253 citations · 580 across the 5 of their papers we have counts for
5 papers
Cross Sections for proton induced high energy -ray emission (PIGE) in reaction F(p,)O at incident proton energies between 1.5 and 4 MeV
P. Cabanelas, J. Cruz, M. Fonseca +11
We have studied the high energy gamma-rays produced in the reaction F(p,)O for incident proton energies from 1.5 to 4.0 MeV over NaF/Ag and CaF/Ag thin target…
First measurement of the 14N(p,gamma)15O cross section down to 70 keV
A. Lemut, D. Bemmerer, F. Confortola +28
In stars with temperatures above 20*10^6 K, hydrogen burning is dominated by the CNO cycle. Its rate is determined by the slowest process, the 14N(p,gamma)15O reaction. Deep underg…
S-factor of 14N(p,gamma)15O at astrophysical energies
G. Imbriani, H. Costantini, A. Formicola +31
The astrophysical S-factor of 14N(p,gamma)15O has been measured for effective center-of-mass energies between E_eff = 119 and 367 keV at the LUNA facility using TiN solid targets a…
Feasibility of low energy radiative capture experiments at the LUNA underground accelerator facility
D. Bemmerer, F. Confortola, A. Lemut +29
The LUNA (Laboratory Underground for Nuclear Astrophysics) facility has been designed to study nuclear reactions of astrophysical interest. It is located deep underground in the Gr…
The bottleneck of the CNO burning and the age of the Globular Clusters
G. Imbriani, H. Costantini, A. Formicola +27
The transition between the Main Sequence and the Red Giant Branch in low mass stars is powered by the onset of the CNO burning, whose bottleneck is the N(p,O. The L…