and during the collapse of a heavy star. In environments where GT transitions are unfavored, first-forbidden transitions become important especially in medium heavy and heavy nuclei. Particularly in case of neutron-rich nuclei, first-forbidden transitions are favored primarily due to the phase-space amplification for these transitions. In this work the total -decay half-lives and the unique first-forbidden(U1F) -decay rates for a number of neutron-rich nickel isotopes, Ni, are calculated using the proton-neutron quasi-particle random phase approximation (pn-QRPA) theory in stellar environment for…
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