140 citations · 265 across the 6 of their papers we have counts for
6 papers
Precision study of ground state capture in the 14N(p,gamma)15O reaction
M. Marta, A. Formicola, Gy. Gyurky +28
The rate of the hydrogen-burning carbon-nitrogen-oxygen (CNO) cycle is controlled by the slowest process, 14N(p,gamma)15O, which proceeds by capture to the ground and several excit…
Photodisintegration studies on p-nuclei: The case of Mo and Sm isotopes
C. Nair, A. R. Junghans, M. Erhard +10
In explosive stellar environments like supernovae, the temperatures are high enough for the production of heavy neutron-deficient nuclei, the socalled p-nuclei. Up to now, the know…
Measurement of 25Mg(p; gamma)26Al resonance strengths via gamma spectrometry
A. Formicola, A. Best, G. Imbriani +28
The COMPTEL instrument performed the first mapping of the 1.809 MeV photons in the Galaxy, triggering considerable interest in determing the sources of interstellar 26Al. The predi…
Ground state capture in N(p,)O studied above the 259 keV resonance at LUNA
H. P. Trautvetter, D. Bemmerer, R. Bonetti +29
We report on a new measurement of N(p,)O for the ground state capture transition at = 360, 380 and 400 keV, using the 400 kV LUNA accelerator. The true coinc…
Comparison of the LUNA 3He(alpha,gamma)7Be activation results with earlier measurements and model calculations
Gy. Gyurky, D. Bemmerer, F. Confortola +27
Recently, the LUNA collaboration has carried out a high precision measurement on the 3He(alpha,gamma)7Be reaction cross section with both activation and on-line gamma-detection met…
Astrophysical S-factor of the 3He(alpha,gamma)7Be reaction measured at low energy via prompt and delayed gamma detection
F. Confortola, D. Bemmerer, H. Costantini +28
Solar neutrino fluxes depend both on astrophysical and on nuclear physics inputs, namely on the cross sections of the reactions responsible for neutrino production inside the Solar…