Systematic Measurement of pd Breakup Cross Section Around Space Star

K. Ohnaka, K. Sagara, Y. Maeda, K. Ishibashi, S. Kimura, S. Tanaka, T. Fukunaga, J. Yasuda, T. Yabe, K. Yashima, Y. Eguchi, H. Shimoda, T. Sueta, S. Kuroita

研究成果: ジャーナルへの寄稿学術誌査読

3 被引用数 (Scopus)

抄録

Space Star (SS) anomaly in nd breakup cross section was first reported in 1989 at En = 13 MeV (Strate et al. in Nucl Phys A 501:51, 1989), but its origin has not been found yet. In order to obtain suggestions for its origin, we made systematic measurements of pd breakup cross section around SS. In SS configuration, three outgoing nucleons form an equilateral triangle and the triangle is perpendicular to the beam axis. Necessity of the equilateral and perpendicular conditions of SS anomaly was investigated by systematic experiments. Also energy dependence of SS anomaly is being studied at energies from Ep = 7.5 to 13 MeV.

本文言語英語
ページ(範囲)725-728
ページ数4
ジャーナルFew-Body Systems
55
8-10
DOI
出版ステータス出版済み - 8月 2014

!!!All Science Journal Classification (ASJC) codes

  • 原子分子物理学および光学

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