Connecting far-from-equilibrium hydrodynamics to resummed transport coefficients and attractors
arXiv:2003.00181 · doi:10.1016/j.nuclphysa.2020.121748
Abstract
We investigate whether hydrodynamic attractors are present in simulations of the quark-gluon plasma formed in heavy-ion collisions. We argue that Lagrangian schemes to solve the relativistic viscous fluid equations can be particularly useful to characterize the properties of attractors in heavy ion collisions. Preliminary results are shown in Israel-Stewart theory to support such a claim. We also discuss how to perform the slow-roll expansion in Israel-Stewart theory undergoing a general flow, which naturally leads to the definition of a resummed shear viscosity coefficient that depends on the gradients of the hydrodynamic fields.
4 pages, 1 figure, contribution to the Quark Matter 2019 proceedings
References in corpus (4)
- Bulk viscosity-driven suppression of shear viscosity effects on the flow harmonics at RHIC
- Studying the validity of relativistic hydrodynamics with a new exact solution of the Boltzmann equation
- Exact hydrodynamic attractor of an ultrarelativistic gas of hard spheres
- How large is the Knudsen number reached in fluid dynamical simulations of ultrarelativistic heavy ion collisions?
Cited by in corpus (13)
- Nonlinear Constraints on Relativistic Fluids Far From Equilibrium
- at RHIC and the LHC comparing clustering vs substructure
- On non-conformal kinetic theory and hydrodynamics for Bjorken flow
- Progress and Challenges in Small Systems
- Relativistic Bulk Rheology: From Neutron Star Mergers to Viscous Cosmology
- Shear flows in far-from-equilibrium strongly coupled fluids
- Shear transport far from equilibrium via holography
- Relativistic Hydrodynamics: A Singulant Perspective
- Linearized dispersion relations in viscous relativistic hydrodynamics
- Field Theory Approaches to Relativistic Hydrodynamics
- Role of slow, out-of-equilibrium modes on the dynamic structure factor near the QCD critical point
- Normal mode analysis within a mutilated relaxation time approximation
- Normal mode analysis within relativistic massive transport