Aspects of the quark-hadron phase transition.

Details Aspects of the quark-hadron phase transition. Aspects of the quark-hadron phase transition.

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hadjs..10...61o&link_type=abstract

Hadronic J. Suppl., Vol. 10, No. 1, p. 61 - 88

Physics

Nucleosynthesis: Big-Bang Theory, Quark Matter: Neutron Stars

Scientific paper

A transition from normal hadronic matter (e.g. protons and neutrons) to quark-gluon matter is expected at both high temperatures and densities. In physical situations, this transition may occur in heavy ion collisions, the early Universe, and in the cores of neutron stars. In this article, the author discusses the transition in the latter two of these environments. He briefly reviews the standard model of big bang nucleosynthesis, the theory describing the primordial origin of the light elements and discuss the effect of inhomogeneities produced by the transition on big bang nucleosynthesis. He also discusses the uncertainties caused by a possible transition to quark matter in the interior of neutron stars.

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