First beta-delayed neutron emission from 54K
ORAL
Abstract
Exotic nuclei in the vicinity of 54Ca have attracted tremendous attention in the last few years owing to the new N=32,34 shell closures emerging with extreme neutron excess [1, 2]. Experimentally, it has been revealed that the N=34 shell gap disappears already in the titanium isotopes where there are two valence protons outside the Z=20 core [3]. Below Z=20, however, it is not yet fully clear how the energy gap evolves as a function of proton number. In order to address the question, the beta decay of 54K was studied at the FRIB Decay Station Initiator (FDSi). Strong Gamow-Teller transitions were observed populating neutron unbound states in 54Ca. In this contribution, I will present the experimental results, including beta-delayed neutron and gamma-ray spectra. In addition, I will discuss the ab-initio calculations with VS-IMSRG as well as the large-scale shell-model calculations we performed to gain insights into the underlying shell structure south of 54Ca.
[1] D. Steppenbeck et al., Nature 502, 207 (2013).
[2] F. Wienholtz et al., Nature 498, 346 (2013).
[3] S. Iimura et al., Phys. Rev. Lett. 130, 012501 (2023).
[1] D. Steppenbeck et al., Nature 502, 207 (2013).
[2] F. Wienholtz et al., Nature 498, 346 (2013).
[3] S. Iimura et al., Phys. Rev. Lett. 130, 012501 (2023).
*This project was supported by the Office of Nuclear Physics, U.S. Department of Energy, under Award No. DE-FG02-96ER40983, No. DE-AC05-00OR22725, and No. DE-AC52-07NA27344, National Nuclear Security Administration under the Stewardship Science Academic Alliances program through DOE Award No. DE-436NA0003899, No. DE-NA0002132, and No. DE-NA0004068, and by NSF Major Research Instrumentation Program Award No. 1919735.
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Presenters
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Zhengyu Xu
- University of Tennessee