17O(p,α)14N reaction measurement at astrophysical energies

M. L. Sergi, C. Spitaleri, R. G. Pizzone, S. V. Burjan, S. Cherubini, A. Coc, M. Gulino, F. Hammache, Z. Hons, B. Irgaziev, G. Kiss, V. Kroha, M. La Cognata, L. Lamia, A. Mukhamedzhanov, S. M R Puglia, G. G. Rapisarda, S. Romano, N. De Séréville, E. Somorjai & 1 others A. Tumino

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The 17O(p,α)14N 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 17O(p,α) 14N reaction via the Trojan Horse Method by applying the approach recently developed for extracting the resonance strength of narrow resonance in the ultra-low energy region.

Original languageEnglish
Title of host publicationAIP Conference Proceedings
PublisherAmerican Institute of Physics Inc.
Pages208-210
Number of pages3
Volume1595
ISBN (Print)9780735412293
DOIs
Publication statusPublished - 2014
Event7th European Summer School on Experimental Nuclear Astrophysics - Sicily, Italy
Duration: Sep 15 2013Sep 27 2013

Other

Other7th European Summer School on Experimental Nuclear Astrophysics
CountryItaly
CitySicily
Period9/15/139/27/13

Fingerprint

astrophysics
novae
asymptotic giant branch stars
massive stars
nuclear fusion
energy

Keywords

  • Direct reactions
  • Nuclear Astrophysics
  • Nucleosynthesis in novae
  • other explosive environments
  • supernovae

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Sergi, M. L., Spitaleri, C., Pizzone, R. G., Burjan, S. V., Cherubini, S., Coc, A., ... Tumino, A. (2014). 17O(p,α)14N reaction measurement at astrophysical energies. In AIP Conference Proceedings (Vol. 1595, pp. 208-210). American Institute of Physics Inc.. https://doi.org/10.1063/1.4875312

17O(p,α)14N reaction measurement at astrophysical energies. / Sergi, M. L.; Spitaleri, C.; Pizzone, R. G.; Burjan, S. V.; Cherubini, S.; Coc, A.; Gulino, M.; Hammache, F.; Hons, Z.; Irgaziev, B.; Kiss, G.; Kroha, V.; La Cognata, M.; Lamia, L.; Mukhamedzhanov, A.; Puglia, S. M R; Rapisarda, G. G.; Romano, S.; De Séréville, N.; Somorjai, E.; Tumino, A.

AIP Conference Proceedings. Vol. 1595 American Institute of Physics Inc., 2014. p. 208-210.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Sergi, ML, Spitaleri, C, Pizzone, RG, Burjan, SV, Cherubini, S, Coc, A, Gulino, M, Hammache, F, Hons, Z, Irgaziev, B, Kiss, G, Kroha, V, La Cognata, M, Lamia, L, Mukhamedzhanov, A, Puglia, SMR, Rapisarda, GG, Romano, S, De Séréville, N, Somorjai, E & Tumino, A 2014, 17O(p,α)14N reaction measurement at astrophysical energies. in AIP Conference Proceedings. vol. 1595, American Institute of Physics Inc., pp. 208-210, 7th European Summer School on Experimental Nuclear Astrophysics, Sicily, Italy, 9/15/13. https://doi.org/10.1063/1.4875312
Sergi ML, Spitaleri C, Pizzone RG, Burjan SV, Cherubini S, Coc A et al. 17O(p,α)14N reaction measurement at astrophysical energies. In AIP Conference Proceedings. Vol. 1595. American Institute of Physics Inc. 2014. p. 208-210 https://doi.org/10.1063/1.4875312
Sergi, M. L. ; Spitaleri, C. ; Pizzone, R. G. ; Burjan, S. V. ; Cherubini, S. ; Coc, A. ; Gulino, M. ; Hammache, F. ; Hons, Z. ; Irgaziev, B. ; Kiss, G. ; Kroha, V. ; La Cognata, M. ; Lamia, L. ; Mukhamedzhanov, A. ; Puglia, S. M R ; Rapisarda, G. G. ; Romano, S. ; De Séréville, N. ; Somorjai, E. ; Tumino, A. / 17O(p,α)14N reaction measurement at astrophysical energies. AIP Conference Proceedings. Vol. 1595 American Institute of Physics Inc., 2014. pp. 208-210
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AU - Cherubini, S.

AU - Coc, A.

AU - Gulino, M.

AU - Hammache, F.

AU - Hons, Z.

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AU - Kiss, G.

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AU - La Cognata, M.

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AU - Rapisarda, G. G.

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AU - Tumino, A.

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AB - The 17O(p,α)14N 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 17O(p,α) 14N reaction via the Trojan Horse Method by applying the approach recently developed for extracting the resonance strength of narrow resonance in the ultra-low energy region.

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