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The 65 keV resonance in the O-17(p,alpha)N-14 thermonuclear reaction

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    SYSNO ASEP0346799
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleThe 65 keV resonance in the O-17(p,alpha)N-14 thermonuclear reaction
    Author(s) Sergi, M. L. (IT)
    Spitaleri, C. (IT)
    Coc, A. (FR)
    Mukhamedzhanov, A. M. (US)
    Burjan, Václav (UJF-V) RID, ORCID, SAI
    Gulino, M. (IT)
    Hammache, F. (FR)
    Hons, Zdeněk (UJF-V) RID, ORCID
    Irgaziev, B. (PK)
    Kiss, G.G. (IT)
    Kroha, Václav (UJF-V) RID
    La Cognata, M. (IT)
    Lamia, L. (IT)
    Pizzone, R. G. (IT)
    de Sereville, N. (FR)
    Somorjai, E. (HU)
    Source TitleNuclear Physics. A. - : Elsevier - ISSN 0375-9474
    Roč. 834, 1-4 (2010), 676C-678C
    Number of pages3 s.
    Action10th International Conference on Nucleus-Nucleus Collisions (NN2009)
    Event date16.08.2009-21.08.2009
    VEvent locationBeijing
    CountryCN - China
    Event typeWRD
    Languageeng - English
    CountryNL - Netherlands
    KeywordsREACTION-RATES ; ENERGIES
    Subject RIVBG - Nuclear, Atomic and Molecular Physics, Colliders
    CEZAV0Z10480505 - UJF-V (2005-2011)
    UT WOS000275930800174
    DOI10.1016/j.nuclphysa.2010.01.122
    AnnotationThe 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.
    WorkplaceNuclear Physics Institute
    ContactMarkéta Sommerová, sommerova@ujf.cas.cz, Tel.: 266 173 228
    Year of Publishing2011
Number of the records: 1  

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