collaborators

7 papers

nucl-ex2025

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…

nucl-ex2025

Improved -factor of the C(p,)N reaction at 330-740 keV and parameters of resonances at 448 keV and 551 keV

J. Skowronski, E. Masha, D. Piatti +23

The C(p,)N reaction is the second reaction of the CNO cycle. This cycle takes place in our Sun and fuels massive, Red, and Asymptotic Giant Branch stars. The $^{1…

nucl-ex2025

Advances in Radiative Capture Studies at LUNA with a Segmented BGO Detector

Jakub Skowronski, Riccardo Maria Gesuè, Axel Boeltzig +43

Studies of charged-particle reactions for low-energy nuclear astrophysics require high sensitivity, which can be achieved by means of detection setups with high efficiency and low…

physics.ins-det2025

Low-energy Cross Section Measurements of Deep Underground at LUNA

Jakub Skowronski, Axel Boeltzig

The reaction cross section is currently under investigation in the low-background environment of the Laboratory for Underground Nuclear…

nucl-ex2025

Improved direct measurement of low-energy resonances in the Ne(p,)Na reaction

R. S. Sidhu, F. Casaburo, E. Masha +57

In the nova temperature range, 0.1 GK 0.4 GK, several low-energy resonances dominate the Ne(p,)Na reaction rate, which is currently affected by large unce…

nucl-ex2025

Total cross section of N+ from 0.1 to 12~MeV

R. J. deBoer, R. Arquette, D. Bemmerer +18

The reaction NC is one of the main neutron poisons during -process nucleosynthesis. In addition, the reaction provides insight into the yields of atmospheric…