Improved results on extraction of 11B(p,α0) 8Be and 10B(p,α)7Be S(E)-factor through the Trojan Horse Method

S. M R Puglia, L. Lamia, S. Romano, C. Spitaleri, N. Carlin, S. Cherubini, M. Del Gulino, M. G. Santo, V. Kroha, S. Kubono, M. La Cognata, C. Li, R. G. Pizzone, W. Qungang, G. G. Rapisarda, M. L. Sergi, E. Somorjai, F. Souza, S. Szanto De Tudisco, A. ToledoA. Tumino, Y. Wakabayashi, H. Yamaguchi

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

Abstract

In this work the analysis of the 10B(p,α)7Be and 11B(p,α)8Be reactions, studied via the indirect Trojan Horse Method (THM), is discussed. In the astrophysical context of light nuclei LiBeB depletion, the above mentioned reactions are the main responsible for the destruction of boron in the stellar interior. The THM application allows their investigation in the astrophysically relevant energy region, around the Gamow Peak (≈10 keV), overcoming the problems due to the presence of the Coulomb barrier and electron screening effect. The experimental procedure and the preliminary results are shown.

Original languageEnglish
Title of host publicationAIP Conference Proceedings
Pages375-377
Number of pages3
Volume1269
DOIs
Publication statusPublished - 2010
Event10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10 - Osaka, Japan
Duration: Mar 8 2010Mar 10 2010

Other

Other10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10
CountryJapan
CityOsaka
Period3/8/103/10/10

Fingerprint

stellar interiors
destruction
astrophysics
depletion
boron
screening
nuclei
electrons
energy

Keywords

  • Abundances-Nuclear astrophysics
  • S(E)-factor
  • Stars
  • Trojan Horse Method-Nuclear Astrophysics

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Puglia, S. M. R., Lamia, L., Romano, S., Spitaleri, C., Carlin, N., Cherubini, S., ... Yamaguchi, H. (2010). Improved results on extraction of 11B(p,α0) 8Be and 10B(p,α)7Be S(E)-factor through the Trojan Horse Method. In AIP Conference Proceedings (Vol. 1269, pp. 375-377) https://doi.org/10.1063/1.3485171

Improved results on extraction of 11B(p,α0) 8Be and 10B(p,α)7Be S(E)-factor through the Trojan Horse Method. / Puglia, S. M R; Lamia, L.; Romano, S.; Spitaleri, C.; Carlin, N.; Cherubini, S.; Del Gulino, M.; Santo, M. G.; Kroha, V.; Kubono, S.; La Cognata, M.; Li, C.; Pizzone, R. G.; Qungang, W.; Rapisarda, G. G.; Sergi, M. L.; Somorjai, E.; Souza, F.; Szanto De Tudisco, S.; Toledo, A.; Tumino, A.; Wakabayashi, Y.; Yamaguchi, H.

AIP Conference Proceedings. Vol. 1269 2010. p. 375-377.

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

Puglia, SMR, Lamia, L, Romano, S, Spitaleri, C, Carlin, N, Cherubini, S, Del Gulino, M, Santo, MG, Kroha, V, Kubono, S, La Cognata, M, Li, C, Pizzone, RG, Qungang, W, Rapisarda, GG, Sergi, ML, Somorjai, E, Souza, F, Szanto De Tudisco, S, Toledo, A, Tumino, A, Wakabayashi, Y & Yamaguchi, H 2010, Improved results on extraction of 11B(p,α0) 8Be and 10B(p,α)7Be S(E)-factor through the Trojan Horse Method. in AIP Conference Proceedings. vol. 1269, pp. 375-377, 10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10, Osaka, Japan, 3/8/10. https://doi.org/10.1063/1.3485171
Puglia SMR, Lamia L, Romano S, Spitaleri C, Carlin N, Cherubini S et al. Improved results on extraction of 11B(p,α0) 8Be and 10B(p,α)7Be S(E)-factor through the Trojan Horse Method. In AIP Conference Proceedings. Vol. 1269. 2010. p. 375-377 https://doi.org/10.1063/1.3485171
Puglia, S. M R ; Lamia, L. ; Romano, S. ; Spitaleri, C. ; Carlin, N. ; Cherubini, S. ; Del Gulino, M. ; Santo, M. G. ; Kroha, V. ; Kubono, S. ; La Cognata, M. ; Li, C. ; Pizzone, R. G. ; Qungang, W. ; Rapisarda, G. G. ; Sergi, M. L. ; Somorjai, E. ; Souza, F. ; Szanto De Tudisco, S. ; Toledo, A. ; Tumino, A. ; Wakabayashi, Y. ; Yamaguchi, H. / Improved results on extraction of 11B(p,α0) 8Be and 10B(p,α)7Be S(E)-factor through the Trojan Horse Method. AIP Conference Proceedings. Vol. 1269 2010. pp. 375-377
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abstract = "In this work the analysis of the 10B(p,α)7Be and 11B(p,α)8Be reactions, studied via the indirect Trojan Horse Method (THM), is discussed. In the astrophysical context of light nuclei LiBeB depletion, the above mentioned reactions are the main responsible for the destruction of boron in the stellar interior. The THM application allows their investigation in the astrophysically relevant energy region, around the Gamow Peak (≈10 keV), overcoming the problems due to the presence of the Coulomb barrier and electron screening effect. The experimental procedure and the preliminary results are shown.",
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AU - Puglia, S. M R

AU - Lamia, L.

AU - Romano, S.

AU - Spitaleri, C.

AU - Carlin, N.

AU - Cherubini, S.

AU - Del Gulino, M.

AU - Santo, M. G.

AU - Kroha, V.

AU - Kubono, S.

AU - La Cognata, M.

AU - Li, C.

AU - Pizzone, R. G.

AU - Qungang, W.

AU - Rapisarda, G. G.

AU - Sergi, M. L.

AU - Somorjai, E.

AU - Souza, F.

AU - Szanto De Tudisco, S.

AU - Toledo, A.

AU - Tumino, A.

AU - Wakabayashi, Y.

AU - Yamaguchi, H.

PY - 2010

Y1 - 2010

N2 - In this work the analysis of the 10B(p,α)7Be and 11B(p,α)8Be reactions, studied via the indirect Trojan Horse Method (THM), is discussed. In the astrophysical context of light nuclei LiBeB depletion, the above mentioned reactions are the main responsible for the destruction of boron in the stellar interior. The THM application allows their investigation in the astrophysically relevant energy region, around the Gamow Peak (≈10 keV), overcoming the problems due to the presence of the Coulomb barrier and electron screening effect. The experimental procedure and the preliminary results are shown.

AB - In this work the analysis of the 10B(p,α)7Be and 11B(p,α)8Be reactions, studied via the indirect Trojan Horse Method (THM), is discussed. In the astrophysical context of light nuclei LiBeB depletion, the above mentioned reactions are the main responsible for the destruction of boron in the stellar interior. The THM application allows their investigation in the astrophysically relevant energy region, around the Gamow Peak (≈10 keV), overcoming the problems due to the presence of the Coulomb barrier and electron screening effect. The experimental procedure and the preliminary results are shown.

KW - Abundances-Nuclear astrophysics

KW - S(E)-factor

KW - Stars

KW - Trojan Horse Method-Nuclear Astrophysics

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