Accès ouvert déclaré
2021
article
ノックアウト反応で明らかにするボロミアン核17Bの小さいs軌道成分
Z. H. Yang, Yuki Kubota, A. Corsi, Kazuki Yoshida, X-X. Sun, J. G. Li, Masaaki KIMURA, N. Michel, Kazuyuki Ogata, C. X. Yuan, Q. Yuan, G. Authelet, H. Baba, C. Caesar, D. Calvet, A. Delbart, Masanori Dozono, J. Feng, F. Flavigny, J.-M. Gheller, J. Gibelin, A. Giganon, A. Gillibert, K. Hasegawa, Tadaaki Isobe, Yoshihiro KANAYA, Shunsuke Kawakami, D. W. Kim, Y. Kiyokawa, Motoki Kobayashi, N. Kobayashi, T. Kobayashi, Y. Kondo, Z. Korkulu, Shumpei KOYAMA, V. Lapoux, Yukie Maeda, F. M. Marqu\'es, Toru Motobayashi, T. Miyazaki, Takashi Nakamura, N. Nakatsuka, Y. Nishio, A. Obertelli, Ayaka Okura, N. A. Orr, Shinsuke Ota, H. Otsu, T. Ozaki, V. Panin, S. Paschalis, E. C. Pollacco, S. Reichert, J.-Y. Rouss\'e, Atsumi Saito, Satoshi Sakaguchi, M. Sako, C. Santamaria, M. Sasano, H. Sato, M. Shikata, Y. Shimizu, Yusuke Shindo, L. Stuhl, T. Sumikama, Y. Y. Sun, M. Tabata, Yasuhiro Togano, Junichi Tsubota, F. R. Xu, Jumpei Yasuda, Kenichiro YONEDA, Juzo Zenihiro, S.-G. Zhou, W. Zuo, Tomohiro Uesaka
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32Institutions déclarées
7Pays d’affiliation déclarés
Rattachement africain : jp, fr, cn, de, kr, hu, us.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
A quasifree ($p$,$pn$) experiment was performed to study the structure of the Borromean nucleus $^{17}$B, which had long been considered to have a neutron halo. By analyzing the momentum distributions and exclusive cross sections, we obtained the spectroscopic factors for $1s_{1/2}$ and $0d_{5/2}$ orbitals, and a surprisingly small percentage of 9(2)\% was determined for $1s_{1/2}$. Our finding of such a small $1s_{1/2}$ component and the halo features reported in prior experiments can be explained by the deformed relativistic Hartree-Bogoliubov theory in continuum, revealing a definite but not dominant neutron halo in $^{17}$B. The present work gives the smallest $s$- or $p$-orbital component among known nuclei exhibiting halo features and implies that the dominant occupation of $s$ or $p$ orbitals is not a prerequisite for the occurrence of a neutron halo.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Le contrôle bibliographique ouvert
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Les sujets associés
Nuclear physics research studiesQuantum Chromodynamics and Particle InteractionsRare-earth and actinide compounds