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 axions mass in the post-inflation scenario and/or give the relationship between the axions mass and the universal axioni...
We calculate the equation of state in 2+1 flavor QCD at finite temperature with physical strange qua...
The present paper concludes our investigation on the QCD equation of state with 2 + 1 staggered flav...
AbstractAxions are one of the most attractive dark matter candidates. The evolution of their number ...
We present a full result for the equation of state (EoS) in 2+1+1 (up/down, strange and charm quarks...
We conclude our investigation on the QCD equation of state (EoS) with 2+1 staggered flavors and one-...
We report on a continuum extrapolated result [1] for the equation of state (EoS) of QCD with N f = 2...
We provide a status report on the calculation of the Equation of State (EoS) of QCD at finite temper...
Borsanyi S, Endrödi G, Fodor Z, et al. N_f=2+1 flavour equation of state. arXiv:1011.4229. 2010.We c...
Unlike the electroweak sector of the standard model of particle physics, quantum chromodynamics (QCD...
We present an ongoing project aimed at determining the thermodynamic Equation of State (EoS) of quar...
We report on a continuum extrapolated result [1] for the equation of state (EoS) of QCD with Nf = 2 ...
Based on S. Borsanyi et al., “Calculation of the axion mass based on high-temperature lattice quantu...
Axions are one of the most attractive dark matter candidates. The evolution of their number density ...
Borsanyi S, Endrödi G, Fodor Z, et al. QCD thermodynamics on the lattice and in the Hadron Resonance...
We report on a continuum extrapolated result [1] for the equation of state (EoS) of QCD with N f = 2...
We calculate the equation of state in 2+1 flavor QCD at finite temperature with physical strange qua...
The present paper concludes our investigation on the QCD equation of state with 2 + 1 staggered flav...
AbstractAxions are one of the most attractive dark matter candidates. The evolution of their number ...
We present a full result for the equation of state (EoS) in 2+1+1 (up/down, strange and charm quarks...
We conclude our investigation on the QCD equation of state (EoS) with 2+1 staggered flavors and one-...
We report on a continuum extrapolated result [1] for the equation of state (EoS) of QCD with N f = 2...
We provide a status report on the calculation of the Equation of State (EoS) of QCD at finite temper...
Borsanyi S, Endrödi G, Fodor Z, et al. N_f=2+1 flavour equation of state. arXiv:1011.4229. 2010.We c...
Unlike the electroweak sector of the standard model of particle physics, quantum chromodynamics (QCD...
We present an ongoing project aimed at determining the thermodynamic Equation of State (EoS) of quar...
We report on a continuum extrapolated result [1] for the equation of state (EoS) of QCD with Nf = 2 ...
Based on S. Borsanyi et al., “Calculation of the axion mass based on high-temperature lattice quantu...
Axions are one of the most attractive dark matter candidates. The evolution of their number density ...
Borsanyi S, Endrödi G, Fodor Z, et al. QCD thermodynamics on the lattice and in the Hadron Resonance...
We report on a continuum extrapolated result [1] for the equation of state (EoS) of QCD with N f = 2...
We calculate the equation of state in 2+1 flavor QCD at finite temperature with physical strange qua...
The present paper concludes our investigation on the QCD equation of state with 2 + 1 staggered flav...
AbstractAxions are one of the most attractive dark matter candidates. The evolution of their number ...