Thermal evolution of phases during the cosmological quark-hadron transition

Details Thermal evolution of phases during the cosmological quark-hadron transition Thermal evolution of phases during the cosmological quark-hadron transition

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...385..393m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 385, Feb. 1, 1992, p. 393-403.

Astronomy and Astrophysics

Astrophysics

Dark Matter, Hadrons, Nuclear Astrophysics, Nuclear Fusion, Quarks, Temperature Gradients, Hubble Constant, Nuclear Reactions, Universe

Scientific paper

The temperatures of the various components of the universe and the time dependence of the scale factor during a first-order quark-hadron transition, taking place with the minimal supercooling needed to drive elementary processes are determined. Both surface and volume effects are taken into account, also according to different ranges of bubble sizes. The range of validity of these results directly covers most relevant cases, including those leading to inhomogeneous primeval nucleosynthesis. Results are also relevant to determine precise cosmological limits on the masses of SUSY partners and therefore of the expected dark matter components.

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