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THM determination of the 65 keV resonance strength intervening in the O-17(p,alpha)N-14 reaction rate

M.L. Sergi C. Spitaleri S.V. Burjan S. Cherubini A. Coc 1 M. Gulino F. Hammache 2 Z. Hons B. Irgaziev G.G. Kiss V. Kroha M. La Cognata L. Lamia A. Mukhamedzhanov R.G. Pizzone S.M.R. Puglia G.G. Rapisarda S. Romano N. de Sereville 2 E. Somorjai A. Tumino
1 CSNSM AN
CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse, CSNSM - Centre de Sciences Nucléaires et de Sciences de la Matière
2 IPNO - Institut de Physique Nucléaire d'Orsay
Abstract : The O-17(p,alpha)N-14 reaction is of paramount importance for the nucleosynthesis in a number of stellar sites, including red giants (RG), asymptotic giant branch (AGB) stars, massive stars and classical novae. We report on the indirect study of the O-17(p,alpha)N-14 reaction via the Trojan Horse Method by applying the approach recently developed for extracting the resonance strength of the narrow resonance at E-c.m.(R) = 65 keV (E-X = 5.673 MeV). The strength of the 65 keV resonance in the O-17(p,alpha)N-14 reaction, measured by means of the THM, has been used to renormalize the corresponding resonance strength in the O-17 + p radiative capture channel.
Keywords : and other explosive environments supernovae Nucleosynthesis in novae ALPHA)N-14 Direct reactions O-18(P O-17(P Nuclear Astrophysics TROJAN HORSE METHOD THERMONUCLEAR REACTION-RATES ASTROPHYSICAL ENERGIES CROSS-SECTION NUCLEOSYNTHESIS
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Conference papers
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http://hal.in2p3.fr/in2p3-01165469
Contributor : Emilie Bonnardel <>
Submitted on : Friday, June 19, 2015 - 12:23:43 PM
Last modification on : Saturday, October 3, 2020 - 3:54:47 AM

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M.L. Sergi, C. Spitaleri, S.V. Burjan, S. Cherubini, A. Coc, et al.. THM determination of the 65 keV resonance strength intervening in the O-17(p,alpha)N-14 reaction rate. EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (V). FROM NUCLEI TO STARS: Carpathian Summer School of Physics 2014, Jul 2014, Sinaia, Romania. pp.392-396, ⟨10.1063/1.4909608⟩. ⟨in2p3-01165469⟩

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