# Transport and Response Coefficients in Second-Order Dissipative Relativistic Hydrodynamics with Quantum Corrections: Probing the Quark–Gluon Plasma

**Authors:** Iberê Kuntz, Roldao da Rocha

PMC · DOI: 10.3390/e27060580 · Entropy · 2025-05-29

## TL;DR

This paper explores quantum corrections in relativistic hydrodynamics to study the quark–gluon plasma and test quantum gravity effects.

## Contribution

The paper introduces quantum corrections to transport and response coefficients in second-order relativistic hydrodynamics.

## Key findings

- Quantum corrections affect the pressure, relaxation time, and shear relaxation time in the quark–gluon plasma.
- The bulk-viscosity-to-entropy-density ratio supports the existence of a functional measure encoding quantum gravity corrections.
- High-temperature plasmas may serve as a testing ground for quantum gravity theories.

## Abstract

A functional measure encompasses quantum corrections and is explored in the fluid/gravity correspondence. Corrections to the response and transport coefficients in the second-order dissipative relativistic hydrodynamics are proposed, including those to the pressure, relaxation time, and shear relaxation time. Their dependence on the quark–gluon plasma (QGP) temperature sets a temperature dependence on the running parameter encoding the one-loop quantum gravity correction, driven by a functional measure. The experimental range of the bulk-viscosity-to-entropy-density ratio of the QGP, obtained by five different analyses (JETSCAPE Bayesian model, Duke, Jyväskylä–Helsinki–Munich, MIT–Utrecht–Genève, and Shanghai) corroborates the existence of the functional measure. Our results suggest that high-temperature plasmas could be used to experimentally test quantum gravity.

## Full-text entities

- **Chemicals:** Quark (-)

## Full text

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## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/PMC12191606/full.md

## References

81 references — full list in the complete paper: https://tomesphere.com/paper/PMC12191606/full.md

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Source: https://tomesphere.com/paper/PMC12191606