Abstract
The β decay of O24 was investigated at NSCL/MSU using a combination of neutron and γ-ray spectroscopy. For the first time, the β-delayed neutron energy spectrum of O24 was measured, revealing three intensely populated, isolated neutron-unbound states in F24. This allowed for the extraction of the decay strength in F24 up to 6.2 MeV. A comprehensive comparison of the experimental results with various nuclear theories, ranging from the empirical shell model to the most advanced ab initio calculations, was conducted. While most theoretical predictions align with the experimental data for low-lying states, discrepancies arise at higher excitation energies. In the transition from O24 to F24, shell model calculations using the empirical USDB interaction predicted the structure of both nuclei without invoking the need for a stronger proton-neutron tensor force, which was postulated for the neighboring isotone F25.
| Original language | English |
|---|---|
| Article number | 034323 |
| Journal | Physical Review C |
| Volume | 110 |
| Issue number | 3 |
| DOIs | |
| State | Published - Sep 2024 |
Funding
This research was partly sponsored by the National Nuclear Security Administration under the Stewardship Science Academic Alliances program through DOE Cooperative Agreements No. DE-NA0003899 and No. DE-NA0004068. This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Contracts No. DE-FG02-96ER40983 (UTK), No. DE-SC0020451 (MSU), and No. DE-AC05-00OR22725 (ORNL). This research was sponsored in part by the National Science Foundation under the Contract No. NSF-MRI-1919735. This work was also supported by the National Nuclear Security Administration through the Nuclear Science and Security Consortium under Award No. DE-NA0003180 and the Stewardship Science Academic Alliances program through U.S. DOE Award No. DOE-DE-NA0003906.