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From Quark-Gluon Universe to Neutrino Decoupling: 200<T<2MeV

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arxiv 1211.4297 v1 pith:5L2TAX6M submitted 2012-11-19 nucl-th astro-ph.COhep-ph

Michael J. Fromerth , Inga Kuznetsova , Lance Labun , Jean Letessier , Jan Rafelski This is my paper · ORCID
classification nucl-thastro-ph.COhep-ph
keywords hadronabundanceshadronsuniversebecomeconsiderationsdecouplingdescribed
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The properties of the quark and hadron Universe are explored. Kinetic theory considerations are presented proving that hadron abundances after phase transformation from quarks to hadrons remain intact till abundances of hadrons become irrelevant. The hadronization process and the evolution of hadron yields is described in detail.

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Cited by 1 Pith paper

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  1. Higgs Thermal Nonequilibrium in Primordial QGP

    hep-ph 2025-02 reject novelty 5.0 of 10

    The paper predicts that primordial Higgs bosons maintained a constant chemical fugacity of 0.69 and a nonthermal, cold momentum distribution below T = 25 GeV.

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