EVAPORATION OF QUARK DROPS DURING THE COSMOLOGICAL Q-H TRANSITION
Astrophysics
2016-08-30 v1 High Energy Physics - Phenomenology
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.
Keywords
Cite
@article{arxiv.astro-ph/9502064,
title = {EVAPORATION OF QUARK DROPS DURING THE COSMOLOGICAL Q-H TRANSITION},
author = {L. Rezzolla and J. C. Miller and O. Pantano},
journal= {arXiv preprint arXiv:astro-ph/9502064},
year = {2016}
}
Comments
12 pages Phys. Rev. format, uuencoded postscript file including 12 figures