Direct measurement of the astrophysical reaction 14O(α,p)17F

M. Notani; S. Kubono; T. Teranishi; Y. Yanagisawa; S. Michimasa; K. Ue; J. J. He; H. Iwasaki; H. Baba; M. Tamaki; T. Minemura; S. Shimoura; N. Hokoiwa; Y. Wakabayashi; T. Sasaki; T. Fukuchi; A. Odahara; Y. Gono; Zs Fülöp; E. K. Lee; K. I. Hahn; J. Y. Moon; C. C. Yun; J. H. Lee; C. S. Lee; S. Kato

doi:10.1016/j.nuclphysa.2004.04.076

Direct measurement of the astrophysical reaction ¹⁴O(α,p)¹⁷F

M. Notani, S. Kubono, T. Teranishi, Y. Yanagisawa, S. Michimasa, K. Ue, J. J. He, H. Iwasaki, H. Baba, M. Tamaki, T. Minemura, S. Shimoura, N. Hokoiwa, Y. Wakabayashi, T. Sasaki, T. Fukuchi, A. Odahara, Y. Gono, Zs Fülöp, E. K. LeeK. I. Hahn, J. Y. Moon, C. C. Yun, J. H. Lee, C. S. Lee, S. Kato

研究成果: ジャーナルへの寄稿 › 学術誌 › 査読

9 被引用数 (Scopus)

抄録

The stellar reaction ¹⁴O(α,p)¹⁷F, that critically determines the onset of the hightemperature rp-process, has been studied through a direct measurement with a low-energy radioactive ¹⁴O beam and a gaseous helium target cooled down to 30 K. The reaction cross section was measured directly by means of a thick target technique in the energy range of E_c.m(^l4O+α) = 0.8-3.8 MeV. The ¹⁴O(α,p)¹⁷F* reaction leading to the first excited state in ¹⁷F was clearly observed for the first time, suggesting an increase of about 50% for the stellar reaction rate through resonances at around 7.1 MeV in 18Ne.

本文言語	英語
ページ（範囲）	411-415
ページ数	5
ジャーナル	Nuclear Physics A
巻	738
号	1-4 SUPPL.
DOI	https://doi.org/10.1016/j.nuclphysa.2004.04.076
出版ステータス	出版済み - 6月 28 2004
外部発表	はい

!!!All Science Journal Classification (ASJC) codes

核物理学および高エネルギー物理学

文献へのアクセス

10.1016/j.nuclphysa.2004.04.076

他のファイルとリンク

引用スタイル

Notani, M., Kubono, S., Teranishi, T., Yanagisawa, Y., Michimasa, S., Ue, K., He, J. J., Iwasaki, H., Baba, H., Tamaki, M., Minemura, T., Shimoura, S., Hokoiwa, N., Wakabayashi, Y., Sasaki, T., Fukuchi, T., Odahara, A., Gono, Y., Fülöp, Z., ... Kato, S. (2004). Direct measurement of the astrophysical reaction ¹⁴O(α,p)¹⁷F. Nuclear Physics A, 738(1-4 SUPPL.), 411-415. https://doi.org/10.1016/j.nuclphysa.2004.04.076

Notani, M, Kubono, S, Teranishi, T, Yanagisawa, Y, Michimasa, S, Ue, K, He, JJ, Iwasaki, H, Baba, H, Tamaki, M, Minemura, T, Shimoura, S, Hokoiwa, N, Wakabayashi, Y, Sasaki, T, Fukuchi, T, Odahara, A, Gono, Y, Fülöp, Z, Lee, EK, Hahn, KI, Moon, JY, Yun, CC, Lee, JH, Lee, CS & Kato, S 2004, 'Direct measurement of the astrophysical reaction ¹⁴O(α,p)¹⁷F', Nuclear Physics A, vol. 738, no. 1-4 SUPPL., pp. 411-415. https://doi.org/10.1016/j.nuclphysa.2004.04.076

