First measurement of the 18O(p,α)15N cross section at astrophysical energies
First measurement of the 18O(p,α)15N cross section at astrophysical energies
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Author / Creator
Cognata, M La , Spitaleri, C , Mukhamedzhanov, A , Tribble, R E , Al-Abdullah, T , Banu, A , Cherubini, S , Coc, A , Crucillà, V , Goldberg, V , Gulino, M , Irgaziev, B , Kiss, G G , Lamia, L , Mrazek, J , Pizzone, R G , Puglia, S M R , Rapisarda, G G , Romano, S , Sergi, M L , Tabacaru, G , Trache, L , Trzaska, W , Tudisco, S and Tumino, A
Publisher
Bristol: IOP Publishing
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English
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Bristol: IOP Publishing
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The 18O(p,α)15N reaction rate has been deduced by means of the Trojan horse method. For the first time the contribution of the 20 keV resonance has been directly evaluated, giving a value about 35% larger than the one in the literature. Moreover, the present approach has allowed to improve the accuracy by a factor 8.5, as it is based on the measure...
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Full title
First measurement of the 18O(p,α)15N cross section at astrophysical energies
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TN_cdi_proquest_journals_2579909568
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2579909568
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ISSN
1742-6596,1742-6588
E-ISSN
1742-6596
DOI
10.1088/1742-6596/202/1/012019
