Confinement transition in cosmology

Physics

Scientific paper

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Scientific paper

We discuss the expansion law and the thermal history of the universe at the time of the quark-hadron transition, assuming that such transition is strongly first order, but takes place reversibly. General thermodynamical proporties are outlined. The possible use of numerical QCD outputs is shown. Results are compared with those holding in the case of a second-order or weakly first-order transition.
On leave of absence from Jagellonian University of Cracow, Poland.

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