@inproceedings{2ce4c585cffc41c69e42f5be401067d0,
title = "Cluster variational method for nuclear matter with the three-body force",
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.",
keywords = "Neutron stars, Nuclear EOS, Nuclear matter, Supernovae, Variational method",
author = "M. Takano and H. Togashi and S. Yamamuro and K. Nakazato and H. Suzuki",
year = "2012",
doi = "10.1063/1.4763426",
language = "English",
isbn = "9780735410961",
series = "AIP Conference Proceedings",
pages = "378--380",
booktitle = "Origin of Matter and Evolution of Galaxies 2011",
note = "International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 ; Conference date: 14-11-2011 Through 17-11-2011",
}