The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 10 curved space wave equations for the components of the space-time metric. A new formulation of constraint-preserving boundary conditions of the Sommerfeld type for such systems has recently been proposed. We implement these boundary conditions in a nonlinear 3D evolution code and test their accuracy
In the harmonic description of general relativity, the principle part of Einstein equations reduces ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
In the harmonic description of general relativity, the principle part of Einstein equations reduces ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
In the harmonic description of general relativity, the principle part of Einstein equations reduces ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
In the harmonic description of general relativity, the principle part of Einstein equations reduces ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
In the harmonic description of general relativity, the principle part of Einstein equations reduces ...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...