“…A phase structure of the strongly interacting matter of quantum chromodynamics (QCD) at nonvanishing temperature and density as well as in the presence of the external magnetic field becomes an interested topic in nuclear physics community in the last few years. In the theory side, many attempts have been done to study the phase-diagram of QCD in the nonvanishing temperature and chemical potential/density , starting from the low density/chemical potential and/or high temperature which is relevant for the early universe phenomena [32] until the low temperature and/or high density/chemical potential, which is relevant to the central core of the neutron star or compact star phenomena [33,34] using several various QCD inspired models [3,6,8,9,[21][22][23][24] with different approaches [8,9,21,26,27] as well as lattice QCD [2,19,25,[28][29][30] and remarkable progresses have been made until today. However, there are some problems to remain, namely, the sign problem [35][36][37], uncertain location of the critical end point (CEP) [38][39][40], and the chiral imbalance [38,41], which is related to the chiral magnetic effect (CME).…”