Pregled bibliografske jedinice broj: 1049142
Study of Nuclear Structure of13C and20Ne by Low Energy Nuclear Reactions
Study of Nuclear Structure of13C and20Ne by Low Energy Nuclear Reactions // Journal of Physics: Conference Series 569, 3rd International Workshop on "State of the Art in Nuclear Cluster Physics".
Yokohama, Japan, 2014. 012068, 6 doi:10.1088/1742-6596/569/1/012068 (predavanje, međunarodna recenzija, sažetak, znanstveni)
CROSBI ID: 1049142 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Study of Nuclear Structure of13C and20Ne by Low Energy Nuclear Reactions
Autori
Lombardo, I. ; Campajola, L. ; Dell'Aquila, Daniele ; Commara, M. La. ; Ordine, A. ; Rosato, E. ; Spadaccini, G. ; Vigilante, M.
Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, sažetak, znanstveni
Izvornik
Journal of Physics: Conference Series 569, 3rd International Workshop on "State of the Art in Nuclear Cluster Physics".
/ - , 2014
Skup
3rd International Workshop on State of the Art in Nuclear Cluster Physics (SOTANCP)
Mjesto i datum
Yokohama, Japan, 26.05.2014. - 30.05.2014
Vrsta sudjelovanja
Predavanje
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
Electrostatic accelerators ; Barrier energy ; Direct kinematics ; Emission threshold ; Excitation function ; High resolution ; Low energy nuclear reactions ; Nuclear structure ; Resonant scattering ; Nuclear reactions
Sažetak
We report some recent experimental results on the spectroscopy of 13C and 20Ne nuclei by means of low energy nuclear reactions carried out with high resolution electrostatic accelerators. In the case of 13C we investigated the possible existence of a-cluster states above the a emission threshold by means of low energy elastic resonant scattering α+9Be in direct kinematics. Excitation functions show the presence of various resonances that have been reproduced by R-matrix fit. We studied also the structure of 20Ne by means of the 19F(p, α0) reaction at sub-barrier energies. The spectroscopy of 20Ne excited states in the region Ex 13.5-14.0 MeV can be probed by analyzing experimental angular distributions and excitation functions. This reaction plays an important role also in the CNOF cycle and is an important ingredient to describe hydrogen-induced destruction of fluorine in massive stars. For this reason we investigated the trend of S- factor, that has been compared with results previously reported in the literature.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
Citiraj ovu publikaciju:
Časopis indeksira:
- Web of Science Core Collection (WoSCC)
- Conference Proceedings Citation Index - Science (CPCI-S)
- Scopus