Curvature energy effects on large-scale inhomogeneities from the cosmological QCD phase transition.

Details Curvature energy effects on large-scale inhomogeneities from the cosmological QCD phase transition. Curvature energy effects on large-scale inhomogeneities from the cosmological QCD phase transition.

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996jkps...29..537s&link_type=abstract

Journal of the Korean Physical Society, Vol. 29, No. 4, p. 537 - 540

Physics

Early Universe: Phase Transitions, Cosmology: Nucleosynthesis

Scientific paper

The authors study the curvature energy effects on large-scale inhomogeneities from the first-order quark-hadron phase transition in the early Universe. They find that, when the curvature term is included in the bubble free energy, the average distance between bubbles nucleated in the phase transition is slightly reduced. However, for some QCD parameter values, the distance scale is calculated to be large enough to affect the primordial nucleosynthesis.

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