TY - GEN
T1 - Cluster variational method for nuclear matter with the three-body force
AU - Takano, M.
AU - Togashi, H.
AU - Yamamuro, S.
AU - Nakazato, K.
AU - Suzuki, H.
PY - 2012
Y1 - 2012
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=84874536715&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84874536715&partnerID=8YFLogxK
U2 - 10.1063/1.4763426
DO - 10.1063/1.4763426
M3 - Conference contribution
AN - SCOPUS:84874536715
SN - 9780735410961
T3 - AIP Conference Proceedings
SP - 378
EP - 380
BT - Origin of Matter and Evolution of Galaxies 2011
T2 - International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
Y2 - 14 November 2011 through 17 November 2011
ER -