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Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes

Author

Listed:
  • D. T. Tran

    (Osaka University
    Vietnam Academy of Science and Technology)

  • H. J. Ong

    (Osaka University)

  • G. Hagen

    (Oak Ridge National Laboratory
    University of Tennessee)

  • T. D. Morris

    (Oak Ridge National Laboratory
    University of Tennessee)

  • N. Aoi

    (Osaka University)

  • T. Suzuki

    (Nihon University
    National Astronomical Observatory of Japan)

  • Y. Kanada-En’yo

    (Kyoto University)

  • L. S. Geng

    (Beihang University)

  • S. Terashima

    (Beihang University)

  • I. Tanihata

    (Osaka University
    Beihang University)

  • T. T. Nguyen

    (Pham Ngoc Thach University of Medicine
    VNUHCM-University of Science
    Sungkyunkwan University)

  • Y. Ayyad

    (Osaka University)

  • P. Y. Chan

    (Osaka University)

  • M. Fukuda

    (Osaka University)

  • H. Geissel

    (GSI Helmholtzzentrum für Schwerionenforschung
    Justus Liebig University)

  • M. N. Harakeh

    (GSI Helmholtzzentrum für Schwerionenforschung
    University of Groningen)

  • T. Hashimoto

    (Institute for Basic Science)

  • T. H. Hoang

    (Osaka University
    Vietnam Academy of Science and Technology)

  • E. Ideguchi

    (Osaka University)

  • A. Inoue

    (Osaka University)

  • G. R. Jansen

    (Oak Ridge National Laboratory
    Oak Ridge National Laboratory)

  • R. Kanungo

    (Saint Mary’s University)

  • T. Kawabata

    (Kyoto University)

  • L. H. Khiem

    (Vietnam Academy of Science and Technology)

  • W. P. Lin

    (Chinese Academy of Sciences)

  • K. Matsuta

    (Osaka University)

  • M. Mihara

    (Osaka University)

  • S. Momota

    (Kochi University of Technology)

  • D. Nagae

    (RIKEN Nishina Center)

  • N. D. Nguyen

    (Dong Nai University)

  • D. Nishimura

    (Tokyo University of Science)

  • T. Otsuka

    (University of Tokyo)

  • A. Ozawa

    (University of Tsukuba)

  • P. P. Ren

    (Chinese Academy of Sciences)

  • H. Sakaguchi

    (Osaka University)

  • C. Scheidenberger

    (GSI Helmholtzzentrum für Schwerionenforschung
    Justus Liebig University)

  • J. Tanaka

    (Osaka University)

  • M. Takechi

    (Niigata University)

  • R. Wada

    (Chinese Academy of Sciences
    Texas A&M University)

  • T. Yamamoto

    (Osaka University)

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.

Suggested Citation

  • D. T. Tran & H. J. Ong & G. Hagen & T. D. Morris & N. Aoi & T. Suzuki & Y. Kanada-En’yo & L. S. Geng & S. Terashima & I. Tanihata & T. T. Nguyen & Y. Ayyad & P. Y. Chan & M. Fukuda & H. Geissel & M. N, 2018. "Evidence for prevalent Z = 6 magic number in neutron-rich carbon isotopes," Nature Communications, Nature, vol. 9(1), pages 1-7, December.
  • Handle: RePEc:nat:natcom:v:9:y:2018:i:1:d:10.1038_s41467-018-04024-y
    DOI: 10.1038/s41467-018-04024-y
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