Carlo Bruno

Dr CG Bruno

Carlo is a member of the following School research institute, research group and research area:

Carlo has featured in the following recent School news stories:

Characterization of the LUNA neutron detector array for the measurement of the 13C(α,n)16O reaction DOI
L. Csedreki, G F Ciani, J Balibrea-Correa, A Best, M. Aliotta, F Barile, D Bemmerer, A Boeltzig, C Broggini, C. G. Bruno, A Caciolli, T. Davinson et al., Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 994 (2021)
The baryon density of the Universe from an improved rate of deuterium burning DOI
M. Aliotta, C. G. Bruno, Thomas Chillery, T. Davinson and LUNA Collaboration, Nature, 587, p. 210-213 (2020)
Underground experimental study finds no evidence of low-energy resonance in the 6Li(p,γ)7Be reaction DOI
Thomas Chillery, M. Aliotta, C. G. Bruno, T. Davinson and LUNA Collaboration, Physical Review C, 102, 5 (2020)
Setup commissioning for an improved measurement of the D(p,gamma)3He cross section at Big Bang Nucleosynthesis energies DOI
(LUNA Collaboration), European Physical Journal A, 56 (2020)
A new approach to monitor 13C-targets degradation in situfor 13C(α,n)16O cross-section measurements at LUNA DOI
G F Ciani, L. Csedreki, J Balibrea-Correa, A. Best, Marialuisa Aliotta, F Barile, D. Bemmerer, A. Boeltzig, C. Broggini, C. G. Bruno, A Caciolli, Thomas Davinson et al., European Physical Journal A: Hadrons and Nuclei (2020)