Thermodynamics of cosmological models with a variable matter equation of state

V.M. Zhuravlev and R.R. Abbyazov1


We consider cosmological models with a self-interacting scalar field and a perfect fluid with a variable equation of state in spatially flat Friedmann-Robertson-Walker space-times. The main purpose of the paper is a study of general thermodynamic properties of such models and their relationship with the dynamics of geometry.


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