Numerical simulations of divergence-type theories for conformal dissipative fluids
arXiv:2304.08584 · doi:10.1103/PhysRevD.107.103041
Abstract
We present the first numerical simulations of the symmetric--hyperbolic theory for conformal dissipative relativistic fluids developed in [1]. In this theory, the information of the fluid dynamics is encoded in a scalar generating function which depends on three free parameters. By adapting the WENO-Z high-resolution shock-capturing central scheme, we show numerical solutions restricted to planar symmetry in Minkowski spacetime, from two qualitatively different initial data: a smooth bump and a discontinuous step. We perform a detailed exploration of the effect of the different parameters of the theory, and numerically assess the constitutive relations associated with the shear viscosity by analyzing the entropy production rate when shocks are produced.
22 pages, 14 figures
References in corpus (10)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Observation of gravitational waves from two neutron star-black hole coalescences
- THC: a new high-order finite-difference high-resolution shock-capturing code for special-relativistic hydrodynamics
- Relativistic hydrodynamics for heavy-ion collisions
- Discontinuous Galerkin methods for general-relativistic hydrodynamics: formulation and application to spherically symmetric spacetimes
- Behaviour of dissipative accretion flows around black holes
- A hyperbolic theory of relativistic conformal dissipative fluids
- Heavy quark collisional energy loss in the quark-gluon plasma including finite relaxation time
- High-energy heavy-ions physics: from RHIC to LHC
- Steady asymptotic equilibria in conformal relativistic fluids