Toward a Consistent Framework for High Order Mesh Refinement Schemes in Numerical Relativity
arXiv:1504.07609 · doi:10.1007/s10714-015-1903-7
Abstract
It has now become customary in the field of numerical relativity to couple high order finite difference schemes to mesh refinement algorithms. To this end, different modifications to the standard Berger-Oliger adaptive mesh refinement algorithm have been proposed. In this work we present a fourth order stable mesh refinement scheme with sub-cycling in time for numerical relativity. We do not use buffer zones to deal with refinement boundaries but explicitly specify boundary data for refined grids. We argue that the incompatibility of the standard mesh refinement algorithm with higher order Runge Kutta methods is a manifestation of order reduction phenomena, caused by inconsistent application of boundary data in the refined grids. Our scheme also addresses the problem of spurious reflections that are generated when propagating waves cross mesh refinement boundaries. We introduce a transition zone on refined levels within which the phase velocity of propagating modes is allowed to decelerate in order to smoothly match the phase velocity of coarser grids. We apply the method to test problems involving propagating waves and show a significant reduction in spurious reflections.
21 pages, 10 figures
References in corpus (15)
- On the Numerical Integration of Einstein's Field Equations
- Evolutions in 3D numerical relativity using fixed mesh refinement
- Calibration of Moving Puncture Simulations
- Accurate black hole evolutions by fourth-order numerical relativity
- High accuracy binary black hole simulations with an extended wave zone
- Reducing phase error in long numerical binary black hole evolutions with sixth order finite differencing
- Binary Black Hole Mergers in 3d Numerical Relativity
- New, efficient, and accurate high order derivative and dissipation operators satisfying summation by parts, and applications in three-dimensional multi-block evolutions
- Stability and collapse of rapidly rotating, supramassive neutron stars: 3D simulations in general relativity
- Implementation of standard testbeds for numerical relativity
- AMR, stability and higher accuracy
- Accuracy Issues for Numerical Waveforms
- Introducing Enzo, an AMR Cosmology Application
- Interface Conditions for Wave Propagation Through Mesh Refinement Boundaries
- Reducing reflections from mesh refinement interfaces in numerical relativity
Cited by in corpus (12)
- Turbulent magnetic field amplification in binary neutron star mergers
- Gravitational Waves from Dark Boson Star binary mergers
- Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: comparing high-resolution and large eddy simulations
- A Simflowny-based finite-difference code for high-performance computing in Relativity
- Large Eddy Simulations of Magnetized Mergers of Neutron Stars with Neutrinos
- Simflowny 3: An upgraded platform for scientific modelling and simulation
- Towards fidelity and scalability in non-vacuum mergers
- Large Eddy Simulations of Magnetized Mergers of Black Holes and Neutron Stars
- AsterX: a new open-source GPU-accelerated GRMHD code for dynamical spacetimes
- Global high-order numerical schemes for the time evolution of the general relativistic radiation magneto-hydrodynamics equations
- On the Hyperbolicity and Stability of Formulations of Metric Gravity
- Impact of magnetic field gradients on the development of the MRI: Applications to binary neutron star mergers and proto-planetary disks