On the well-posedness of relativistic viscous fluids with non-zero vorticity
arXiv:1407.6963 · doi:10.1063/1.4944910
Abstract
We study the problem of coupling Einstein's equations to a relativistic and physically well-motivated version of the Navier-Stokes equations. Under a natural evolution condition for the vorticity, we prove existence and uniqueness in a suitable Gevrey class if the fluid is incompressible, where this condition is given an appropriate relativistic interpretation, and show that the solutions enjoy the finite propagation speed property.
25 pages
References in corpus (9)
- Dissipative collapse of axially symmetric, general relativistic, sources: A general framework and some applications
- Observable primordial vector modes
- A New Approach to Cosmological Bulk Viscosity
- Shear-free axially symmetric dissipative fluids
- Vorticity production through rotation, shear and baroclinicity
- Can cosmological perturbations produce early universe vorticity?
- Viscosity driven instability in rotating relativistic stars
- Vorticity survival in magnetised Friedmann universes
- Shear Dynamics in Higher Dimensional FLRW Cosmology
Cited by in corpus (6)
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- Recent developments in mathematical aspects of relativistic fluids
- Bianchi I cosmology in the presence of a causally regularized viscous fluid
- New symmetry in higher curvature spacetimes
- Symmetry evolution for the imperfect fluid under perturbations