Equation of State of Nuclear Matter, Neutron Rich Nuclei in Laboratories and Pasta Nuclei in Neutron Star Crusts(Proceedings of the YITP Workshop on Nuclear Matter under Extreme Conditions)

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Author(s)

    • IIDA Kei
    • The Institute of Physical and Chemical Research (RIKEN)

Abstract

Macroscopic properties of neutron rich nuclei in laboratories and nuclei in neutron star crusts are supposed to be dominated by the equation of state (EOS) of asymmetric nuclear matter. In this study, we attempt to identify the most important EOS parameter that governs these properties.

Journal

  • Progress of theoretical physics. Supplement   [List of Volumes]

    Progress of theoretical physics. Supplement (156), 137-138, 2004-12-28  [Table of Contents]

    The Physical Society of Japan (JPS)

References:  3

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Codes

  • NII Article ID (NAID)
    110001211802
  • NII NACSIS-CAT ID (NCID)
    AA00791466
  • Text Lang
    ENG
  • Article Type
    ART
  • ISSN
    03759687
  • Data Source
    CJP  NII-ELS 
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