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Transport coefficients of the quark-gluon plasma at the critical point and across the first-order line

Joaquin Grefa, Mauricio Hippert, Jorge Noronha, Jacquelyn Noronha-Hostler, Israel Portillo, Claudia Ratti, and Romulo Rougemont
Phys. Rev. D 106, 034024 – Published 23 August 2022

Abstract

A bottom-up Einstein-Maxwell-dilaton holographic model is used to compute, for the first time, the behavior of several transport coefficients of the hot and baryon-rich strongly coupled quark-gluon plasma at the critical point and also across the first-order phase transition line in the phase diagram. The observables under study are the shear and bulk viscosities, the baryon and thermal conductivities, the baryon diffusion, the jet quenching parameter q^, as well as the heavy-quark drag force and the Langevin diffusion coefficients. These calculations provide a phenomenologically promising estimate for these coefficients, given that our model quantitatively reproduces lattice QCD thermodynamics results, both at zero and finite baryon density, besides naturally incorporating the nearly perfect fluidity of the quark-gluon plasma. We find that the diffusion of baryon charge, and also the shear and bulk viscosities, are suppressed with increasing baryon density, indicating that the medium becomes even closer to perfect fluidity at large densities. On the other hand, the jet quenching parameter and the heavy-quark momentum diffusion are enhanced with increasing density. The observables display a discontinuity gap when crossing the first-order phase transition line, while developing an infinite slope at the critical point. The transition temperatures associated with different transport coefficients differ in the crossover region but are found to converge at the critical point.

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  • Received 30 March 2022
  • Accepted 1 August 2022

DOI:https://doi.org/10.1103/PhysRevD.106.034024

© 2022 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Joaquin Grefa1, Mauricio Hippert2, Jorge Noronha2, Jacquelyn Noronha-Hostler2, Israel Portillo1, Claudia Ratti1, and Romulo Rougemont3

  • 1Physics Department, University of Houston, Houston, Texas 77204, USA
  • 2Illinois Center for Advanced Studies of the Universe, Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
  • 3Instituto de Física, Universidade Federal de Goiás, Av. Esperança—Campus Samambaia, CEP 74690-900, Goiânia, Goiás, Brazil

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Issue

Vol. 106, Iss. 3 — 1 August 2022

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