Abstract
In QCD above the chiral restoration temperature there exists an Anderson transition in the fermion spectrum from localized to delocalized modes. We investigate whether the same holds for nonlinear sigma models which share properties like dynamical mass generation and asymptotic freedom with QCD. In particular we study the spectra of fermions coupled to (quenched) CP(N-1) configurations at high temperatures. We compare results in two and three space-time dimensions: in two dimensions the Anderson transition is absent, since all fermion modes are localized, while in three dimensions it is present. Our measurements include a more recent observable characterizing level spacings: the distribution of ratios of consecutive level spacings.
Highlights
Anderson localization has been studied for a number of years in the context of QCD
We investigate whether the same holds for nonlinear sigma models which share properties like dynamical mass generation and asymptotic freedom with QCD
In the confined phase the QCD Dirac operator has no gap in the spectrum; its statistics is well described by the Gaussian unitary ensemble (GUE) of random matrix theory
Summary
Anderson localization has been studied for a number of years in the context of QCD. In the confined phase the QCD Dirac operator has no gap in the spectrum; its statistics is well described by the Gaussian unitary ensemble (GUE) of random matrix theory. In QCD above the chiral restoration temperature there exists an Anderson transition in the fermion spectrum from localized to delocalized modes. At the same time the statistics of the low end of the spectrum becomes Poissonian, that is, the eigenmodes become localized [1,2,3,4,5], the same is true for the quenched case [1, 6]. For eigenvalues corresponding to localized modes the level spacing is Poissonian, P(s) = e−s.
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