76 citations · 377 across the 18 of their papers we have counts for
18 papers
Real-Time Readout System Design for the BULLKID-DM Experiment: Enhancing Dark Matter Search Capabilities
T. Muscheid, R. Gartmann, L. E. Ardila-Perez +41
The BULLKID-DM experiment aims to detect WIMP-like potential Dark Matter particles with masses below 1 GeV/c^2. Sensing these particles is challenging, as it requires nuclear recoi…
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…
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…
Solid Target production for Astrophysical Reasearch: the European target laboratory partnership in ChETEC-INFRA
Roberta Spartà, Alexandra Spiridon, Rosanna Depalo +28
The joint work of European target laboratories in the ChETEC-INFRA project is presented, to face the new experimental challenges of nuclear astrophysics. In particular, results are…
Characterization of the LUNA neutron detector array for the measurement of the 13C(a,n)16O reaction
L. Csedreki, G. F. Ciani, J. Balibrea-Correa +46
We introduce the LUNA neutron detector array developed for the investigation of the 13C(a,n)16O reaction towards its astrophysical s-process Gamow peak in the low-background enviro…
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…