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Quantum Corrections to $η/s$ from JT Gravity

Sera Cremonini, Li Li, Xiao-Long Liu, Jun Nian

TL;DR

This work investigates how IR quantum fluctuations of near-extremal black branes, captured via Jackiw–Teitelboim (JT) gravity and its Schwarzian sector, modify the holographic shear viscosity to entropy ratio $\eta/s$ at finite chemical potential. By computing the quantum-corrected IR retarded Green's function and relating it to the UV function through the standard holographic dictionary, the authors introduce a temperature-dependent renormalized dimension $\ell'$ that encapsulates quantum effects and yields a corrected $\eta'/s'$ in two regimes: a semiclassical regime ($T\gg 1/C$) and a quantum regime ($T\ll 1/C$). They find that $\eta/s$ develops a nontrivial $T$-dependence, with a minimum below the KSS bound in the semiclassical region and a rapid rise above the bound in the deep quantum regime, driven by quantum corrections to the entropy $s'$, which includes a $\log(CT)$ term. The results are cross-checked against the quantum-corrected absorption cross-section, showing consistent transport-absorption behavior and offering insight into how finite-$N$ IR effects can alter hydrodynamic bounds in holographic theories.

Abstract

We revisit the computation of the shear viscosity to entropy ratio $η/s$ at finite chemical potential in a holographic model that takes into account the quantum fluctuations in the IR region of near-extremal black branes. Such quantum corrections can be computed from JT gravity and generate non-trivial temperature dependence for $η/s$, which deviates from the universal $1/4π$ result. In the semi-classical regime, $η/s$ attains a minimum which is below the KSS bound, generated by the presence of the quantum effects. In the quantum regime at lower temperatures, $η/s$ increases and is well above the KSS bound. We also compare the shear viscosity to the quantum-corrected absorption cross-section of near-extremal black holes, and find agreement.

Quantum Corrections to $η/s$ from JT Gravity

TL;DR

This work investigates how IR quantum fluctuations of near-extremal black branes, captured via Jackiw–Teitelboim (JT) gravity and its Schwarzian sector, modify the holographic shear viscosity to entropy ratio at finite chemical potential. By computing the quantum-corrected IR retarded Green's function and relating it to the UV function through the standard holographic dictionary, the authors introduce a temperature-dependent renormalized dimension that encapsulates quantum effects and yields a corrected in two regimes: a semiclassical regime () and a quantum regime (). They find that develops a nontrivial -dependence, with a minimum below the KSS bound in the semiclassical region and a rapid rise above the bound in the deep quantum regime, driven by quantum corrections to the entropy , which includes a term. The results are cross-checked against the quantum-corrected absorption cross-section, showing consistent transport-absorption behavior and offering insight into how finite- IR effects can alter hydrodynamic bounds in holographic theories.

Abstract

We revisit the computation of the shear viscosity to entropy ratio at finite chemical potential in a holographic model that takes into account the quantum fluctuations in the IR region of near-extremal black branes. Such quantum corrections can be computed from JT gravity and generate non-trivial temperature dependence for , which deviates from the universal result. In the semi-classical regime, attains a minimum which is below the KSS bound, generated by the presence of the quantum effects. In the quantum regime at lower temperatures, increases and is well above the KSS bound. We also compare the shear viscosity to the quantum-corrected absorption cross-section of near-extremal black holes, and find agreement.
Paper Structure (13 sections, 72 equations, 2 figures)

This paper contains 13 sections, 72 equations, 2 figures.

Figures (2)

  • Figure 4: The quantum-corrected shear viscosity-entropy ratio as a function of temperature in the semiclassical regime $CT\gg 1$. The dashed blue line denotes the KSS bound. We have chosen $\kappa = 1$, $L = 0.1$, $r_0 = 1$.
  • Figure 5: The left panel shows the temperature dependence of the quantum-corrected shear viscosity-entropy ratio in the quantum regime $CT\ll 1$. The dashed blue line denotes the KSS bound and the dashed red line denoted the fitting function $4\pi(\eta'/s')=e^{-0.33}\times(CT)^{- 1.03}$. The right panel shows the same quantities in a log-log plot. The blue shaded area schematically represents the region where the entropy is negative, indicating the breakdown of the quantum-corrected $\eta/s$. We have set $\kappa = 1$, $L = 0.1$, $r_0 = 1$.