D. Rapagnani

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

^{22}

Ne(α,γ)

^{26}

Mg reaction

24 citations · 27 across the 2 of their papers we have counts for

collaborators

2 papers

physics.ins-det2025★ 3 cited

Towards a comprehensive study of the 14N(p,g)15O astrophysical key reaction: Description of the experimental technique including novel target preparation

A. Compagnucci, A. Formicola, M. Campostrini +46

While the 14N(p,g)15O reaction plays a key role in the hydrogen-burning processes in various stellar conditions, its reaction rate is not known with sufficient precision. Therefore…

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…

Towards a comprehensive study of the 14N(p,g)15O astrophysical key reaction: Description of the experimental technique including novel target preparation

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

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