Determination of the astrophysical S factor of the 8B(p, γ)9C capture reaction from the d(8B, 9C)n reaction

D. Beaumel; T. Kubo; T. Teranishi; H. Sakurai; S. Fortier; A. Mengoni; N. Aoi; N. Fukuda; M. Hirai; N. Imai; H. Iwasaki; H. Kumagai; H. Laurent; S. M. Lukyanov; J. M. Maison; T. Motobayashi; T. Nakamura; H. Ohnuma; S. Pita; K. Yoneda; M. Ishihara

doi:10.1016/S0370-2693(01)00828-0

Determination of the astrophysical S factor of the ⁸B(p, γ)⁹C capture reaction from the d(⁸B, ⁹C)n reaction

D. Beaumel, T. Kubo, T. Teranishi, H. Sakurai, S. Fortier, A. Mengoni, N. Aoi, N. Fukuda, M. Hirai, N. Imai, H. Iwasaki, H. Kumagai, H. Laurent, S. M. Lukyanov, J. M. Maison, T. Motobayashi, T. Nakamura, H. Ohnuma, S. Pita, K. YonedaM. Ishihara

研究成果: ジャーナルへの寄稿 › 学術誌 › 査読

42 被引用数 (Scopus)

抄録

The asymptotic normalization coefficients for the virtual decay ⁹C → ⁸B + p have been determined by measuring the cross-section of the ⁸B(d, n)⁹C reaction in inverse kinematics at 14.4 MeV/u, using the RIPS facility. The deduced astrophysical S factor S₁₈ of the ⁸B(p, γ)⁹C capture reaction in the center of mass energy range 1-100 keV is S₁₈ = 45 ± 13 eV b.

本文言語	英語
ページ（範囲）	226-232
ページ数	7
ジャーナル	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
巻	514
号	3-4
DOI	https://doi.org/10.1016/S0370-2693(01)00828-0
出版ステータス	出版済み - 8月 16 2001
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/S0370-2693(01)00828-0

他のファイルとリンク

引用スタイル

Beaumel, D., Kubo, T., Teranishi, T., Sakurai, H., Fortier, S., Mengoni, A., Aoi, N., Fukuda, N., Hirai, M., Imai, N., Iwasaki, H., Kumagai, H., Laurent, H., Lukyanov, S. M., Maison, J. M., Motobayashi, T., Nakamura, T., Ohnuma, H., Pita, S., ... Ishihara, M. (2001). Determination of the astrophysical S factor of the ⁸B(p, γ)⁹C capture reaction from the d(⁸B, ⁹C)n reaction. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 514(3-4), 226-232. https://doi.org/10.1016/S0370-2693(01)00828-0

Beaumel, D, Kubo, T, Teranishi, T, Sakurai, H, Fortier, S, Mengoni, A, Aoi, N, Fukuda, N, Hirai, M, Imai, N, Iwasaki, H, Kumagai, H, Laurent, H, Lukyanov, SM, Maison, JM, Motobayashi, T, Nakamura, T, Ohnuma, H, Pita, S, Yoneda, K & Ishihara, M 2001, 'Determination of the astrophysical S factor of the ⁸B(p, γ)⁹C capture reaction from the d(⁸B, ⁹C)n reaction', Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, vol. 514, no. 3-4, pp. 226-232. https://doi.org/10.1016/S0370-2693(01)00828-0

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title = "Determination of the astrophysical S factor of the 8B(p, γ)9C capture reaction from the d(8B, 9C)n reaction",

abstract = "The asymptotic normalization coefficients for the virtual decay 9C → 8B + p have been determined by measuring the cross-section of the 8B(d, n)9C reaction in inverse kinematics at 14.4 MeV/u, using the RIPS facility. The deduced astrophysical S factor S18 of the 8B(p, γ)9C capture reaction in the center of mass energy range 1-100 keV is S18 = 45 ± 13 eV b.",

author = "D. Beaumel and T. Kubo and T. Teranishi and H. Sakurai and S. Fortier and A. Mengoni and N. Aoi and N. Fukuda and M. Hirai and N. Imai and H. Iwasaki and H. Kumagai and H. Laurent and Lukyanov, {S. M.} and Maison, {J. M.} and T. Motobayashi and T. Nakamura and H. Ohnuma and S. Pita and K. Yoneda and M. Ishihara",

note = "Funding Information: We wish to thank the RIKEN RARF and Orsay tandem accelerator staffs. We acknowledge Dr. N. Smirnova for shell-model calculations, and Dr. Y. Blumenfeld, Dr. S. Gal{\`e}s and Dr. J.P. Thibaud for careful reading of the manuscript. Part of this work was achieved within the IN2P3-RIKEN agreements and supported by the Science and Technology Agency of the Japanese government. ",

year = "2001",

month = aug,

day = "16",

doi = "10.1016/S0370-2693(01)00828-0",

language = "English",

volume = "514",

pages = "226--232",

journal = "Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics",

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T1 - Determination of the astrophysical S factor of the 8B(p, γ)9C capture reaction from the d(8B, 9C)n reaction

AU - Beaumel, D.

AU - Kubo, T.

AU - Teranishi, T.

AU - Sakurai, H.

AU - Fortier, S.

AU - Mengoni, A.

AU - Aoi, N.

AU - Fukuda, N.

AU - Hirai, M.

AU - Imai, N.

AU - Iwasaki, H.

AU - Kumagai, H.

AU - Laurent, H.

AU - Lukyanov, S. M.

AU - Maison, J. M.

AU - Motobayashi, T.

AU - Nakamura, T.

AU - Ohnuma, H.

AU - Pita, S.

AU - Yoneda, K.

AU - Ishihara, M.

N1 - Funding Information: We wish to thank the RIKEN RARF and Orsay tandem accelerator staffs. We acknowledge Dr. N. Smirnova for shell-model calculations, and Dr. Y. Blumenfeld, Dr. S. Galès and Dr. J.P. Thibaud for careful reading of the manuscript. Part of this work was achieved within the IN2P3-RIKEN agreements and supported by the Science and Technology Agency of the Japanese government.

PY - 2001/8/16

Y1 - 2001/8/16

N2 - The asymptotic normalization coefficients for the virtual decay 9C → 8B + p have been determined by measuring the cross-section of the 8B(d, n)9C reaction in inverse kinematics at 14.4 MeV/u, using the RIPS facility. The deduced astrophysical S factor S18 of the 8B(p, γ)9C capture reaction in the center of mass energy range 1-100 keV is S18 = 45 ± 13 eV b.

AB - The asymptotic normalization coefficients for the virtual decay 9C → 8B + p have been determined by measuring the cross-section of the 8B(d, n)9C reaction in inverse kinematics at 14.4 MeV/u, using the RIPS facility. The deduced astrophysical S factor S18 of the 8B(p, γ)9C capture reaction in the center of mass energy range 1-100 keV is S18 = 45 ± 13 eV b.

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VL - 514

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EP - 232

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

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