Alessandro Compagnucci

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

^{22}

Ne(α,γ)

^{26}

Mg reaction

24 citations · 64 across the 3 of their papers we have counts for

collaborators

3 papers

nucl-ex2023★ 24 cited

New proton-capture rates on carbon isotopes and their impact on the astrophysical $^{12} C /^{13} C$ ratio

J. Skowronski, A. Boeltzig, G. F. Ciani +43

The $^{12} C /^{13} C$ ratio is a significant indicator of nucleosynthesis and mixing processes during hydrogen burning in stars. Its value mainly depends on the…

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,…

New proton-capture rates on carbon isotopes and their impact on the astrophysical 12C/13C ratio

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

New proton-capture rates on carbon isotopes and their impact on the astrophysical $^{12} C /^{13} C$ ratio

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