activity
20172026
most citedDirect measurement of the 13C(α,n)16O cross section into the s-process Gamow peak

64 citations · 198 across the 15 of their papers we have counts for

collaborators
Showing nucl-exShow all

15 papers · 1 filter

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-ex20259 cited

First Proton-Induced Cross Sections on a Stored Rare Ion Beam: Measurement of 118Te(p,γ) for Explosive Nucleosynthesis

F. Dellmann, J. Glorius, Yu. A. Litvinov +75

We present the first nuclear cross-section measurements of (p,γ) and (p,n) reactions on 118Te at energies relevant for the γ-process nucleosynthesis. Absolute cross-section values…

nucl-ex202527 cited

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…

nucl-ex20252 cited

Status and future directions for direct cross-section measurements of the 13C(a,n)16O reaction for astrophysics

L. Csedreki, Gy. Gyürky, D. Rapagnani +45

The 13C(a,n)16O reaction is the main neutron source of the s-process taking place in thermally pulsing AGB stars and it is one of the main candidate sources of neutrons for the i-p…

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 uncer…

nucl-ex2025

A Comparative Analysis of R-Matrix Fitting: CN as Test Case

J. Skowronski, D. Piatti, D. Rapagnani +49

In nuclear astrophysics, the accurate determination of nuclear reaction cross sections at astrophysical energies is critical for understanding stellar evolution and nucleosynthesis…