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 high resolutions. This...
The initial data for black hole collisions are constructed using a conformal-imaging approach and a ...
textThe strongest potential source of gravitational radiation for current and future detectors is t...
This thesis is concerned with the development of better techniques for the 3 + 1 numerical relativit...
We present results of 3D numerical simulations using a finite difference code featuring fixed mesh r...
We demonstrate the flexibility and utility of the Berger-Rigoutsos Adaptive Mesh Refinement (AMR) al...
The use of adaptive mesh refinement (AMR) techniques is crucial for accurate and efficient simulatio...
We have carried out numerical simulations of strongly gravitating systems based on the Einstein equa...
Centered finite volume methods are considered in the context of Numerical Relativity. A specific for...
Various topics in numerical relativity will be discussed, including solving the initial value proble...
I review recent developments in numerical relativity, focussing on progress made in 3D black hole ev...
In this work, we introduce ${\mathtt{GRChombo}}:$ a new numerical relativity code which incorporates...
We describe a generic infrastructure for time evolution simulations in numerical relativity using mu...
We use rigorous techniques from numerical analysis of hyperbolic equations in bounded domains to con...
In order to perform an evolutionary calculation in General Relativity, accurate initial data is need...
New numerical methods have been applied in relativity to obtain a numerical evolution of Einstein eq...
The initial data for black hole collisions are constructed using a conformal-imaging approach and a ...
textThe strongest potential source of gravitational radiation for current and future detectors is t...
This thesis is concerned with the development of better techniques for the 3 + 1 numerical relativit...
We present results of 3D numerical simulations using a finite difference code featuring fixed mesh r...
We demonstrate the flexibility and utility of the Berger-Rigoutsos Adaptive Mesh Refinement (AMR) al...
The use of adaptive mesh refinement (AMR) techniques is crucial for accurate and efficient simulatio...
We have carried out numerical simulations of strongly gravitating systems based on the Einstein equa...
Centered finite volume methods are considered in the context of Numerical Relativity. A specific for...
Various topics in numerical relativity will be discussed, including solving the initial value proble...
I review recent developments in numerical relativity, focussing on progress made in 3D black hole ev...
In this work, we introduce ${\mathtt{GRChombo}}:$ a new numerical relativity code which incorporates...
We describe a generic infrastructure for time evolution simulations in numerical relativity using mu...
We use rigorous techniques from numerical analysis of hyperbolic equations in bounded domains to con...
In order to perform an evolutionary calculation in General Relativity, accurate initial data is need...
New numerical methods have been applied in relativity to obtain a numerical evolution of Einstein eq...
The initial data for black hole collisions are constructed using a conformal-imaging approach and a ...
textThe strongest potential source of gravitational radiation for current and future detectors is t...
This thesis is concerned with the development of better techniques for the 3 + 1 numerical relativit...