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Evidence of halo structure in ^<37>Mg observed via reaction cross sections and intruder orbitals beyond the island of inversion
http://hdl.handle.net/10173/1504
http://hdl.handle.net/10173/150468e0866f-e59f-49cd-8702-3f5a821aa429
名前 / ファイル | ライセンス | アクション |
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28-31.pdf (422.7 kB)
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2017-03-24 | |||||
タイトル | ||||||
タイトル | Evidence of halo structure in ^<37>Mg observed via reaction cross sections and intruder orbitals beyond the island of inversion | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
著者 |
Takechi, M.
× Takechi, M.× Suzuki, S.× Nishimura, D.× Fukuda, M.× Ohtsubo, T.× Nagashima, M.× Suzuki, T.× Yamaguchi, T.× Ozawa, A.× Moriguchi, T.× Ohishi, H.× Sumikama, T.× Geissel, H.× Aoi, N.× Chen, Rui-Jiu× Fang, De-Qing× Fukuda, N.× Fukuoka, S.× Furuki, H.× Inabe, N.× Ishibashi, Y.× Itoh, T.× Izumikawa, T.× Kameda, D.× Kubo, T.× Lantz, M.× Lee, C. S.× Ma, Yu-Gang× Matsuta, K.× Mihara, M.× Momota, S.× Nagae, D.× Nishikiori, R.× Niwa, T.× Ohnishi, T.× Okumura, K.× Ohtake, M.× Ogura, T.× Sakurai, H.× Sato, K.× Shimbara, Y.× Suzuki, H.× Takeda, H.× Takeuchi, S.× Tanaka, K.× Tanaka, M.× Uenishi, H.× Winkler, M.× Yanagisawa, Y.× Watanabe, S.× Minomo, K.× Tagami, S.× Shimada, M.× Kimura, M.× Matsumoto, T.× Shimizu, Y. R.× Yahiro, M. |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | Precise reaction cross sections (σR) for ^<24−38>Mg on C targets at energies around 240 MeV/nucleon have been measured at the Radioactive Isotope Beam Factory at RIKEN. The σR for ^<36−38>Mg have been measured for the first time. An enhancement of σ_R compared to the systematics for spherical stable nuclei has been observed, especially in the neutron-rich region, which reflects the deformation of those isotopes. In the vicinity of the drip line the σ_R for ^<37>Mg is especially large. It is shown by analysis using a recently developed theoretical method that this prominent enhancement of σ_R for ^<37>Mg should come from the p-orbital halo formation breaking the N=28 shell gap. | |||||
書誌情報 |
Physical Review C 巻 90, 号 6, p. 061305-1-061305-5, 発行日 2014-12 |
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ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 2469-9985 | |||||
DOI | ||||||
関連タイプ | isIdenticalTo | |||||
識別子タイプ | DOI | |||||
関連識別子 | 10.1103/PhysRevC.90.061305 | |||||
権利 | ||||||
権利情報 | ©2014 American Physical Society | |||||
著者版フラグ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
出版者 | ||||||
出版者 | American Physical Society |