55 citations · 269 across the 11 of their papers we have counts for
11 papers
Setup commissioning for an improved measurement of the D(p,gamma)3He cross section at Big Bang Nucleosynthesis energies
V. Mossa, K. Stöckel, F. Cavanna +44
Among the reactions involved in the production and destruction of deuterium during Big Bang Nucleosynthesis, the deuterium-burning D(p,gamma)3He reaction has the largest uncertaint…
Astrophysical S-factor of the reaction at 0.4 -- 1.3\,MeV
L. Wagner, S. Akhmadaliev, M. Anders +18
The reaction is the slowest reaction of the carbon-nitrogen cycle of hydrogen burning and thus determines its rate. The precise knowl…
Constraining the Be()B -factor with the new precise Be solar neutrino flux from Borexino
Marcell P. Takács, Daniel Bemmerer, Arnd R. Junghans +1
Among the solar fusion reactions, the rate of the Be()B reaction is one of the most difficult to determine rates. In a number of previous experiments, its astrophysica…
Origin of meteoritic stardust unveiled by a revised proton-capture rate of O
M. Lugaro, A. I. Karakas, C. G. Bruno +34
Stardust grains recovered from meteorites provide high-precision snapshots of the isotopic composition of the stellar environment in which they formed. Attributing their origin to…
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…
The impact of the revised ON reaction rate on O stellar abundances and yields
O. Straniero, C. G. Bruno, M. Aliotta +33
Context. Material processed by the CNO cycle in stellar interiors is enriched in 17O. When mixing processes from the stellar surface reach these layers, as occurs when stars become…
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…
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…
Constraining Big Bang lithium production with recent solar neutrino data
Marcell P. Takács, Daniel Bemmerer, Tamás Szücs +1
The 3He(α,γ)7Be reaction affects not only the production of 7Li in Big Bang nucleosynthesis, but also the fluxes of 7Be and 8B neutrinos from the Sun. This double role is exploited…
Determination of gamma-ray widths in N using nuclear resonance fluorescence
T. Szücs, D. Bemmerer, A. Caciolli +9
The stable nucleus N is the mirror of O, the bottleneck in the hydrogen burning CNO cycle. Most of the N level widths below the proton emission threshold are k…