Abstract

We use holography to investigate the process of homogeneous isotropization and thermalization in a strongly coupled mathcal{N}=4 Super Yang-Mills plasma charged under a U(1) subgroup of the global SU(4) R-symmetry which features a critical point in its phase diagram. Isotropization dynamics at late times is affected by the critical point in agreement with the behavior of the characteristic relaxation time extracted from the analysis of the lowest non-hydrodynamic quasinormal mode in the SO(3) quintuplet (external scalar) channel of the theory. In particular, the isotropization time may decrease or increase as the chemical potential increases depending on whether one is far or close enough to the critical point, respectively. On the other hand, the thermalization time associated with the equilibration of the scalar condensate, which happens only after the system has relaxed to a (nearly) isotropic state, is found to always increase with chemical potential in agreement with the characteristic relaxation time associated to the lowest non-hydrodynamic quasinormal mode in the SO(3) singlet (dilaton) channel. These conclusions about the late dynamics of the system are robust in the sense that they hold for different initial conditions seeding the time evolution of the far-from-equilibrium plasma.

Highlights

  • The far-from-equilibrium dynamics describing the relaxation of holographic fluids toward thermodynamic equilibrium in many different settings

  • We use holography to investigate the process of homogeneous isotropization and thermalization in a strongly coupled N = 4 Super Yang-Mills plasma charged under a U(1) subgroup of the global SU(4) R-symmetry which features a critical point in its phase diagram

  • Isotropization dynamics at late times is affected by the critical point in agreement with the behavior of the characteristic relaxation time extracted from the analysis of the lowest non-hydrodynamic quasinormal mode in the SO(3) quintuplet channel of the theory

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Summary

The holographic model and its equations of motion

Before we delve into the numerics and solve the system of PDEs (2.14a)–(2.14g) following the above algorithm, there are still some technical details that we need to take into account Some of these details are: the boundary conditions, the equilibrium solutions, and the initial data. Still, using the formulas derived from holographic renormalization in appendix A, we provide holographic formulas to calculate the energy density and the pressure coming from Tμν , the charge density that comes from the temporal component of Jμ , and the expectation value of the scalar operator dual to the dilaton field, Oφ.

Near-boundary expansion of the bulk fields
Thermodynamics
Field redefinitions
Radial position of the black hole event horizon
Initial states
Numerical techniques
Equilibration dynamics: results for different initial data
Constant metric anisotropy and dilaton profiles
Constant metric anisotropy profile and Gaussian dilaton profile
Gaussian metric anisotropy profile and constant dilaton profile
Gaussian metric anisotropy and dilaton profiles
Gaussian metric anisotropy profile and equilibrium dilaton profile
Matching the quasinormal modes
Outlook and final remarks
A Holographic renormalization
Counterterm action
One-point functions

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