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

S. Kubis·M. Kutschera
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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.

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S. Kubis, M. Kutschera. 1996-03-23. Comment on "Brown Dwarfs, Quark Stars, and Quark-Hadron Phase Transition". https://doi.org/10.1103/physrevlett.76.3876

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