“…Namely, chiral condensate must be non-zero in the presence of the large monopole cluster, i.e., in the confinement phase. In the high temperature, deconfinement phase, the large monopole cluster is absent [18], and, as a result, the chiral symmetry breaking ceases to exist. Naively, one may suggest that the chiral condensate is proportional to the density of the largest monopole cluster, ρ IR , at least, at zero temperatures,…”