On the convexity of Relativistic Hydrodynamics
arXiv:1302.3758 · doi:10.1088/0264-9381/30/5/057002
Abstract
The relativistic hydrodynamic system of equations for a perfect fluid obeying a causal equation of state is hyperbolic (Anile 1989 {\it Relativistic Fluids and Magneto-Fluids} (Cambridge: Cambridge University Press)). In this report, we derive the conditions for this system to be convex in terms of the fundamental derivative of the equation of state (Menikoff and Plohr 1989 {\it Rev. Mod. Phys.} {\bf 61} 75). The classical limit is recovered.
10 pages
Cited by in corpus (9)
- Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
- The internal structure of overpressured, magnetized, relativistic jets
- Neutron star collapse and gravitational waves with a non-convex equation of state
- A new scheme of causal viscous hydrodynamics for relativistic heavy-ion collisions: A Riemann solver for quark-gluon plasma
- On the relativistic compressibility conditions
- Gravitational-wave imprints of non-convex dynamics in binary neutron star mergers
- Anomalous dynamics triggered by a non-convex equation of state in relativistic flows
- On the convexity of Relativistic Ideal Magnetohydrodynamics
- One- and two-argument equation of state parametrizations with continuous sound speed for neutron star simulations