Breakdown of smooth solutions to the Müller-Israel-Stewart equations of relativistic viscous fluids
arXiv:2008.03841 · doi:10.1007/s11005-023-01677-9
Abstract
We consider equations of Müller-Israel-Stewart type describing a relativistic viscous fluid with bulk viscosity in four-dimensional Minkowski space. We show that there exists a class of smooth initial data that are localized perturbations of constant states for which the corresponding unique solutions to the Cauchy problem break down in finite time. Specifically, we prove that in finite time such solutions develop a singularity or become unphysical in a sense that we make precise. We also show that in general Riemann invariants do not exist in 1+1 dimensions for physically relevant equations of state and viscosity coefficients. Finally, we present a more general version of a result by Y. Guo and A.S. Tahvildar-Zadeh: we prove large-data singularity formation results for perfect fluids under very general assumptions on the equation of state, allowing any value for the fluid sound speed strictly less than the speed of light.
References in corpus (29)
- Collective flow and viscosity in relativistic heavy-ion collisions
- Global hyperon polarization in nuclear collisions: evidence for the most vortical fluid
- Relativistic viscous hydrodynamics, conformal invariance, and holography
- Derivation of transient relativistic fluid dynamics from the Boltzmann equation
- Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers
- The Bulk Viscosity of High-Temperature QCD
- First-order relativistic hydrodynamics is stable
- Causality and existence of solutions of relativistic viscous fluid dynamics with gravity
- On the importance of viscous dissipation and heat conduction in binary neutron-star mergers
- Nonlinear causality of general first-order relativistic viscous hydrodynamics
- Does Bulk Viscosity Create a Viable Unified Dark Matter Model?
- Transport Coefficients of Bulk Viscous Pressure in the 14-moment approximation
- Stable and causal relativistic Navier-Stokes equations
- General relativistic viscous hydrodynamics of differentially rotating neutron stars
- Causality of the Einstein-Israel-Stewart Theory with Bulk Viscosity
- Effects of bulk viscosity and hadronic rescattering in heavy ion collisions at RHIC and LHC
- On the Deconfinement Phase Transition in Neutron-Star Mergers
- Nonlinear Constraints on Relativistic Fluids Far From Equilibrium
- Gravitational waves from remnant massive neutron stars of binary neutron star merger: Viscous hydrodynamics effects
- Light Rays, Singularities, and All That
- Shock Formation in Small-Data Solutions to Quasilinear Wave Equations: An Overview
- A hyperbolic theory of relativistic conformal dissipative fluids
- Anisotropic Hydrodynamics: Motivation and Methodology
- Remarks on cosmological bulk viscosity in different epochs
- The relativistic Euler equations: Remarkable null structures and regularity properties
- The relativistic Euler equations with a physical vacuum boundary: Hadamard local well-posedness, rough solutions, and continuation criterion
- Remarks on the Einstein-Euler-Entropy system
- Dynamical relativistic liquid bodies
- A priori estimates for a relativistic liquid with free surface boundary
Cited by in corpus (5)
- Recent developments in mathematical aspects of relativistic fluids
- First-Order Viscous Relativistic Hydrodynamics on the Two-Sphere
- Finite-time gradient blow-up and shock formation in Israel-Stewart theory: Bulk, shear, and diffusion regimes
- Nonlinear causality of Israel-Stewart theory with diffusion
- Extending Israel-Stewart theory: Causal bulk viscosity at large gradients