Effective holographic models for QCD: Thermodynamics and viscosity coefficients
Alfonso Ballon-Bayona, Luis A. H. Mamani, Alex S. Miranda, Vilson, T. Zanchin

TL;DR
This paper extends effective holographic QCD models to finite temperature, analyzing black hole solutions, thermodynamics, and viscosity coefficients, and compares results with lattice and experimental data.
Contribution
It introduces a finite temperature extension of EHQCD models, classifies black hole solutions, and computes thermodynamic and viscosity properties, linking them to lattice and experimental results.
Findings
Large black holes are thermally stable and dual to non-conformal plasma.
Shear viscosity to entropy ratio remains universal at 1/4π.
Bulk viscosity varies with temperature and model parameters, increasing near T_min.
Abstract
A finite temperature extension of the effective holographic models for QCD (EHQCD), proposed in Ref.[1], is investigated in the present work. EHQCD models are characterized by two parameters, the conformal dimension of the relevant operator that deforms the CFT and the associated coupling. We find that black hole solutions appear at temperatures higher than some temperature and can be categorized in two classes: large and small black holes. A large black hole is thermally stable and it is therefore interpreted as the gravity dual of a non-conformal plasma. A small black hole, on the other hand, is thermally unstable. We show that thermodynamic quantities such as the entropy density , specific heat , and speed of sound are sensitive to the model parameters. We investigate perturbations of the black hole solutions and calculate the viscosity coefficients of the…
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