### 抜粋

We construct a new nuclear equation of state (EOS) for core-collapse supernova (SN) simulations using the variational many-body theory. For uniform nuclear matter, the EOS is constructed with the cluster variational method starting from the realistic nuclear Hamiltonian composed of the Argonne v18 two-body potential and the Urbana IX three-body potential. The masses and radii of neutron stars calculated with the obtained EOS at zero temperature are consistent with recent observational data. For non-uniform nuclear matter, we construct the EOS in the Thomas-Fermi approximation. In this approximation, we assume a functional form of the density distributions of protons, neutrons, and alpha-particles, and minimize the free energy density in a Wigner-Seitz cell with respect to the parameters included in the assumed density distribution functions. The phase diagram of hot nuclear matter at a typical temperature is reasonable as compared with that of the Shen EOS.

元の言語 | 英語 |
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記事番号 | 012058 |

ジャーナル | Journal of Physics: Conference Series |

巻 | 569 |

発行部数 | 1 |

DOI | |

出版物ステータス | 出版済み - 1 1 2014 |

イベント | 3rd International Workshop on State of the Art in Nuclear Cluster Physics, SOTANCP 2014 - Yokohama, 日本 継続期間: 5 26 2014 → 5 30 2014 |

### All Science Journal Classification (ASJC) codes

- Physics and Astronomy(all)

## フィンガープリント Equation of state for nuclear matter in core-collapse supernovae by the variational method' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。

## これを引用

*Journal of Physics: Conference Series*,

*569*(1), [012058]. https://doi.org/10.1088/1742-6596/569/1/012058