K. Stöckel

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

^{22}

Ne(α,γ)

^{26}

Mg reaction

24 citations · 26 across the 2 of their papers we have counts for

collaborators

2 papers

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…

physics.ins-det2016★ 2 cited

Progress of the Felsenkeller shallow-underground accelerator for nuclear astrophysics

D. Bemmerer, F. Cavanna, T. E. Cowan +15

Low-background experiments with stable ion beams are an important tool for putting the model of stellar hydrogen, helium, and carbon burning on a solid experimental foundation. The…

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

Progress of the Felsenkeller shallow-underground accelerator for nuclear astrophysics

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