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

M. Takano, H. Togashi, S. Yamamuro, Kenichiro Nakazato, H. Suzuki

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Citation (Scopus)

Abstract

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.

Original languageEnglish
Title of host publicationOrigin of Matter and Evolution of Galaxies 2011
Pages378-380
Number of pages3
DOIs
Publication statusPublished - Dec 1 2012
Externally publishedYes
EventInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan
Duration: Nov 14 2011Nov 17 2011

Publication series

NameAIP Conference Proceedings
Volume1484
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherInternational Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
CountryJapan
CityWako
Period11/14/1111/17/11

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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    Takano, M., Togashi, H., Yamamuro, S., Nakazato, K., & Suzuki, H. (2012). Cluster variational method for nuclear matter with the three-body force. In Origin of Matter and Evolution of Galaxies 2011 (pp. 378-380). (AIP Conference Proceedings; Vol. 1484). https://doi.org/10.1063/1.4763426