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)

Search this Article

Author(s)

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 = Progress of theoretical physics. Supplement

    Progress of theoretical physics. Supplement = Progress of theoretical physics. Supplement 156, 137-138, 2004-12-28

References:  3

  • <no title>

    OYAMATSU K.

    Nucl. Phys. A 561, 431, 1993

    DOI Cited by (6)

  • <no title>

    PETHICK C. J.

    Nucl. Phys. A 584, 675, 1995

    DOI Cited by (2)

  • Saturation of Nuclear Matter and Radii of Unstable Nuclei

    Kazuhiro OYAMATSU , Kei IIDA , Department of Media Production and Theories Aichi Shukutoku University : The Institute of Physical and Chemical Research (RIKEN) , The Institute of Physical and Chemical Research (RIKEN)

    Progress of theoretical physics = Progress of theoretical physics 109(4), 631-650, 2003-04-25

    CiNii Fulltext Link IR DOI References (39) Cited by (6)

Codes

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