On the magnitude of baryon-to-photon ratio inhomogeneities resulting from a first-order quark-hadron transition

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Particle-Theory And Field-Theory Models Of The Early Universe, Lattice Qcd Calculations, Quark-Gluon Plasma, Origin, Formation, And Abundances Of The Elements

Scientific paper

We show that consideration of the low-lying baryon states in addition to the neutron and proton (specifically, the Λ, Σ, and Δ states) reduces the ratio of baryon-number density in the quark phase to that in the hadronic phase by more than a factor of 2. This implies that inhomogeneities in the local baryon-number-to-photon ratio produced during the quark-hadron transition are likely to be smaller than previous estimates, and therefore unless the transition temperature is less than ~150 MeV, the effects upon primordial nucleosynthesis will not be significant.

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