Jul 21 – 26, 2024
APS Conference Center, Argonne
America/Chicago timezone
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Direct measurement of hexacontatetrapole, E6 γ decay from 53mFe

Jul 25, 2024, 9:25 AM
20m
Auditorium (APS Conference Center, Argonne)

Auditorium

APS Conference Center, Argonne

Speaker

A. J. Mitchell (The Australian National University)

Description

First-order electromagnetic processes are the primary mechanism by which excited states in atomic nuclei relax, most-often via single γ-ray emission. Since both the initial- and final-state wave functions possess a well-defined spin and parity, conservation laws impose a characteristic multipolarity for each discrete transition. Nature favours pathways that proceed via the lowest- available multipole order. However, situations arise in which the only available decay pathway is hindered by a larger spin-change requirement. The only proposed observation of a discrete, hexacontatetrapole (E6) transition in nature occurs from the isomeric, T1/2 = 2.54-minute decay of 53mFe. However, there are conflicting claims concerning its γ-decay branching ratio, and a rigorous interrogation of γ-ray sum contributions is lacking [1-3]. Experiments performed at the Australian Heavy Ion Accelerator Facility were used to study the decay of 53mFe. For the first time, sum-coincidence contributions to the weak E6, M5 and E4 decay branches have been firmly quantified using complementary experimental and computational methods [4]. Shell-model calculations were also performed in the full pf model space to investigate the nature of these high-multipolarity transitions. This presentation will provide an overview the experiments, results obtained from this work and their interpretation. The authors are grateful for excellent support from technical staff of the Heavy Ion Accelerator Facility. This work is supported by the Australian Research Council Grants No. DP170101673 and DP170101675, the International Technology Centre Pacific (ITC-PAC) under Contract No. FA520919PA138, and NSF Grant PHY-2110365. Support for the ANU Heavy Ion Accelerator Facility operations through the Australian National Collaborative Research Infrastructure Strategy program is acknowledged.

[1] J. N. Black, W. C. McHarris, and W. H. Kelly, Phys. Rev. Lett. 26, 451 (1971).
[2] J. N. Black, W. C. McHarris, W. H. Kelly, and B. H. Wildenthal, Phys. Rev. C 11, 939 (1975).
[3] D. Geesaman, Spin gap isomers in 52Fe,
53Fe, and 54Co, Ph.D. thesis, State University of New
York, Stony Brook (USA) (1976).
[4] T. Palazzo et al., Phys. Rev. Lett. 130, 122503 (2023).

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