GRChombo : Numerical relativity with adaptive mesh refinement
From MaRDI portal
Publication:2788981
DOI10.1088/0264-9381/32/24/245011zbMath1331.83003arXiv1503.03436OpenAlexW3104129920MaRDI QIDQ2788981
Katy Clough, Hal Finkel, Markus Kunesch, Eugene A. Lim, Saran Tunyasuvunakool, Pau Figueras
Publication date: 23 February 2016
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1503.03436
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Computational methods for problems pertaining to relativity and gravitational theory (83-08)
Related Items (23)
CTTK: a new method to solve the initial data constraints in numerical relativity ⋮ Local continuity of angular momentum and noether charge for matter in general relativity ⋮ Malaise and remedy of binary boson-star initial data ⋮ The effects of potential shape on inhomogeneous inflation ⋮ Axions from strings: the attractive solution ⋮ Primordial black hole formation with full numerical relativity ⋮ Numerical Relativity and the Discovery of Gravitational Waves ⋮ One-loop gravitational bremsstrahlung and waveforms from a heavy-mass effective field theory ⋮ Coherent gravitational waveforms and memory from cosmic string loops ⋮ Gravitational collapse in cubic Horndeski theories ⋮ A spectral method algorithm for numerical simulations of gravitational fields ⋮ Level-by-level artificial viscosity and visualization for MHD simulation with adaptive mesh refinement ⋮ Application of local discontinuous Galerkin method to Einstein equations ⋮ Full 3D numerical relativity simulations of neutron star–boson star collisions with BAM ⋮ Aliasing instabilities in the numerical evolution of the Einstein field equations ⋮ GRChombo ⋮ Evidence for violations of weak cosmic censorship in black hole collisions in higher dimensions ⋮ Lessons for adaptive mesh refinement in numerical relativity ⋮ Robustness of inflation to inhomogeneous initial conditions ⋮ The role of fluctuation-dissipation dynamics in setting initial conditions for inflation ⋮ The new discontinuous Galerkin methods based numerical relativity program Nmesh ⋮ The fate of dense scalar stars ⋮ Oscillon collapse to black holes
Uses Software
Cites Work
- Unnamed Item
- Numerical solution of gravitational dynamics in asymptotically anti-de Sitter spacetimes
- A multidomain spectral method for solving elliptic equations
- Adaptive mesh refinement for hyperbolic partial differential equations
- Local adaptive mesh refinement for shock hydrodynamics
- The large-\(N\) limit of superconformal field theories and supergravity
- Critical collapse of scalar fields beyond axisymmetry
- An instability of higher-dimensional rotating black holes
- Decay Properties of Klein-Gordon Fields on Kerr-AdS Spacetimes
- Black Holes in Higher Dimensions
- Critical collapse of the massless scalar field in axisymmetry
- On critical collapse of gravitational waves
- Evolution of three-dimensional gravitational waves: Harmonic slicing case
- Numerical integration of Einstein’s field equations
- Fully Covariant and Conformal Formulation of the Z4 System Compared to the BSSN Formulation in Spherical Symmetry
- Implementation of standard testbeds for numerical relativity
- Evolutions in 3D numerical relativity using fixed mesh refinement
- A fast apparent horizon finder for three-dimensional Cartesian grids in numerical relativity
- Black strings andp-branes are unstable
- Introduction to 3+1 Numerical Relativity
- Constraint damping in the Z4 formulation and harmonic gauge
- Black holes in higher dimensions
- Critical phenomena in gravitational collapse
This page was built for publication: GRChombo : Numerical relativity with adaptive mesh refinement