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Isospin dependence of kinetic energies in light neutron-rich nuclei

  • Section I: Nuclear Moments and Nuclear β-decays Studied by Polarization Phenomena
  • Published:
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Abstract

Energy spectra andelectric dipole transitions ofN=7 isotones are studied by shell model calculations with isospin dependent kinetic energies for s-d shell orbits. The ground states of10Li and9He are predicted. Electric dipole transitions in13C and11Be are studied by using the realistic single-particle wave functions in Woods-Saxon potential.

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References

  1. B.A. Brown, A. Etchegoyen andW.D.M. Rae, A shell model program OXBASH, MSU Cyclotron Laboratory Report No. 524 (1986).

  2. D.J. Millener, J.W. Olness, E.K. Warburton andS.S. Hanna, Phys. Rev. C 28 (1983) 497.

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Authors and Affiliations

  1. Research Center for Nuclear Physics, Osaka University, Mihogaoka 10-1, 567, Ibaraki, Osaka, Japan

    H. Kitagawa & H. Sagawa

  2. Department of Physics, Faculty of Science, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, 113, Tokyo, Japan

    H. Sagawa

Authors
  1. H. Kitagawa
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  2. H. Sagawa
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JSPS Fellow for Japanese Junior Scientists.

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Kitagawa, H., Sagawa, H. Isospin dependence of kinetic energies in light neutron-rich nuclei. Hyperfine Interact 78, 179–183 (1993). https://doi.org/10.1007/BF00568136

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  • DOI: https://doi.org/10.1007/BF00568136

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