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Indirect measurement of O-17(p,alpha)N-14 cross section at ultra-low energies
- 1.0486832 - ÚJF 2018 GB eng C - Conference Paper (international conference)
Sergi, M. L. - Spitaleri, C. - Coc, A. - Mukhamedzhanov, A. - Burjan, Václav - Cherubini, S. - Crucilla, V. - Gulino, M. - Hammache, F. - Hons, Zdeněk - Irgaziev, B. - Kiss, G. G. - Kroha, Václav - La Cognata, M. - Lamia, L. - Pizzone, R. G. - Puglia, S. M. R. - Rapisarda, G. G. - Romano, S. - de Sereville, N. - Somorjai, E. - Tudisco, S. - Tumino, A.
Indirect measurement of O-17(p,alpha)N-14 cross section at ultra-low energies.
Journal of Physics: Conference Series. Vol. 202. Bristol: IOP Publishing, 2010, č. článku 012021. ISSN 1742-6588.
[4th International Conference on Nuclear Physics in Astrophysics. Frascati (IT), 08.06.2009-12.06.2009]
Institutional support: RVO:61389005
Keywords : astrophysics * nuclear reaction * reaction rates
OECD category: Nuclear physics
The indirect measurement of O-17(p,alpha)N-14 cross section was performed by means of the Trojan Horse Method. This approach allowed to investigate the ultra-low energy range (E-c.m.= 0-300 keV) relevant for several astrophysics environments, where two resonant levels of F-18 at E-c.m.(R) = 65 keV and E-c.m.(R) = 183 keV play a significant role in the reaction rate determination.
Permanent Link: http://hdl.handle.net/11104/0281546
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