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First results from measurements of capture reactions on Sn and Pd for the γ-process using HECTOR

https://doi.org/10.1016/j.nuclphysa.2025.123124

McDonaugh, JP; Simon, A; Jones, C; Koros, J; Matney, M; Zimmer, L; Bailey, TL; Boomershine, C; Carmichael, S; Fang, R; et al (August 2025, Nuclear Physics A)

Free, publicly-accessible full text available August 1, 2026
Probing the most important ${}^{14}O (α, p) {}^{17}F$ resonance through a study of ${}^{17}F (p, p^{'}) {}^{17}F^{*}$

https://doi.org/10.1103/bljj-k2nv

Coil, S; Bardayan, D W; O'Malley, P D; Bailey, T L; Boomershine, C; Carmichael, S; Dembski, C; Gore, T; Houff, A M; Jones, C; et al (September 2025, Physical Review C)

Free, publicly-accessible full text available September 1, 2026
Strength measurements of the $E_{R}^{lab} = 647$ and 1842 keV resonances in the ${}^{40}{Ca} (p, γ) {}^{41}{Sc}$ reaction and their relevance in novae nucleosynthesis

https://doi.org/10.1103/PhysRevC.111.025804

Sidhu, R S; deBoer, R J; Görres, J; Wiescher, M; Koros, J; Manukyan, K; Matney, M; McDonaugh, J; Picciotto, V; Sanchez, A T; et al (February 2025, Physical Review C)

Here we report on the direct measurement of the resonance strengths of the $E_{R}^{lab} = 647 keV$ and 1842 keV resonances in the ${}^{40}{Ca} (p, γ) {}^{41}{Sc}$ reaction. At novae temperatures, $0.2 < T_{9} < 0.7$ , the ${}^{40}{Ca} (p, γ) {}^{41}{Sc}$ reaction is governed by the low energy resonance at $E_{R}^{lab} = 647 keV$ , whereas the $E_{R}^{lab} = 1842 keV$ resonance serves as a normalization standard for nuclear reaction experiments within the astrophysically relevant energy range. For the $E_{R}^{lab} = 647 keV$ resonance, we obtain a resonance strength $ω γ = (2.51 \pm 0 . 09_{stat} \pm 0 . 22_{syst}) meV$ , with an uncertainty a factor of 2.5 smaller than the previous direct measurement value. For the $E_{R}^{lab} = 1842 keV$ resonance, we obtain a resonance strength $ω γ = (0.148 \pm 0 . 006_{stat} \pm 0 . 013_{syst}) eV$ , which is consistent with previous studies but deviates by $2 σ$ from the most recent measurement. Our results suggest ${}^{40}{Ca}$ to be a strong waiting point in the nucleosynthesis path of oxygen-neon (ONe) novae. Published by the American Physical Society2025
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Free, publicly-accessible full text available February 1, 2026
Breakdown of the Stokes–Einstein relationship and rapid structural ordering in CuZrAl metallic glass-forming liquids

https://doi.org/10.1063/5.0062724

Chen, F. Z.; Mauro, N. A.; Bertrand, S. M.; McGrath, P.; Zimmer, L.; Kelton, K. F. (September 2021, The Journal of Chemical Physics)

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