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

Abstract

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.

arXiv comment24 small pages, Presented by JR at 52 Kraków School of Theoretical Physics: Astroparticle Physics in the LHC Era, Zakopane, May 19-27, 2012

Cited by in corpus (16)

• Hadron production and QGP Hadronization in Pb--Pb collisions at $\sqrt{s_{NN}}=2.76$ TeV
• Beam Energy Dependence of Jet-Quenching Effects in Au+Au Collisions at $\sqrt{s_{{}_{\mathrm{NN}}}}$ = 7.7, 11.5, 14.5, 19.6, 27, 39, and 62.4 GeV
• Discovery of Quark-Gluon-Plasma: Strangeness Diaries
• Connecting QGP-Heavy Ion Physics to the Early Universe
• A short survey of matter-antimatter evolution in the primordial universe
• Measurements of chemical potentials in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$ TeV
• Traveling Through the Universe: Back in Time to the Quark-Gluon Plasma Era
• The case for mixed dark matter from sterile neutrinos
• Cosmological Strangeness Abundance
• The Trajectory of the Cosmic Plasma Through the Quark Matter Phase Diagram
• Matter-antimatter origin of cosmic magnetism
• Diffusion coefficients and constraints on hadronic inhomogeneities in the early universe
• Short Note on Spin Magnetization in QGP
• Quarks to Cosmos: Particles and Plasma in Cosmological evolution
• Highly suppressed detection probability of the primordial antimatter in the present-day universe
• Higgs Thermal Nonequilibrium in Primordial QGP