Quark-hadron phase transition in bianchi type I cosmology

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Scientific paper

Assuming the quark-hadron transition is a first order singular transition, it is investigated in a cosmological anisotropic framework. We find a general form for the expansion law in the actual phase transition: it deviates from a ``radiative'' behaviour as in a FRW model. The actual phase transition time length is shorter than in the FRW case.

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