THC: a new high-order finite-difference high-resolution shock-capturing code for special-relativistic hydrodynamics
arXiv:1206.6502 · doi:10.1051/0004-6361/201219735
Abstract
We present THC: a new high-order flux-vector-splitting code for Newtonian and special-relativistic hydrodynamics designed for direct numerical simulations of turbulent flows. Our code implements a variety of different reconstruction algorithms, such as the popular weighted essentially non oscillatory and monotonicity-preserving schemes, or the more specialised bandwidth-optimised WENO scheme that has been specifically designed for the study of compressible turbulence. We show the first systematic comparison of these schemes in Newtonian physics as well as for special-relativistic flows. In particular we will present the results obtained in simulations of grid-aligned and oblique shock waves and nonlinear, large-amplitude, smooth adiabatic waves. We will also discuss the results obtained in classical benchmarks such as the double-Mach shock reflection test in Newtonian physics or the linear and nonlinear development of the relativistic Kelvin-Helmholtz instability in two and three dimensions. Finally, we study the turbulent flow induced by the Kelvin-Helmholtz instability and we show that our code is able to obtain well-converged velocity spectra, from which we benchmark the effective resolution of the different schemes.
Updated to match the published version
References in corpus (50)
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- HARM: A Numerical Scheme for General Relativistic Magnetohydrodynamics
- Fundamental differences between SPH and grid methods
- The missing link: Merging neutron stars naturally produce jet-like structures and can power short Gamma-Ray Bursts
- Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole
- Three-dimensional relativistic simulations of rotating neutron-star collapse to a Kerr black hole
- ECHO: an Eulerian Conservative High Order scheme for general relativistic magnetohydrodynamics and magnetodynamics
- Gravitational waves and neutrino emission from the merger of binary neutron stars
- An efficient shock-capturing central-type scheme for multidimensional relativistic flows. II. Magnetohydrodynamics
- Very High Order $\PNM$ Schemes on Unstructured Meshes for the Resistive Relativistic MHD Equations
- The Piecewise Parabolic Method for Multidimensional Relativistic Fluid Dynamics
- Relativistic Magnetohydrodynamics In Dynamical Spacetimes: Numerical Methods And Tests
- WhiskyMHD: a new numerical code for general relativistic magnetohydrodynamics
- Numerical 3+1 general relativistic magnetohydrodynamics: a local characteristic approach
- Tidal effects in binary neutron star coalescence
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- RAM: A Relativistic Adaptive Mesh Refinement Hydrodynamics Code
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- A Well-Posed Kelvin-Helmholtz Instability Test and Comparison
- A five-wave HLL Riemann solver for relativistic MHD
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- Accurate numerical simulations of inspiralling binary neutron stars and their comparison with effective-one-body analytical models
- Can magnetic fields be detected during the inspiral of binary neutron stars?
- A Second Order Godunov Method for Multidimensional Relativistic Magnetohydrodynamics
- Three-Dimensional Relativistic MHD Simulations of the Kelvin-Helmholtz Instability: Magnetic Field Amplification by a Turbulent Dynamo
- General relativistic radiation hydrodynamics of accretion flows. I: Bondi-Hoyle accretion
- Algorithmic comparisons of decaying, isothermal, supersonic turbulence
- Relativistic Radiation Magnetohydrodynamics in Dynamical Spacetimes: Numerical Methods and Tests
- Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms
- Three-Dimensional Simulations of MHD Turbulence Behind Relativistic Shock Waves and Their Implications for GRBs
- Discontinuous Galerkin methods for general-relativistic hydrodynamics: formulation and application to spherically symmetric spacetimes
- Astrophysical turbulence modeling
- Stability of three-dimensional relativistic jets: implications for jet collimation
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- Numerical Simulations of Driven Relativistic MHD Turbulence
- The exact solution of the Riemann problem with non-zero tangential velocities in relativistic hydrodynamics
- Local simulations of the magnetized Kelvin-Helmholtz instability in neutron-star mergers
- An Improved Exact Riemann Solver for Multidimensional Relativistic Flows
- Accurate evolutions of inspiralling neutron-star binaries: assessment of the truncation error
- Conservative, special-relativistic smoothed particle hydrodynamics
- Smoothed Particle Hydrodynamics Simulations of Ultra-Relativistic Shocks with Artificial Viscosity
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- New Relativistic Effects in the Dynamics of Nonlinear Hydrodynamical Waves
- Resonant Kelvin-Helmholtz modes in sheared relativistic flows
- Symmetries, scaling laws and convergence in shearing-box simulations of MRI driven turbulence
- Relativistic MHD and black hole excision: Formulation and initial tests
- Multi-Dimensional Astrophysical Structural and Dynamical Analysis I. Development of a Nonlinear Finite Element Approach
- An Efficient Implementation of Flux Formulae in Multidimensional Relativistic Hydrodynamical Codes
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