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

Experimental Particle Physics

Research output: Contribution to journal › Article › peer-review

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.

Original language	English
Pages (from-to)	315-317
Number of pages	3
Journal	Few-Body Systems
Volume	50
Issue number	1-4
DOIs	https://doi.org/10.1007/s00601-011-0218-9
Publication status	Published - May 1 2011

All Science Journal Classification (ASJC) codes

Atomic and Molecular Physics, and Optics

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10.1007/s00601-011-0218-9

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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 et al.

In: Few-Body Systems, Vol. 50, No. 1-4, 01.05.2011, p. 315-317.

Research output: Contribution to journal › Article › peer-review

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

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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

Abstract

All Science Journal Classification (ASJC) codes

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