Lattice QCD for Cosmology
Sz. Borsanyi, Z. Fodor, K. H. Kampert, S. D. Katz, T. Kawanai, T. G., Kovacs, S. W. Mages, A. Pasztor, F. Pittler, J. Redondo, A. Ringwald, K. K., Szabo

TL;DR
This paper provides detailed lattice QCD calculations of the universe's equation of state across a wide temperature range, including effects of electroweak theory, and explores implications for dark matter axion properties.
Contribution
It extends lattice QCD calculations to 2+1+1+1 flavors and incorporates electroweak effects to model cosmological evolution and dark matter axion constraints.
Findings
Equation of state for 2+1+1+1 flavor QCD across broad temperature range
Calculated topological susceptibility up to a few GeV temperature
Provided relations between axion mass, initial angle, and universe evolution
Abstract
We present a full result for the equation of state (EoS) in 2+1+1 (up/down, strange and charm quarks are present) flavour lattice QCD. We extend this analysis and give the equation of state in 2+1+1+1 flavour QCD. In order to describe the evolution of the universe from temperatures several hundreds of GeV to several tens of MeV we also include the known effects of the electroweak theory and give the effective degree of freedoms. As another application of lattice QCD we calculate the topological susceptibility (chi) up to the few GeV temperature region. These two results, EoS and chi, can be used to predict the dark matter axion's mass in the post-inflation scenario and/or give the relationship between the axion's mass and the universal axionic angle, which acts as a initial condition of our universe.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Cosmology and Gravitation Theories
