Weak isoscalar response of 11B

T. Kawabata; H. Akimune; H. Fujimura; H. Fujita; Y. Fujita; M. Fujiwara; K. Hara; K. Y. Hara; K. Hatanaka; T. Ishikawa; M. Itoh; J. Kamiya; M. Nakamura; H. Sakaguchi; Y. Shimbara; H. Takeda; A. Tamii; T. Noro; H. Toyokawa; M. Uchida; T. Wakasa; Y. Yasuda; H. P. Yoshida; M. Yosoi

doi:10.1134/1.1811180

Weak isoscalar response of ¹¹B

T. Kawabata, H. Akimune, H. Fujimura, H. Fujita, Y. Fujita, M. Fujiwara, K. Hara, K. Y. Hara, K. Hatanaka, T. Ishikawa, M. Itoh, J. Kamiya, M. Nakamura, H. Sakaguchi, Y. Shimbara, H. Takeda, A. Tamii, T. Noro, H. Toyokawa, M. UchidaT. Wakasa, Y. Yasuda, H. P. Yoshida, M. Yosoi

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

Weak-interaction responses of ¹¹B were studied by measuring the ¹¹B(³He, t) and ¹¹B(p, p′) reactions. Obtained nuclear transition matrix elements B(GT), B(στ), and B(σ) were compared with the shell-model calculations. The shell-model calculations, which explained the isovector parts B(GT) and B(στ) reasonably well if the quenching factors of 0.5-0.7 were taken into account, did not describe the isoscalar part B(σ).

本文言語	英語
ページ（範囲）	1974-1798
ページ数	177
ジャーナル	Physics of Atomic Nuclei
巻	67
号	10
DOI	https://doi.org/10.1134/1.1811180
出版ステータス	出版済み - 10月 2004

!!!All Science Journal Classification (ASJC) codes

原子分子物理学および光学
核物理学および高エネルギー物理学

文献へのアクセス

10.1134/1.1811180

他のファイルとリンク

引用スタイル

Kawabata, T., Akimune, H., Fujimura, H., Fujita, H., Fujita, Y., Fujiwara, M., Hara, K., Hara, K. Y., Hatanaka, K., Ishikawa, T., Itoh, M., Kamiya, J., Nakamura, M., Sakaguchi, H., Shimbara, Y., Takeda, H., Tamii, A., Noro, T., Toyokawa, H., ... Yosoi, M. (2004). Weak isoscalar response of ¹¹B. Physics of Atomic Nuclei, 67(10), 1974-1798. https://doi.org/10.1134/1.1811180

Kawabata, T, Akimune, H, Fujimura, H, Fujita, H, Fujita, Y, Fujiwara, M, Hara, K, Hara, KY, Hatanaka, K, Ishikawa, T, Itoh, M, Kamiya, J, Nakamura, M, Sakaguchi, H, Shimbara, Y, Takeda, H, Tamii, A, Noro, T, Toyokawa, H, Uchida, M, Wakasa, T, Yasuda, Y, Yoshida, HP & Yosoi, M 2004, 'Weak isoscalar response of ¹¹B', Physics of Atomic Nuclei, vol. 67, no. 10, pp. 1974-1798. https://doi.org/10.1134/1.1811180

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title = "Weak isoscalar response of 11B",

abstract = "Weak-interaction responses of 11B were studied by measuring the 11B(3He, t) and 11B(p, p′) reactions. Obtained nuclear transition matrix elements B(GT), B(στ), and B(σ) were compared with the shell-model calculations. The shell-model calculations, which explained the isovector parts B(GT) and B(στ) reasonably well if the quenching factors of 0.5-0.7 were taken into account, did not describe the isoscalar part B(σ).",

author = "T. Kawabata and H. Akimune and H. Fujimura and H. Fujita and Y. Fujita and M. Fujiwara and K. Hara and Hara, {K. Y.} and K. Hatanaka and T. Ishikawa and M. Itoh and J. Kamiya and M. Nakamura and H. Sakaguchi and Y. Shimbara and H. Takeda and A. Tamii and T. Noro and H. Toyokawa and M. Uchida and T. Wakasa and Y. Yasuda and Yoshida, {H. P.} and M. Yosoi",

year = "2004",

month = oct,

doi = "10.1134/1.1811180",

language = "English",

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T1 - Weak isoscalar response of 11B

AU - Kawabata, T.

AU - Akimune, H.

AU - Fujimura, H.

AU - Fujita, H.

AU - Fujita, Y.

AU - Fujiwara, M.

AU - Hara, K.

AU - Hara, K. Y.

AU - Hatanaka, K.

AU - Ishikawa, T.

AU - Itoh, M.

AU - Kamiya, J.

AU - Nakamura, M.

AU - Sakaguchi, H.

AU - Shimbara, Y.

AU - Takeda, H.

AU - Tamii, A.

AU - Noro, T.

AU - Toyokawa, H.

AU - Uchida, M.

AU - Wakasa, T.

AU - Yasuda, Y.

AU - Yoshida, H. P.

AU - Yosoi, M.

PY - 2004/10

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N2 - Weak-interaction responses of 11B were studied by measuring the 11B(3He, t) and 11B(p, p′) reactions. Obtained nuclear transition matrix elements B(GT), B(στ), and B(σ) were compared with the shell-model calculations. The shell-model calculations, which explained the isovector parts B(GT) and B(στ) reasonably well if the quenching factors of 0.5-0.7 were taken into account, did not describe the isoscalar part B(σ).

AB - Weak-interaction responses of 11B were studied by measuring the 11B(3He, t) and 11B(p, p′) reactions. Obtained nuclear transition matrix elements B(GT), B(στ), and B(σ) were compared with the shell-model calculations. The shell-model calculations, which explained the isovector parts B(GT) and B(στ) reasonably well if the quenching factors of 0.5-0.7 were taken into account, did not describe the isoscalar part B(σ).

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