Uncertainty quantification of holographic transport and energy loss for the hot and baryon-dense QGP

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Main Authors: Khan, Musa R., Nascimento, Ayrton, Yang, Yumu, Grefa, Joaquin, Hippert, Mauricio, Noronha, Jorge, Ratti, Claudia, Rougemont, Romulo
Format: Preprint
Published: 2026
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author Khan, Musa R.
Nascimento, Ayrton
Yang, Yumu
Grefa, Joaquin
Hippert, Mauricio
Noronha, Jorge
Ratti, Claudia
Rougemont, Romulo
author_facet Khan, Musa R.
Nascimento, Ayrton
Yang, Yumu
Grefa, Joaquin
Hippert, Mauricio
Noronha, Jorge
Ratti, Claudia
Rougemont, Romulo
contents We investigate several transport coefficients across the phase diagram of a holographic Einstein-Maxwell-Dilaton (EMD) model of hot and dense QCD with $N_f=2+1$ flavors. Our results are obtained from an open-source implementation of this model in C++, publicly available as a module within the MUSES Framework. This code includes a new numerical method to extract thermodynamic quantities from near-boundary asymptotics in holographic models, introduced here for the first time, which greatly improves numerical stability and performance in comparison to earlier implementations. Thanks to this improved technique, we are able to compute results for many realizations of our holographic model, sampled from a Bayesian posterior distribution constrained by lattice QCD results at zero chemical potential. This allows us to propagate lattice QCD error bars to predictions of transport coefficients in a wide window of temperature and baryon chemical potential, covering the crossover region, the neighborhood of the predicted critical point, and the line of first-order phase transition. The physical observables include baryon and thermal conductivities, baryon diffusion, shear and bulk viscosities, the jet-quenching parameter, the heavy-quark drag force, and Langevin diffusion coefficients. At vanishing baryon density, we compare our results to estimates extracted by the JETSCAPE Collaboration from heavy-ion data, with which we find good agreement.
format Preprint
id arxiv_https___arxiv_org_abs_2603_20482
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Uncertainty quantification of holographic transport and energy loss for the hot and baryon-dense QGP
Khan, Musa R.
Nascimento, Ayrton
Yang, Yumu
Grefa, Joaquin
Hippert, Mauricio
Noronha, Jorge
Ratti, Claudia
Rougemont, Romulo
Nuclear Theory
High Energy Physics - Phenomenology
High Energy Physics - Theory
We investigate several transport coefficients across the phase diagram of a holographic Einstein-Maxwell-Dilaton (EMD) model of hot and dense QCD with $N_f=2+1$ flavors. Our results are obtained from an open-source implementation of this model in C++, publicly available as a module within the MUSES Framework. This code includes a new numerical method to extract thermodynamic quantities from near-boundary asymptotics in holographic models, introduced here for the first time, which greatly improves numerical stability and performance in comparison to earlier implementations. Thanks to this improved technique, we are able to compute results for many realizations of our holographic model, sampled from a Bayesian posterior distribution constrained by lattice QCD results at zero chemical potential. This allows us to propagate lattice QCD error bars to predictions of transport coefficients in a wide window of temperature and baryon chemical potential, covering the crossover region, the neighborhood of the predicted critical point, and the line of first-order phase transition. The physical observables include baryon and thermal conductivities, baryon diffusion, shear and bulk viscosities, the jet-quenching parameter, the heavy-quark drag force, and Langevin diffusion coefficients. At vanishing baryon density, we compare our results to estimates extracted by the JETSCAPE Collaboration from heavy-ion data, with which we find good agreement.
title Uncertainty quantification of holographic transport and energy loss for the hot and baryon-dense QGP
topic Nuclear Theory
High Energy Physics - Phenomenology
High Energy Physics - Theory
url https://arxiv.org/abs/2603.20482