291 citations · 3.6k across the 81 of their papers we have counts for
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Nuclear Physics Mid Term Plan at LNGS
R. Buompane, F. Cavanna, C. Curceanu +59
The Istituto Nazionale di Fisica Nucleare-Laboratori Nazionali del Gran Sasso (LNGS) is one of the largest underground physics laboratory, a very peculiar environment suited for ex…
First direct measurement of the 64.5 keV resonance strength in O(p,)F reaction
R. M. Gesuè, G. F. Ciani, D. Piatti +50
The CNO cycle is one of the most important nuclear energy sources in stars. At temperatures of hydrostatic H-burning (20 MK T 80 MK) the O(p,)F reaction ra…
Experimental Be production cross section from the Li(p,n)Be reaction at E MeV
Á. Tóth, Gy. Gyürky, E. Papp +1
The Li(p,n)Be reaction is widely used as neutron source for neutron induced reaction cross section measurements, and for Be radioactive source production. There are two…
New proton-capture rates on carbon isotopes and their impact on the astrophysical ratio
J. Skowronski, A. Boeltzig, G. F. Ciani +43
The ratio is a significant indicator of nucleosynthesis and mixing processes during hydrogen burning in stars. Its value mainly depends on the…
Experimental determination of the He(,)Be reaction cross section above the Be proton separation threshold
Á. Tóth, T. Szücs, T. N. Szegedi +4
The He(,)Be reaction plays a major role both in the BBN producing the majority of the primordial Li, and in the pp-chain, where it is the branching point. As a fe…
Cross section measurement of the 12C(p,gamma)13N reaction with activation in a wide energy range
Gy. Gyürky, L. Csedreki, T. Szücs +3
The CNO cycle is one of the fundamental processes of hydrogen burning in stars. The first reaction of the cycle is the radiative proton capture on 12C and the rate of this 12C(p,ga…