Theta dependence of the vacuum energy density in chiral effective Lagrangian models at finite temperature, above
arXiv:1903.10307 · doi:10.1103/PhysRevD.99.114009
Abstract
In this work, extending a previous study at zero temperature (), we perform a systematic study of the modifications to the QCD vacuum energy density in the finite-temperature case, above the chiral transition at , caused by a nonzero value of the parameter , using two different effective Lagrangian models which implement the axial anomaly of the fundamental theory and which are both well defined also above . In particular, we derive (and critically compare) the expressions for the topological susceptibility and for the second cumulant starting from the dependence of in the two models.
arXiv comment23 pages; revised version
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