“…The equation of state (EOS) for nuclear matter at high density is closely related to the structure of neutron star [1], and at lower density it connects to the α-particle condensation in symmetric nuclear matter [2], together with the α cluster states in finite nuclear system [3]. The typical ab initio methods for nuclear matter calculations are the Brueckner-Hartree-Fock (BHF) [4][5][6], the Brueckner-Bethe-Goldstone (BBG) [5][6][7], the Fermi hypernetted chain/single-operator chain (FHNC/SOC) [8][9][10][11], the selfconsistent Green's function (SCGF) [12][13][14], the auxiliary field diffusion Monte Carlo (AFDMC) [15][16][17], the coupled-cluster (CC) [18][19][20], the lowest-order constrained variational (LOCV) [21][22][23], and so on. The comparative study of the EOS's obtained by BHF, BBG, FHNC/SOC, SCGF, and AFDMC, using the Argonne two-nucleon potentials (AV4', AV6', AV8' and AV18) [24], has disclosed [6] that the EOS for symmetric nuclear matter depends significantly on the ab initio methods, in particular, at the higher density region.…”