The cosmological quark-hadron transition

Details The cosmological quark-hadron transition The cosmological quark-hadron transition

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991nuphs..24...54b&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 24, Issue 2, p. 54-58.

Physics

Nuclear Physics

Scientific paper

Current results on homogenous primeval nucleosynthesis are hardly consistent with a baryonic density large enough to allow cooling down primeval fluctuations (over galactic scale) and the growing consensus than H >~ 75 km s-1 Mpc-1. The quark-hadron transition may result in inhomogeneous nucleosynthesis. Computations of supercooling during the transition are a step towards connecting microphysical parameters and inhomogeneity features. Recent results on supercooling are given.

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