Comment on "Brown Dwarfs, Quark Stars, and Quark-Hadron Phase Transition"
Astrophysics
2016-08-30 v1
Abstract
Recently, Cottingham, Kalafatis and Vinh Mau proposed, in the framework of the Lee-Wick model, a scenario of formation of quark stars in the cosmological quark-hadron phase transition with high degree of supercooling. We show here that the cosmological quark-hadron phase transition in the Lee-Wick model with such a high degree of supercooling cannot be completed. No quark stars could be formed in this scenario.
Cite
@article{arxiv.astro-ph/9603126,
title = {Comment on "Brown Dwarfs, Quark Stars, and Quark-Hadron Phase Transition"},
author = {S. Kubis and M. Kutschera},
journal= {arXiv preprint arXiv:astro-ph/9603126},
year = {2016}
}
Comments
2 pages, plain TEX, no figures, Physical Review Letters in press