Jul 26–31, 2026
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Direct Observation of Superallowed Alpha Decay of 104Te

Jul 28, 2026, 2:50 p.m.
20m
Fletcher Challenge Canada (Simon Fraser University Harbour Centre)

Fletcher Challenge Canada

Simon Fraser University Harbour Centre

515 West Hastings St, Vancouver, B.C. V6B 5K3

Speaker

Ian Cox (Argonne National Laboratory)

Description

Historically, the simplest $\alpha$ decay is that of $^{212}$Po, which is conceptualized as a doubly magic $^{208}$Pb core with a valence $\alpha$ particle. For decades, this well-measured isotope has stood as the baseline for $\alpha$-decay models and comparison among other $\alpha$-emitting nuclei. However, a lighter region of $\alpha$ radioactivity was found in neutron-deficient tellurium and xenon isotopes resulting from the Z=50 and N=50 shell closures. Discovered by Macfarlane and Siivola, these decays are enhanced relative to $^{212}$Po, allowing the authors to coin the term “superallowed” $\alpha$ decay for the nuclei [1]. The self-conjugate decay of $^{104}$Te to $^{100}$Sn was then postulated to be the most enhanced $\alpha$ decay due to an increase in proton-neutron correlations. Two events of $^{104}$Te were measured by Auranen et al. Despite limited statistics, the authors placed an upper limit on the half-life via the decay chain of $^{108}$Xe [2]. This work reports an experiment at RIKEN RIBF using the fragmentation of $^{124}$Xe to produce the decay chain of $^{108}$Xe to $^{104}$Te to $^{100}$Sn [3]. In preparation for the short lifetime, a fast-response charged particle detector was utilized [4]. The half-life of $^{104}$Te was measured for the first time and is found to be the fastest ground-state $\alpha$-emitting nucleus known to date. Additionally, the deduced preformation demonstrates that the enhancement is greater for $^{104}$Te than for any other $\alpha$-decaying nucleus [3]. This presentation will compare the results with previous results from Auranen et al and numerous theoretical models.

[1] R. Macfarlane and A. Siivola, Phys. Rev. Lett. 14, 144 (1965)
[2] K. Auranen, et al. Phys. Rev. Lett. 121, 182501 (2018)
[3] I. Cox, et al. Nature, in Press (2026) https://doi.org/10.21203/rs.3.rs-7991707/v1
[4] Y. Xiao, et al. Phys. Rev. C 100, 034315 (2019)

This work was supported by US DOE No. DE-FG02-96ER40983 and NNSA No. DE-NA0003899

Authors

Ian Cox (Argonne National Laboratory) Robert Grzywacz (University of Tennessee)

Co-authors

Thomas King (Oak Ridge National Laboratory) Krzysztof Rykaczewski (Oak Ridge National Laboratory) Shunji Nishimura (RIKEN Nishina Center) Naoki FUKUDA (RIKEN Nishina Center) Noritaka Kitamura (Center for Nuclear Study, University of Tokyo) Shintaro Go (RIKEN) Chiara Mazzocchi (University of Warsaw) James Allmond (ORNL) Aleksander Augustyn (National Centre for Nuclear Research) Nico Braukman (University of Tennessee Knoxville) Pierre Brionnet (RIKEN Nishina Center) Arwin Esmaylzadeh (IKP University of Koeln) Julia Fischer (IKP University of Koeln) Gabriel Garcia de Lorenze (Grupo de Física Nuclear, EMFTEL & IPARCOS, Universidad Complutense de Madrid) Shutaro Hanai (Center for Nuclear Study, University of Tokyo) Donnie Hoskins (University of Tennessee, Knoxville) Nobu Imai (Center for Nuclear Study, Univ. of Tokyo) Kay Kolos (Lawrence Livermore National Laboratory) Agnieszka Korgul (University of Warsaw) Ben Kreider (University of Tennessee, Knoxville) Shin'ichiro Michimasa (RIKEN Nishina Center) Katsuhisa Nishio (Japan Atimic Energy Agency) Vi Phong (RIKEN Nishina Center) Thomas Ruland (Oak Ridge National Laboratory) Hiroyoshi Sakurai (RIKEN) Dr Yohei Shimizu (RIKEN Nishina Center for Accelerator-Based Science) Aleksandra Skruch (University of Warsaw) Hiroshi Suzuki (RIKEN Nishina Center) Hiroyuki Takeda (RIKEN Nishina Center) Yasuhiro Togano (RIKEN Nishina Center) Zhengyu Xu (University of Tennessee, Knoxville) Masahiro Yoshimoto (RIKEN Nishina Center)

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