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title = "Direct measurement of the astrophysical reaction 14O(α,p)17F",

abstract = "The stellar reaction 14O(α,p)17F, that critically determines the onset of the hightemperature rp-process, has been studied through a direct measurement with a low-energy radioactive 14O beam and a gaseous helium target cooled down to 30 K. The reaction cross section was measured directly by means of a thick target technique in the energy range of Ec.m(l4O+α) = 0.8-3.8 MeV. The 14O(α,p)17F* reaction leading to the first excited state in 17F was clearly observed for the first time, suggesting an increase of about 50% for the stellar reaction rate through resonances at around 7.1 MeV in 18Ne.",

author = "M. Notani and S. Kubono and T. Teranishi and Y. Yanagisawa and S. Michimasa and K. Ue and He, {J. J.} and H. Iwasaki and H. Baba and M. Tamaki and T. Minemura and S. Shimoura and N. Hokoiwa and Y. Wakabayashi and T. Sasaki and T. Fukuchi and A. Odahara and Y. Gono and Zs F{\"u}l{\"o}p and Lee, {E. K.} and Hahn, {K. I.} and Moon, {J. Y.} and Yun, {C. C.} and Lee, {J. H.} and Lee, {C. S.} and S. Kato",

year = "2004",

month = jun,

day = "28",

doi = "10.1016/j.nuclphysa.2004.04.076",

language = "English",

volume = "738",

pages = "411--415",

journal = "Nuclear Physics A",

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publisher = "Elsevier",

number = "1-4 SUPPL.",

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TY - JOUR

T1 - Direct measurement of the astrophysical reaction 14O(α,p)17F

AU - Notani, M.

AU - Kubono, S.

AU - Teranishi, T.

AU - Yanagisawa, Y.

AU - Michimasa, S.

AU - Ue, K.

AU - He, J. J.

AU - Iwasaki, H.

AU - Baba, H.

AU - Tamaki, M.

AU - Minemura, T.

AU - Shimoura, S.

AU - Hokoiwa, N.

AU - Wakabayashi, Y.

AU - Sasaki, T.

AU - Fukuchi, T.

AU - Odahara, A.

AU - Gono, Y.

AU - Fülöp, Zs

AU - Lee, E. K.

AU - Hahn, K. I.

AU - Moon, J. Y.

AU - Yun, C. C.

AU - Lee, J. H.

AU - Lee, C. S.

AU - Kato, S.

PY - 2004/6/28

Y1 - 2004/6/28

N2 - The stellar reaction 14O(α,p)17F, that critically determines the onset of the hightemperature rp-process, has been studied through a direct measurement with a low-energy radioactive 14O beam and a gaseous helium target cooled down to 30 K. The reaction cross section was measured directly by means of a thick target technique in the energy range of Ec.m(l4O+α) = 0.8-3.8 MeV. The 14O(α,p)17F* reaction leading to the first excited state in 17F was clearly observed for the first time, suggesting an increase of about 50% for the stellar reaction rate through resonances at around 7.1 MeV in 18Ne.

AB - The stellar reaction 14O(α,p)17F, that critically determines the onset of the hightemperature rp-process, has been studied through a direct measurement with a low-energy radioactive 14O beam and a gaseous helium target cooled down to 30 K. The reaction cross section was measured directly by means of a thick target technique in the energy range of Ec.m(l4O+α) = 0.8-3.8 MeV. The 14O(α,p)17F* reaction leading to the first excited state in 17F was clearly observed for the first time, suggesting an increase of about 50% for the stellar reaction rate through resonances at around 7.1 MeV in 18Ne.

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U2 - 10.1016/j.nuclphysa.2004.04.076

DO - 10.1016/j.nuclphysa.2004.04.076

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SN - 0375-9474

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EP - 415

JO - Nuclear Physics A

JF - Nuclear Physics A

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