2016/06/23 by Sz. Borsanyi, Sz. Borsányi, Z. Fodor +31 · 1 voice · 66 citations
Physics and Astronomy · #Astrophysics #Axion #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Electroweak interaction #Equation of state #Lattice QCD #Particle physics #Particle physics theoretical and experimental studies #Physics #Quantum chromodynamics #Quantum mechanics #Quark #Theoretical physics #astro-ph.CO #hep-lat #hep-ph
paper · pdf · doi:10.48550/arxiv.1606.07494
published in arXiv (Cornell University) (Cornell University) · pdflatex, 40 figures; Section on experimental setups added, small corrections
openalex publication_date 2016/06/23 · arxiv created 2016/06/27 · arxiv updated 2016/06/29 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
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.