Baryon-number fluctuations in a quark-hadron phase transition

Details Baryon-number fluctuations in a quark-hadron phase transition Baryon-number fluctuations in a quark-hadron phase transition

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvd..49.4023s&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 49, Issue 8, 15 April 1994, pp.4023-4027

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9

Relativistic Stars: Structure, Stability, And Oscillations, Quark-Gluon Plasma, Origin, Formation, And Abundances Of The Elements

Scientific paper

Isothermal baryon-number fluctuations arising from a first-order quark-hadron phase transition in the early Universe are obtained by including the quark-gluon interactions up to the order g3s in the perturbative QCD coupling constant in the quark-gluon plasma (QGP) phase and the finite-size volume corrections for the hadrons in the hadron-resonance gas (HRG) and their effects on the primordial nucleosynthesis (PNS) are analyzed. The ratio of the baryon-number densities in the QGP and HRG phases at the critical temperature Tc is larger than one in the range 150 MeV

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