Cosmological quark-hadron phase transition and formation of isothermal density fluctuations

Details Cosmological quark-hadron phase transition and formation of isothermal density fluctuations Cosmological quark-hadron phase transition and formation of isothermal density fluctuations

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phlb..169..337i&link_type=abstract

Physics Letters B, Volume 169, Issue 4, p. 337-342.

Physics

24

Scientific paper

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.

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