Variational Calculations for the Nuclear Equation of State toward Supernova Simulations

H. Kanzawa, K. Oyamatsu, K. Sumiyoshi, Masatoshi Takano

    研究成果: Conference contribution

    抄録

    We construct an equation of state (EOS) for uniform nuclear matter at zero and finite temperatures with the variational method starting from the realistic nuclear Hamiltonian composed of the AV18 two-body potential and the UIX three-body interaction. Using the obtained EOS, we perform the Thomas-Fermi calculation of atomic nuclei, and tune adjustable parameters in the EOS for uniform matter to reproduce empirical data of β-stable nuclei, toward a nuclear EOS table for supernova simulations.

    本文言語English
    ホスト出版物のタイトルOrigin of Matter and Evolution of Galaxies - 10th International Symposium on Origin of Matter and Evolution of Galaxies
    ホスト出版物のサブタイトルFrom the Dawn of Universe to the Formation of Solar System, OMEG 2007
    出版社American Institute of Physics Inc.
    ページ261-266
    ページ数6
    1016
    ISBN(電子版)9780735405370
    DOI
    出版ステータスPublished - 2008 1 1
    イベント10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System, OMEG 2007 - Sapporo, Japan
    継続期間: 2007 12 42007 12 7

    Other

    Other10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System, OMEG 2007
    CountryJapan
    CitySapporo
    Period07/12/407/12/7

    ASJC Scopus subject areas

    • Physics and Astronomy(all)

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