EVAPORATION OF QUARK DROPS DURING THE COSMOLOGICAL Q-H TRANSITION

Details EVAPORATION OF QUARK DROPS DURING THE COSMOLOGICAL Q-H TRANSITION EVAPORATION OF QUARK DROPS DURING THE COSMOLOGICAL Q-H TRANSITION

1995-02-13

arxiv.org/abs/astro-ph/9502064v1

Phys.Rev. D52 (1995) 3202-3213

Astronomy and Astrophysics

Astrophysics

12 pages Phys. Rev. format, uuencoded postscript file including 12 figures

Scientific paper

10.1103/PhysRevD.52.3202

We have carried out a study of the hydrodynamics of disconnected quark regions during the final stages of the cosmological quark-hadron transition. A set of relativistic Lagrangian equations is presented for following the evaporation of a single quark drop and results from the numerical solution of this are discussed. A self-similar solution is shown to exist and the formation of baryon number density inhomogeneities at the end of the drop contraction is discussed.

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