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, an...
In order to perform an evolutionary calculation in General Relativity, accurate initial data is need...
We present a new numerical dissipation algorithm, which can be efficiently used in combination with ...
A new numerical scheme to solve the Einstein field equations based upon the generalized harmonic dec...
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...
Various topics in numerical relativity will be discussed, including solving the initial value proble...
We use rigorous techniques from numerical analysis of hyperbolic equations in bounded domains to con...
This thesis is concerned with the development of better techniques for the 3 + 1 numerical relativit...
We describe a generic infrastructure for time evolution simulations in numerical relativity using mu...
We present a detailed study of the effects of mesh refinement boundaries on the convergence and stab...
Centered finite volume methods are considered in the context of Numerical Relativity. A specific for...
This work concerns the evolution of equations of general relativity; their mathematical properties a...
The use of adaptive mesh refinement (AMR) techniques is crucial for accurate and efficient simulatio...
The gauge polyvalence of a new numerical code is tested, both in harmonic-coordinate simulations (ga...
In this work, we introduce ${\mathtt{GRChombo}}:$ a new numerical relativity code which incorporates...
In order to perform an evolutionary calculation in General Relativity, accurate initial data is need...
We present a new numerical dissipation algorithm, which can be efficiently used in combination with ...
A new numerical scheme to solve the Einstein field equations based upon the generalized harmonic dec...
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...
Various topics in numerical relativity will be discussed, including solving the initial value proble...
We use rigorous techniques from numerical analysis of hyperbolic equations in bounded domains to con...
This thesis is concerned with the development of better techniques for the 3 + 1 numerical relativit...
We describe a generic infrastructure for time evolution simulations in numerical relativity using mu...
We present a detailed study of the effects of mesh refinement boundaries on the convergence and stab...
Centered finite volume methods are considered in the context of Numerical Relativity. A specific for...
This work concerns the evolution of equations of general relativity; their mathematical properties a...
The use of adaptive mesh refinement (AMR) techniques is crucial for accurate and efficient simulatio...
The gauge polyvalence of a new numerical code is tested, both in harmonic-coordinate simulations (ga...
In this work, we introduce ${\mathtt{GRChombo}}:$ a new numerical relativity code which incorporates...
In order to perform an evolutionary calculation in General Relativity, accurate initial data is need...
We present a new numerical dissipation algorithm, which can be efficiently used in combination with ...
A new numerical scheme to solve the Einstein field equations based upon the generalized harmonic dec...