Abstract
This paper examines the thermodynamics of relativistic phase transitions in which the heterogeneity of the system (the vacuum condensate, scalar and vector particles) is considered evident. The given system does not have a united functional of state which is common to both low-symmetric and high-symmetric phases. The theory acquires the necessary physical content after the introduction of additional parameters of order identified with the parameters of the energetic spectrum (effective masses of particles), The many-parameter thermodynamics of relativistic phase transitions in heterogeneous systems changes the current conceptions about the character of these transitions and about the properties of the system near the critical point. For T>Tcrit the system of Higgs fields has no thermodynamical equilibrium states and it can evolve under stochastic laws only. For T<Tcrit the stochastic regime of evolution begins to relax to the local thermodynamical equilibrium regime.
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