Speaker
Description
Electron-capture rates on medium-heavy nuclei play a crucial role in the last stage of core-collapse supernovae of massive stars during the deleptonization process. While these rates are highly sensitive to their Gamow-Teller (GT) strength [1], their direct measurement remains experimentally challenging. As an isospin analogue, the isovector spin-flip M1 (IVSM1) response offers an alternative probe, which we investigate in the $N=50$ isotones $^{90}$Zr and $^{92}$Mo. The presence of two extra protons in $^{92}$Mo's proton $g_{9/2}$ orbital beyond the closed pf shell makes it a potential candidate for exhibiting enhanced isovector spin-flip M1 (IVSM1) strength in comparison to $^{90}$Zr. Furthermore, $^{92}$Mo is of additional interest as it provides a testing ground for exploring the recently proposed $\nu r$ process [2]. The complete characterization of dipole strength for both isotones in terms of E1 and M1 strength has been studied using nuclear resonance fluorescence (NRF) with the Clover array, a newly developed hybrid array of HPGe Clover and LaBr$_3$ detectors at the High Intensity $\gamma$-ray Source (HI$\gamma$S) facility of the Triangle Universities Nuclear Laboratory, Duke University using fully-polarized $\gamma$-ray beams with a beam-energy resolution of about $3\%$. By measuring asymmetries of ground-state transitions in an integral approach, we aim to obtain the overall M1/E1 ground-state transition strength up to 10 MeV. The experimental setup, status, and first results of the analysis will be presented.
This work has been supported by DFG Project Nos. 279384907–SFB 1245, 499256822-GRK 2891, and U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Grants No. DE-FG02-97ER41041 (UNC), and No. DE-FG02-97ER41033 (Duke, TUNL).
[1] K. Langanke et al., Rep. Prog. Phys. 84, 066301 (2021).
[2] Z. Xiong et al., Physical Review L. 132, 192701 (2024).