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Study of neutron-rich nuclei with an m -scheme cluster-orbital shell model approach

  • Regular Article - Theoretical Physics
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Abstract

We propose an m -scheme approach of the cluster-orbital shell model (COSM) formalism. In order to take into account the contribution of the unbound states, the radial wave function is treated as the super position of the Gaussian functions with different width parameters. We apply the m -scheme COSM to oxygen isotopes. Energies and r.m.s. radii of oxygen isotopes are studied.

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Authors and Affiliations

  1. Information Processing Center, Kitami Institute of Technology, 090-8507, Kitami, Japan

    H. Masui

  2. Department of Physics, Faculty of Science, Hokkaido University, 060-0810, Sapporo, Japan

    K. Katō

  3. The Institute of Physical, Chemical Research (RIKEN), 351-0198, Wako, Japan

    K. Ikeda

Authors
  1. H. Masui
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  2. K. Katō
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  3. K. Ikeda
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Corresponding author

Correspondence to H. Masui.

Additional information

Communicated by W. Nazarewicz

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Masui, H., Katō, K. & Ikeda, K. Study of neutron-rich nuclei with an m -scheme cluster-orbital shell model approach. Eur. Phys. J. A 42, 535–540 (2009). https://doi.org/10.1140/epja/i2009-10839-9

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  • DOI: https://doi.org/10.1140/epja/i2009-10839-9

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