Abstract
The possibility of a mini-inflationary era before and during the cosmic confinement transition is demonstrated. The inflationary growth of the space is caused by some supercooling of the quark-gluon matter. We study the temperature evolution by exploiting nucleation theory.
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Jenkovszky, L.L., Kämpfer, B. & Sysoev, V.M. On the expansion of the universe during the confinement transition. Z. Phys. C - Particles and Fields 48, 147–150 (1990). https://doi.org/10.1007/BF01565617
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DOI: https://doi.org/10.1007/BF01565617