Journal
PHYSICAL REVIEW D
Volume 61, Issue 8, Pages -Publisher
AMERICAN PHYSICAL SOC
DOI: 10.1103/PhysRevD.61.083509
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The abundance and size distribution of quark nuggets (QN's), formed a few microseconds after the big bang due to a first-order QCD phase transition in the early universe, has been estimated. It appears that stable QN's could be a viable candidate for cosmological dark matter. The evolution of baryon inhomogeneity due to evaporated (unstable) QN's is also examined.
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