QCD -vacua from the chiral limit to the quenched limit
arXiv:1408.1189 · doi:10.1016/j.nuclphysb.2014.11.002
Abstract
We investigate the dependence of the QCD vacuum structure on the -angle and quark mass, using the Di-Vecchia--Veneziano model. Although the Di-Vecchia--Veneziano model is a chiral effective model, it contains the topological properties of the pure Yang--Mills theory. It is shown that within this model, the ground state energies for all are continuous functions of quark mass from the chiral limit to the quenched limit, even including the first order phase transition at . Based on this effective model, we discuss (i) how the ground state depends on quark mass, and (ii) why the phase transition at is present both in the chiral and quenched limit. In order to analyze the relation between quark mass and the -vacua, we calculate the chiral condensate as a function of quark mass. Also, considering the presence of the innate metastable states included in the QCD -vacuum, we also give a unified understanding of the phase transitions at in the chiral and quenched limit.
18 pages, 8 figures
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