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- W2079454102 abstract "The dynamical process of the cosmological quark-hadron phase transition is investigated under the assumption of a weakly first-order phase transition. In particular the characteristic mass of these nuggets is determined to be smaller than 1019 g, using a spatial correlation function of the trapped quark phase. Furthermore, the possibility of these nuggets being left as isothermal baryonic clouds with very high density (δϱb/ϱb ∼ 5.0×1012) after evaporation is pointed out, and its cosmological implications are discussed." @default.
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- W2079454102 date "1986-04-01" @default.
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- W2079454102 title "Cosmological quark-hadron phase transition and formation of isothermal density fluctuations" @default.
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- W2079454102 doi "https://doi.org/10.1016/0370-2693(86)90368-0" @default.
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