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EVAPORATION OF QUARK DROPS DURING THE COSMOLOGICAL Q-H TRANSITION

L. Rezzolla·J. C. Miller·O. Pantano
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Abstract

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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L. Rezzolla, J. C. Miller, O. Pantano. 1995-02-13. EVAPORATION OF QUARK DROPS DURING THE COSMOLOGICAL Q-H TRANSITION. https://doi.org/10.1103/physrevd.52.3202

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