Equation of State for Cosmological Matter at and beyond QCD and Electroweak Eras

28 Feb 2019 Tawfik Abdel Nasser Nile U., ECTP & WLCAPP, Cairo Mishustin Igor Frankfurt U., FIAS & Kurchatov Inst., Moscow

Various thermodynamic quantities for baryon-free matter are calculated by combining the most reliable non-perturbative and perturbative calculations, especially the most recent ones including as many quark flavors as possible. We extend these calculations by including other degrees of freedom (dof), such as photons, neutrinos, leptons, electroweak particles, and Higgs bosons, that allows us to consider the temperatures up to the TeV-scale... (read more)

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  • HIGH ENERGY PHYSICS - PHENOMENOLOGY
  • HIGH ENERGY PHYSICS - LATTICE