Extending the truncated Dyson-Schwinger equation to finite temperatures
S. M. Dorkin, M. Viebach, L. P. Kaptari, B. Kampfer

TL;DR
This paper investigates how the truncated Dyson-Schwinger equation for the quark propagator can be extended to finite temperatures, analyzing the temperature dependence of the interaction kernel and its implications for meson properties and quark deconfinement.
Contribution
It introduces modifications to the Dyson-Schwinger equation at finite temperatures, especially screening effects, to better match lattice QCD results and explore in-medium meson modifications.
Findings
Vacuum interaction parameters are reasonable at low T.
Interaction kernel needs screening modifications above T_c.
Analysis provides insights into quark deconfinement conditions.
Abstract
In view of the properties of mesons in hot strongly interacting matter the properties of the solutions of the truncated Dyson-Schwinger equation for the quark propagator at finite temperatures within the rainbow-ladder approximation are analysed in some detail. In Euclidean space within the Matsubara imaginary time formalism the quark propagator is not longer a O(4) symmetric function and possesses a discrete spectra of the fourth component of the momentum. This makes the treatment of the Dyson-Schwinger and Bethe-Salpeter equations conceptually different from the vacuum and technically much more involved. The question whether the interaction kernel known from vacuum calculations can be applied at finite temperatures remains still open. We find that, at low temperatures, the model interaction with vacuum parameters provides a reasonable description of the quark propagator, while at…
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