Cluster variational method for nuclear matter with the three-body force

M. Takano*, H. Togashi, S. Yamamuro, K. Nakazato, H. Suzuki

*この研究の対応する著者

研究成果: Conference contribution

1 被引用数 (Scopus)

抄録

We report the current status of our project to construct a new nuclear equation of state (EOS), which may be used for supernova numerical simulations, based on the cluster variational method starting from the realistic nuclear Hamiltonian. We also take into account a higher-order correction to the energy of the nuclear three-body force (TBF). The nuclear EOSs with and without the higher-order TBF correction at zero temperature are very close to each other, when parameters are readjusted so as to reproduce the empirical saturation data.

本文言語English
ホスト出版物のタイトルOrigin of Matter and Evolution of Galaxies 2011
ページ378-380
ページ数3
DOI
出版ステータスPublished - 2012
イベントInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan
継続期間: 2011 11 142011 11 17

出版物シリーズ

名前AIP Conference Proceedings
1484
ISSN(印刷版)0094-243X
ISSN(電子版)1551-7616

Conference

ConferenceInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
国/地域Japan
CityWako
Period11/11/1411/11/17

ASJC Scopus subject areas

  • 物理学および天文学(全般)

フィンガープリント

「Cluster variational method for nuclear matter with the three-body force」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

引用スタイル