Relics of the Cosmological QCD Phase Transition

Details Relics of the Cosmological QCD Phase Transition Relics of the Cosmological QCD Phase Transition

1999-01-14

arxiv.org/abs/hep-ph/9901308v2

Phys.Rev. D61 (2000) 083509

Physics

High Energy Physics

High Energy Physics - Phenomenology

To appear in Physical Review D

Scientific paper

10.1103/PhysRevD.61.083509

The abundance and size distribution of quark nuggets (QN), formed a few
microseconds after the big bang due to first order QCD phase transition in the
early universe, has been estimated. It appears that stable QNs could be a
viable candidate for cosmological dark matter. The evolution of baryon
inhomogeneity due to evaporated (unstable) QNs are also examined.

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