76 citations · 227 across the 6 of their papers we have counts for
6 papers
First direct limit on the 334 keV resonance strength in the Ne(α,γ)Mg reaction
D. Piatti, E. Masha, M. Aliotta +44
In stars, the fusion of Ne and He may produce either Mg, with the emission of a neutron, or Mg and a ray. At high temperature, the () channel domi…
Ne and Na ejecta from intermediate-mass stars: The impact of the new LUNA rate for Ne(p,)Na
A. Slemer, P. Marigo, D. Piatti +36
We investigate the impact of the new LUNA rate for the nuclear reaction NeNa on the chemical ejecta of intermediate-mass stars, with particular focus on the ther…
-scattering and -induced reaction cross sections of Zn at low energies
A. Ornelas, P. Mohr, Gy. Gyürky +12
Background: alpha-nucleus potentials play an essential role for the calculation of alpha-induced reaction cross sections at low energies in the statistical model... Purpose: The pr…
Direct measurement of low-energy Ne(p,)Na resonances
R. Depalo, F. Cavanna, M. Aliotta +30
The Ne(p,)Na reaction is the most uncertain process in the neon-sodium cycle of hydrogen burning. At temperatures relevant for nucleosynthesis in asymptotic giant…
Improved Direct Measurement of the 64.5 keV Resonance Strength in the 17O(p,a)14N Reaction at LUNA
C. G. Bruno, D. A. Scott, M. Aliotta +32
The O(p,)N reaction plays a key role in various astrophysical scenarios, from asymptotic giant branch stars to classical novae. It affects the synthesis of rare is…
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…