Beta decay of the new isotopesK52,Ca52, andSc52; a test of the shell model far from stability

Abstract
The nuclides K52, Ca52, and Sc52 have been produced by fragmentation of a uranium target with a 600 MeV proton beam. The subsequent β decays to the daughter nuclei Ca52, Sc52, and Ti52 have been studied by neutron and γ spectroscopy on sources obtained from on-line mass separation. β decay energies have been determined by β-γ coincidence spectroscopy. In addition to the short half-life of K52 (T1/2=110±30 ms), we attributed two different half-lives (T1/2=4.6±0.3 s and T1/2=8.2±0.2 s) to Ca52 and Sc52, respectively. A decay scheme has been established for K52 involving five β branches to delayed neutron emitting states between 6.6 and 10.3 MeV and one β branch to a bound level at Ex=2.56 MeV. The Ca52 decay scheme accounts for β branches to four levels at 1.64, 2.75, 3.46, and 4.27 MeV for which the deduced logft values restrict the angular momentum and parity to Jπ =1+. For the Sc52 ground state, strong β transitions to the 2+ (1.05 MeV) and the (4+) (2.32 MeV) levels in Ti52 strongly favor a Jπ =3+ attribution. The measured Qβ values for the Ca52 (5.7±0.2 MeV) and Sc52 (8.02±0.25 MeV) decay are noticeably lower than expected from mass systematics. The energy level diagrams of Ca52, Sc52, and Ti52 nuclei have been calculated in the framework of the shell model with a realistic interaction. Good agreement between theory and experiment is achieved as well for excitation energies as for mass excesses, assuring then the applicability of the theory to this region of nuclei far from stability.

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