Alessandro Compagnucci

most citedFirst direct limit on the 334 keV resonance strength in the

^{22}

Ne(α,γ)

^{26}

Mg reaction

24 citations · 40 across the 2 of their papers we have counts for

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nucl-ex2022★ 24 cited

First direct limit on the 334 keV resonance strength in the $^{22}$ Ne(α,γ) $^{26}$ Mg reaction

D. Piatti, E. Masha, M. Aliotta +44

In stars, the fusion of $^{22}$ Ne and $^{4}$ He may produce either $^{25}$ Mg, with the emission of a neutron, or $^{26}$ Mg and a $γ$ ray. At high temperature, the ( $α, n$ ) channel domi…

nucl-ex2022★ 16 cited

Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars

Chemseddine Ananna, Francesco Barile, Axel Boeltzig +11

Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy. Unfortunately,…

First direct limit on the 334 keV resonance strength in the 22Ne(α,γ)26Mg reaction

Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars

First direct limit on the 334 keV resonance strength in the $^{22}$ Ne(α,γ) $^{26}$ Mg reaction