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

J. Chen, A. A. Chen, H. Schatz, S. Kubono, A. B. Reyes, A. Smith, B. Wales, C. Ouellet, D. Kahl, D. G. Redondo, G. Lorusso, J. LeNestour, J. P. Conca, K. Smith, M. Amthor, M. Matos, H. Yamaguchi, N. Iwasa, S. Hayakawa, S. MichimasaT. Teranishi, Y. Kurihawa, Y. Wakabayashi

研究成果: ジャーナルへの寄稿記事

5 引用 (Scopus)

抄録

The astrophysically important states in 26Si have been studied with different reactions because of their dominant contribution to the 25Al(p,γ)26Si reaction rate at nova temperatures. We performed two different experiments to study the states of interest in 26Si, with the aim of reducing the main uncertainty in the current 25Al(p,γ)26Si rate by determining the level parameters of the dominant states more accurately. One is the p(27Si,26Si*)d experiment at NSCL, in which we measured the gamma-ray decays from the excited states in 26Si. The other one is the 25Al+p elastic scattering experiment with CRIB at RIKEN.

元の言語英語
ページ(範囲)667c-669c
ジャーナルNuclear Physics A
834
発行部数1-4
DOI
出版物ステータス出版済み - 3 1 2010

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elastic scattering
reaction kinetics
gamma rays
decay
excitation
temperature

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics

これを引用

Chen, J., Chen, A. A., Schatz, H., Kubono, S., Reyes, A. B., Smith, A., ... Wakabayashi, Y. (2010). Study of astrophysically important states in 26Si with the p(27Si,26Si*)d reaction and the p(25Al,p)25Al elastic scattering. Nuclear Physics A, 834(1-4), 667c-669c. https://doi.org/10.1016/j.nuclphysa.2010.01.119

Study of astrophysically important states in 26Si with the p(27Si,26Si*)d reaction and the p(25Al,p)25Al elastic scattering. / Chen, J.; Chen, A. A.; Schatz, H.; Kubono, S.; Reyes, A. B.; Smith, A.; Wales, B.; Ouellet, C.; Kahl, D.; Redondo, D. G.; Lorusso, G.; LeNestour, J.; Conca, J. P.; Smith, K.; Amthor, M.; Matos, M.; Yamaguchi, H.; Iwasa, N.; Hayakawa, S.; Michimasa, S.; Teranishi, T.; Kurihawa, Y.; Wakabayashi, Y.

:: Nuclear Physics A, 巻 834, 番号 1-4, 01.03.2010, p. 667c-669c.

研究成果: ジャーナルへの寄稿記事

Chen, J, Chen, AA, Schatz, H, Kubono, S, Reyes, AB, Smith, A, Wales, B, Ouellet, C, Kahl, D, Redondo, DG, Lorusso, G, LeNestour, J, Conca, JP, Smith, K, Amthor, M, Matos, M, Yamaguchi, H, Iwasa, N, Hayakawa, S, Michimasa, S, Teranishi, T, Kurihawa, Y & Wakabayashi, Y 2010, 'Study of astrophysically important states in 26Si with the p(27Si,26Si*)d reaction and the p(25Al,p)25Al elastic scattering', Nuclear Physics A, 巻. 834, 番号 1-4, pp. 667c-669c. https://doi.org/10.1016/j.nuclphysa.2010.01.119
Chen, J. ; Chen, A. A. ; Schatz, H. ; Kubono, S. ; Reyes, A. B. ; Smith, A. ; Wales, B. ; Ouellet, C. ; Kahl, D. ; Redondo, D. G. ; Lorusso, G. ; LeNestour, J. ; Conca, J. P. ; Smith, K. ; Amthor, M. ; Matos, M. ; Yamaguchi, H. ; Iwasa, N. ; Hayakawa, S. ; Michimasa, S. ; Teranishi, T. ; Kurihawa, Y. ; Wakabayashi, Y. / Study of astrophysically important states in 26Si with the p(27Si,26Si*)d reaction and the p(25Al,p)25Al elastic scattering. :: Nuclear Physics A. 2010 ; 巻 834, 番号 1-4. pp. 667c-669c.
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abstract = "The astrophysically important states in 26Si have been studied with different reactions because of their dominant contribution to the 25Al(p,γ)26Si reaction rate at nova temperatures. We performed two different experiments to study the states of interest in 26Si, with the aim of reducing the main uncertainty in the current 25Al(p,γ)26Si rate by determining the level parameters of the dominant states more accurately. One is the p(27Si,26Si*)d experiment at NSCL, in which we measured the gamma-ray decays from the excited states in 26Si. The other one is the 25Al+p elastic scattering experiment with CRIB at RIKEN.",
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AU - Chen, J.

AU - Chen, A. A.

AU - Schatz, H.

AU - Kubono, S.

AU - Reyes, A. B.

AU - Smith, A.

AU - Wales, B.

AU - Ouellet, C.

AU - Kahl, D.

AU - Redondo, D. G.

AU - Lorusso, G.

AU - LeNestour, J.

AU - Conca, J. P.

AU - Smith, K.

AU - Amthor, M.

AU - Matos, M.

AU - Yamaguchi, H.

AU - Iwasa, N.

AU - Hayakawa, S.

AU - Michimasa, S.

AU - Teranishi, T.

AU - Kurihawa, Y.

AU - Wakabayashi, Y.

PY - 2010/3/1

Y1 - 2010/3/1

N2 - The astrophysically important states in 26Si have been studied with different reactions because of their dominant contribution to the 25Al(p,γ)26Si reaction rate at nova temperatures. We performed two different experiments to study the states of interest in 26Si, with the aim of reducing the main uncertainty in the current 25Al(p,γ)26Si rate by determining the level parameters of the dominant states more accurately. One is the p(27Si,26Si*)d experiment at NSCL, in which we measured the gamma-ray decays from the excited states in 26Si. The other one is the 25Al+p elastic scattering experiment with CRIB at RIKEN.

AB - The astrophysically important states in 26Si have been studied with different reactions because of their dominant contribution to the 25Al(p,γ)26Si reaction rate at nova temperatures. We performed two different experiments to study the states of interest in 26Si, with the aim of reducing the main uncertainty in the current 25Al(p,γ)26Si rate by determining the level parameters of the dominant states more accurately. One is the p(27Si,26Si*)d experiment at NSCL, in which we measured the gamma-ray decays from the excited states in 26Si. The other one is the 25Al+p elastic scattering experiment with CRIB at RIKEN.

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