Evolutions in 3D numerical relativity using fixed mesh refinement
arXiv:gr-qc/0310042 · doi:10.1088/0264-9381/21/6/014
Abstract
We present results of 3D numerical simulations using a finite difference code featuring fixed mesh refinement (FMR), in which a subset of the computational domain is refined in space and time. We apply this code to a series of test cases including a robust stability test, a nonlinear gauge wave and an excised Schwarzschild black hole in an evolving gauge. We find that the mesh refinement results are comparable in accuracy, stability and convergence to unigrid simulations with the same effective resolution. At the same time, the use of FMR reduces the computational resources needed to obtain a given accuracy. Particular care must be taken at the interfaces between coarse and fine grids to avoid a loss of convergence at higher resolutions, and we introduce the use of "buffer zones" as one resolution of this issue. We also introduce a new method for initial data generation, which enables higher-order interpolation in time even from the initial time slice. This FMR system, "Carpet", is a driver module in the freely available Cactus computational infrastructure, and is able to endow generic existing Cactus simulation modules ("thorns") with FMR with little or no extra effort.
20 pages, 15 figures; published version, but with colour figures
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- Piercing of a solitonic boson star by a black hole
- Diffusivity in force-free simulations of global magnetospheres
- Bowen-York Type Initial Data for Binaries with Neutron Stars
- A Toy Model for the Electromagnetic Output of Neutron-star Merger Prompt Collapse to a Black Hole: Magnetized Neutron-star Collisions
- Fully general relativistic simulations of rapidly rotating quark stars: Oscillation modes and universal relations
- Secular Outflows from Long-Lived Neutron Star Merger Remnants
- Investigating the migration of immiscible contaminant fluid flow in homogeneous and heterogeneous aquifers with high-precision numerical simulations
- Problematic systematics in neutron-star merger simulations
- Gravitational wave extraction in higher dimensional numerical relativity using the Weyl tensor
- Relativistic gas accretion onto supermassive black Hole binaries from inspiral through merger
- Falloff of the Weyl scalars in binary black hole spacetimes
- Revealing Phase Transition in Dense Matter with Gravitational Wave Spectroscopy of Binary Neutron Star Mergers
- Black hole pulsars and monster shocks as outcomes of black hole--neutron star mergers
- Exploring the Phase Diagram of V-QCD with Neutron Star Merger Simulations
- Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms
- Boson star superradiance with spinning effects and in time domain
- Spin induction from scattering of two spinning black holes in dense clusters
- Force-free wave interaction in magnetar magnetospheres: Computational modeling in axisymmetry
- The Nonlinear Sigma Model With Distributed Adaptive Mesh Refinement
- Exploring pathways to forming twin stars
- Component Specification in the Cactus Framework: The Cactus Configuration Language
- General Relativistic Simulations of High-Mass Binary Neutron Star Mergers: rapid formation of low-mass stellar black holes
- Self-gravitating disks around rapidly spinning, tilted black holes: General relativistic simulations
- Kicks in charged black hole binaries
- Testing the Boundary-to-Bound Correspondence with Numerical Relativity
- Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers
- Inside the Final Black Hole: Puncture and Trapped Surface Dynamics
- Topology change and emergent scale symmetry in compact star matter via gravitational wave detection
- Optimizing the Placement of Numerical Relativity Simulations using a Mismatch Predicting Neural Network
- Evolution of jets driven by relativistic radiation hydrodynamics as Long and Low Luminosity GRBs
- Adapted gauge to a quasilocal measure of the black holes recoil
- Electrodynamics and dissipation in the binary magnetosphere of pre-merger neutron stars
- Neutron-quark stars: Discerning viable alternatives for the higher-density part of the equation of state of compact stars
- Characterizing the effect of eccentricity on the dynamics of binary black hole mergers in numerical relativity
- Computational General Relativistic Force-Free Electrodynamics: I. Multi-Coordinate Implementation and Testing
- Structure formation and quasi-spherical collapse from initial curvature perturbations with numerical relativity simulations
- Exploring the Use of Numerical Relativity Waveforms in Burst Analysis of Precessing Black Hole Mergers
- Orbiting black-hole binaries and apparent horizons in higher dimensions
- Probing the Binary Black Hole Merger Regime with Scalar Perturbations
- Geometric horizons in binary black hole mergers
- Effect of magnetic fields on the dynamics and gravitational wave emission of PPI-saturated self-gravitating accretion disks: simulations in full GR
- Impact of Neutrino Flavor Conversions on Neutron Star Merger Dynamics, Ejecta, Nucleosynthesis, and Multi-Messenger Signals
- A complete waveform comparison of post-Newtonian and numerical relativity in eccentric orbits
- Can quasi-circular mergers of charged black holes produce extremal black holes?
- Stability and collisions of excited spherical boson stars: glimpses of chains and rings
- Comparing an analytical spacetime metric for a merging binary to a fully nonlinear numerical evolution using curvature scalars
- Spin-up and mass-gain in hyperbolic encounters of spinning black holes
- Inspiraling black-hole binary spacetimes: Challenges in transitioning from analytical to numerical techniques
- Insights into Binary Neutron Star Merger Simulations: A Multi-Code Comparison
- Splitting the Gravitational Atom: Instabilities of Black Holes with Synchronized or Resonant Hair
- General relativistic hydrodynamic simulations of binary strange star mergers
- Fixed mesh refinement in the characteristic formulation of General Relativity
- Investigating Binary Black Hole Mergers with Principal Component Analysis
- -mode oscillations of compact stars with realistic equations of state in dynamical spacetime
- Neutron Star Mergers and the Quark Matter Equation of State
- Curvature and dynamical spacetimes: can we peer into the quantum regime?
- Effects of dynamical capture on two equal-mass nonspinning black holes
- Effect of spin in binary neutron star mergers
- Three little pieces for computer and relativity
- Safety first: Stability and dissipation of line-tied force-free flux tubes in magnetized coronae
- Fully general-relativistic simulations of isolated and binary strange quark stars
- Binary black holes gone MAD: Magnetically arrested minidisks around nonspinning black holes
- Rapidly Rotating Neutron Star Collapse in Massive Scalar-Tensor Theories
- Nyquist-resolving gravitational waves via orbital frequency-based refinement
- BHaHAHA: A Fast, Robust Apparent Horizon Finder Library for Numerical Relativity
- Impact of ultralight bosonic dark matter on the dynamical bar-mode instability of rotating neutron stars
- Holography in Quark-Gluon Plasma and Neutron Stars
- Signatures of deconfined quark phases in binary neutron star mergers
- superB/NRPy: Scalable, Task-Based Numerical Relativity for 3G Gravitational Wave Science
- General Relativistic Stability and Gravitational Wave Content of Rotating Triaxial Neutron Stars
- A User-Friendly Python Interface for the Numerical Relativity Code AMSS-NCKU
- Propagation of a realistic magnetar jet through binary neutron star merger medium and implications for short gamma-ray bursts
- Misaligned Spinning Binary Black Hole Mergers in Hot Magnetized Plasma
- Piercing of a boson star by a black hole
- Persistence of post-Newtonian amplitude structure in binary black hole mergers
- Aliasing Instabilities in the Numerical Evolution of the Einstein Field Equations
- A New Moment-Based General-Relativistic Neutrino-Radiation Transport Code: Methods and First Applications to Neutron Star Mergers
- The Fourth RIT binary black hole simulations catalog: Extension to Eccentric Orbits
- Multimessenger Signatures of Tilted, Self-Gravitating, Black Hole Disks