Baryon-number density in hadronic gas models and baryon asymmetry in the early Universe

Details Baryon-number density in hadronic gas models and baryon asymmetry in the early Universe Baryon-number density in hadronic gas models and baryon asymmetry in the early Universe

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phrvd..53..993p&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 53, Issue 2, 15 January 1996, pp.993-996

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3

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

Scientific paper

We have recently shown that the inclusion of finite-size volume corrections for the hadrons in the hadronic gas phase drastically alters the conclusions regarding isothermal baryon-number fluctuations arising from a first-order quark-hadron phase transition in the early Universe. In this paper we compare in detail the predictions of various existing thermodynamically consistent hadron gas (HG) models for the baryon density in the HG phase and its dependence on the temperature in order to draw a firm conclusion regarding the results obtained in the earlier paper.

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