Abstract

Density fluctuations in small phase space bins for centrally produced particles are conveniently parametrized by a Gaussian free energy functional of the density fluctuation field. This observation leads to the investigation of the O( N) linear σ-model; the O(4) version serves as a prototype theory of the QCD chiral order parameter. We derive an exact, non-perturbative and finite equation for its finite temperature effective action. In the large- N limit, well-known results on the nature of the phase transition are recovered. Thus, we obtain the Ginzburg-Landau theory for a QCD system in thermodynamic equilibrium.

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