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:

Direct measurement of the 13C(α,n)16O cross section into the s-process Gamow peak
LUNA Collaboration, G F Ciani, M. Aliotta, A Best, C. G. Bruno, T Chillery and T. Davinson, Physical Review Letters (2021)
Low-energy resonances in the 18O (p,Υ) 19F reaction DOI
LUNA Collaboration, F R Pantaleo, A Boeltzig, M. Aliotta, C. G. Bruno, T Chillery and T. Davinson, Physical Review C, 104, 2, p. 1-12 (2021)
ß-delayed neutron emission of r-process nuclei at the N=82 shell closure DOI
O. Hall, T. Davinson, A. Estrade, J. Liu, G. Lorusso, F. Montes, S. Nishimura, V. H. Phong, P. J. Woods, J. Agramunti, D. S. Ahn, A. Algora, C. G. Bruno et al., Physics Letters B, 816, p. 1-7 (2021)
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
LUNA Collaboration, M. Aliotta, C. G. Bruno, Thomas Chillery and T. Davinson, Nature, 587, p. 210-213 (2020)