Comment on "Brown Dwarfs, Quark Stars, and Quark-Hadron Phase Transition"

Details Comment on "Brown Dwarfs, Quark Stars, and Quark-Hadron Phase Transition" Comment on "Brown Dwarfs, Quark Stars, and Quark-Hadron Phase Transition"

1996-03-23

arxiv.org/abs/astro-ph/9603126v1

Phys.Rev.Lett. 76 (1996) 3876

Astronomy and Astrophysics

Astrophysics

2 pages, plain TEX, no figures, Physical Review Letters in press

Scientific paper

10.1103/PhysRevLett.76.3876

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.

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