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Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes.
Tran, D T; Ong, H J; Hagen, G; Morris, T D; Aoi, N; Suzuki, T; Kanada-En'yo, Y; Geng, L S; Terashima, S; Tanihata, I; Nguyen, T T; Ayyad, Y; Chan, P Y; Fukuda, M; Geissel, H; Harakeh, M N; Hashimoto, T; Hoang, T H; Ideguchi, E; Inoue, A; Jansen, G R; Kanungo, R; Kawabata, T; Khiem, L H; Lin, W P; Matsuta, K; Mihara, M; Momota, S; Nagae, D; Nguyen, N D; Nishimura, D; Otsuka, T; Ozawa, A; Ren, P P; Sakaguchi, H; Scheidenberger, C; Tanaka, J; Takechi, M; Wada, R; Yamamoto, T.
Affiliation
  • Tran DT; Research Center for Nuclear Physics, Osaka University, Osaka, 567-0047, Japan.
  • Ong HJ; Institute of Physics, Vietnam Academy of Science and Technology, Hanoi, 10000, Vietnam.
  • Hagen G; Research Center for Nuclear Physics, Osaka University, Osaka, 567-0047, Japan. onghjin@rcnp.osaka-u.ac.jp.
  • Morris TD; Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN, 37831, USA.
  • Aoi N; Department of Physics and Astronomy, University of Tennessee, Knoxville, TN, 37996, USA.
  • Suzuki T; Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN, 37831, USA.
  • Kanada-En'yo Y; Department of Physics and Astronomy, University of Tennessee, Knoxville, TN, 37996, USA.
  • Geng LS; Research Center for Nuclear Physics, Osaka University, Osaka, 567-0047, Japan.
  • Terashima S; Department of Physics, College of Humanities and Sciences, Nihon University, Tokyo, 156-8550, Japan.
  • Tanihata I; National Astronomical Observatory of Japan, Tokyo, 181-8588, Japan.
  • Nguyen TT; Department of Physics, Kyoto University, Kyoto, 606-8502, Japan.
  • Ayyad Y; School of Physics and Nuclear Energy Engineering, Beihang University, 100191, Beijing, China.
  • Chan PY; School of Physics and Nuclear Energy Engineering, Beihang University, 100191, Beijing, China.
  • Fukuda M; Research Center for Nuclear Physics, Osaka University, Osaka, 567-0047, Japan.
  • Geissel H; School of Physics and Nuclear Energy Engineering, Beihang University, 100191, Beijing, China.
  • Harakeh MN; Pham Ngoc Thach University of Medicine, Ho Chi Minh, 700000, Vietnam.
  • Hashimoto T; Faculty of Physics and Engineering, VNUHCM-University of Science, Ho Chi Minh City, 70250, Vietnam.
  • Hoang TH; Sungkyunkwan University, Gyeonggi-do, 16419, South Korea.
  • Ideguchi E; Research Center for Nuclear Physics, Osaka University, Osaka, 567-0047, Japan.
  • Inoue A; Research Center for Nuclear Physics, Osaka University, Osaka, 567-0047, Japan.
  • Jansen GR; Department of Physics, Osaka University, Osaka, 560-0043, Japan.
  • Kanungo R; GSI Helmholtzzentrum für Schwerionenforschung, 64291, Darmstadt, Germany.
  • Kawabata T; Justus Liebig University, 35392, Giessen, Germany.
  • Khiem LH; GSI Helmholtzzentrum für Schwerionenforschung, 64291, Darmstadt, Germany.
  • Lin WP; KVI Center for Advanced Radiation Technology, University of Groningen, 9747 AA, Groningen, The Netherlands.
  • Matsuta K; Rare Isotope Science Project, Institute for Basic Science, Daejeon, 34047, Korea.
  • Mihara M; Research Center for Nuclear Physics, Osaka University, Osaka, 567-0047, Japan.
  • Momota S; Institute of Physics, Vietnam Academy of Science and Technology, Hanoi, 10000, Vietnam.
  • Nagae D; Research Center for Nuclear Physics, Osaka University, Osaka, 567-0047, Japan.
  • Nguyen ND; Research Center for Nuclear Physics, Osaka University, Osaka, 567-0047, Japan.
  • Nishimura D; Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN, 37831, USA.
  • Otsuka T; National Center for Computational Sciences, Oak Ridge National Laboratory, Oak Ridge, TN, 37831, USA.
  • Ozawa A; Astronomy and Physics Department, Saint Mary's University, Halifax, NS, B3H 3C3, Canada.
  • Ren PP; Department of Physics, Kyoto University, Kyoto, 606-8502, Japan.
  • Sakaguchi H; Institute of Physics, Vietnam Academy of Science and Technology, Hanoi, 10000, Vietnam.
  • Scheidenberger C; Institute of Modern Physics, Chinese Academy of Sciences, 730000, Lanzhou, China.
  • Tanaka J; Department of Physics, Osaka University, Osaka, 560-0043, Japan.
  • Takechi M; Department of Physics, Osaka University, Osaka, 560-0043, Japan.
  • Wada R; Kochi University of Technology, Kochi, 782-8502, Japan.
  • Yamamoto T; RIKEN Nishina Center, Saitama, 351-0198, Japan.
Nat Commun ; 9(1): 1594, 2018 04 23.
Article in En | MEDLINE | ID: mdl-29686394
ABSTRACT
The nuclear shell structure, which originates in the nearly independent motion of nucleons in an average potential, provides an important guide for our understanding of nuclear structure and the underlying nuclear forces. Its most remarkable fingerprint is the existence of the so-called magic numbers of protons and neutrons associated with extra stability. Although the introduction of a phenomenological spin-orbit (SO) coupling force in 1949 helped in explaining the magic numbers, its origins are still open questions. Here, we present experimental evidence for the smallest SO-originated magic number (subshell closure) at the proton number six in 13-20C obtained from systematic analysis of point-proton distribution radii, electromagnetic transition rates and atomic masses of light nuclei. Performing ab initio calculations on 14,15C, we show that the observed proton distribution radii and subshell closure can be explained by the state-of-the-art nuclear theory with chiral nucleon-nucleon and three-nucleon forces, which are rooted in the quantum chromodynamics.

Full text: 1 Collection: 01-internacional Database: MEDLINE Type of study: Qualitative_research Language: En Journal: Nat Commun Year: 2018 Document type: Article

Full text: 1 Collection: 01-internacional Database: MEDLINE Type of study: Qualitative_research Language: En Journal: Nat Commun Year: 2018 Document type: Article