Study of astrophysically important states in 26Si with the p(27Si,d)26Si* reaction and the p( 25Al,p)25Al elastic scattering

J. Chen, A. A. Chen, G. Amadio, D. Bazin, A. Becerril, A. M. Amthor, S. Cherubini, M. La Cognata, D. Galaviz, A. Gade, T. Glasmacher, H. Fujikawa, S. Hayakawa, N. Iwasa, J. J. He, D. Kahl, L. H. Khiem, S. Kubono, Y. Kurihawa, Y. K. KwonJ. LeNestour, G. Lorusso, M. Matos, J. Y. Moon, M. Niikura, S. Nishimura, A. Odahara, C. V. Ouellet, J. Pearson, J. Pereira, R. Pizzone, A. Saito, H. Schatz, A. Signoracci, C. Signorini, A. Smith, K. Smith, T. Teranishi, Y. Togano, B. Wales, Y. Wakabayashi, D. Weisshaar, H. Yamaguchi, R. Zegers

研究成果: Contribution to journalConference article査読


The radioisotope 26 Al is an important probe of the interstellar medium of our galaxy, but its production is now still not well determined partially due to the lack of knowledge of the important states in 26Si, which dominate the large uncertainty in the 25Al(p,γ)26Si reaction rate at nova temperatures. We give an update on two experiments that were performed to study these states. One is a measurement of the 27Si(p,d)26Si * reaction at the NSCL, and the other one is a measurement of the 25 Al+p elastic scattering with the CRIB facility at RIKEN.

ジャーナルProceedings of Science
出版ステータス出版済み - 2008
イベント10th Symposium on Nuclei in the Cosmos, NIC 2008 - Mackinac Island, MI, 米国
継続期間: 7 27 20088 1 2008

All Science Journal Classification (ASJC) codes

  • 一般


「Study of astrophysically important states in <sup>26</sup>Si with the p(<sup>27</sup>Si,d)<sup>26</sup>Si<sup>*</sup> reaction and the p( <sup>25</sup>Al,p)<sup>25</sup>Al elastic scattering」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。