Direct Measurement of 
                        12
                        C + 
                        4
                        He Fusion Cross Section Near Stellar energy

K. Sagara; Kunihiro Fujita; Takashi Teranishi; M. Taniguchi; N. Oba; H. Yamaguchi; S. Matsuda

doi:10.1007/s00601-011-0218-9

Direct Measurement of ¹² C + ⁴ He Fusion Cross Section Near Stellar energy

K. Sagara, Kunihiro Fujita, Takashi Teranishi, M. Taniguchi, N. Oba, H. Yamaguchi, S. Matsuda

基礎粒子系物理学

研究成果: ジャーナルへの寄稿 › 学術誌 › 査読

抄録

The reaction ¹² C + ⁴ He → ¹⁶ O + γ at E _cm = 0.3 MeV plays an important role in stellar evolution, but the reaction cross section has not been measured yet. Recently we succeeded to measure total cross section of the reaction down to E _cm = 1.5 MeV at Kyushu University. We have a plan to measure the cross section down to 0.7 MeV in several years, and to extrapolate the results to 0.3 MeV.

本文言語	英語
ページ（範囲）	315-317
ページ数	3
ジャーナル	Few-Body Systems
巻	50
号	1-4
DOI	https://doi.org/10.1007/s00601-011-0218-9
出版ステータス	出版済み - 5月 1 2011

!!!All Science Journal Classification (ASJC) codes

原子分子物理学および光学

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10.1007/s00601-011-0218-9

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引用スタイル

Sagara, K., Fujita, K., Teranishi, T., Taniguchi, M., Oba, N., Yamaguchi, H., & Matsuda, S. (2011). Direct Measurement of ¹² C + ⁴ He Fusion Cross Section Near Stellar energy Few-Body Systems, 50(1-4), 315-317. https://doi.org/10.1007/s00601-011-0218-9

Direct Measurement of ¹² C + ⁴ He Fusion Cross Section Near Stellar energy . / Sagara, K.; Fujita, Kunihiro; Teranishi, Takashi その他.
In: Few-Body Systems, Vol. 50, No. 1-4, 01.05.2011, p. 315-317.

研究成果: ジャーナルへの寄稿 › 学術誌 › 査読

Sagara, K, Fujita, K, Teranishi, T, Taniguchi, M, Oba, N, Yamaguchi, H & Matsuda, S 2011, ' Direct Measurement of ¹² C + ⁴ He Fusion Cross Section Near Stellar energy ', Few-Body Systems, vol. 50, no. 1-4, pp. 315-317. https://doi.org/10.1007/s00601-011-0218-9

Sagara K, Fujita K, Teranishi T, Taniguchi M, Oba N, Yamaguchi H その他. Direct Measurement of ¹² C + ⁴ He Fusion Cross Section Near Stellar energy Few-Body Systems. 2011 5月 1;50(1-4):315-317. doi: 10.1007/s00601-011-0218-9

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abstract = " The reaction 12 C + 4 He → 16 O + γ at E cm = 0.3 MeV plays an important role in stellar evolution, but the reaction cross section has not been measured yet. Recently we succeeded to measure total cross section of the reaction down to E cm = 1.5 MeV at Kyushu University. We have a plan to measure the cross section down to 0.7 MeV in several years, and to extrapolate the results to 0.3 MeV.",

author = "K. Sagara and Kunihiro Fujita and Takashi Teranishi and M. Taniguchi and N. Oba and H. Yamaguchi and S. Matsuda",

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AU - Oba, N.

AU - Yamaguchi, H.

AU - Matsuda, S.

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AB - The reaction 12 C + 4 He → 16 O + γ at E cm = 0.3 MeV plays an important role in stellar evolution, but the reaction cross section has not been measured yet. Recently we succeeded to measure total cross section of the reaction down to E cm = 1.5 MeV at Kyushu University. We have a plan to measure the cross section down to 0.7 MeV in several years, and to extrapolate the results to 0.3 MeV.

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Direct Measurement of 12 C + 4 He Fusion Cross Section Near Stellar energy

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!!!All Science Journal Classification (ASJC) codes

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Direct Measurement of ¹² C + ⁴ He Fusion Cross Section Near Stellar energy