Design of parallel algorithms for Einstein’s equations requires a better understanding of conditions that one can specify at the artificial boundary. The special interest is paid to conditions capable of trading “physical” radiation through the boundary. We propose a new way of constructing boundary conditions and a new way of specifying IBVPs for Einstein Equations using static constrain evolution reductions. Below we give two model problem of constrained evolution. For the first (constrained) problem, a well-posed IBVP is constructed, and a well-posed free evolution problem can be proposed based on the new approach. For the second problem, more investigation is needed to establish existence. Trivial constraint evolution reductions and sta...
The technique of maximally dissipative boundary conditions is applied to establish a simple, well-po...
We analyze Einstein's vacuum field equations in generalized harmonic coordinates on a compact spatia...
Rapid growth of constraints is often observed in free evolutions of highly gravitating systems. To a...
A well-posed initial-boundary value problem is formulated for the model problem of vector wave equat...
In this paper we address the problem of specifying boundary conditions for Einstein's equations when...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
New boundary conditions are constructed and tested numerically for a general first-order form of the...
We show how the use of the normal projection of the Einstein tensor as a set of boundary conditions ...
New boundary conditions are constructed and tested numerically for a general first-order form of the...
In this paper we address the problem of specifying boundary conditions for Einstein\u27s equations w...
AbstractIn this paper, we address the problem of artificial boundary conditions for the symmetric li...
Techniques are developed for projecting the solutions of symmetric-hyperbolic evolution systems onto...
Specifying boundary conditions continues to be a challenge in numerical relativity in order to obtai...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
Computational techniques which establish the stability of an evolution-boundary algorithm for a mode...
The technique of maximally dissipative boundary conditions is applied to establish a simple, well-po...
We analyze Einstein's vacuum field equations in generalized harmonic coordinates on a compact spatia...
Rapid growth of constraints is often observed in free evolutions of highly gravitating systems. To a...
A well-posed initial-boundary value problem is formulated for the model problem of vector wave equat...
In this paper we address the problem of specifying boundary conditions for Einstein's equations when...
We present a set of well-posed constraint-preserving boundary conditions for a first-order in time, ...
New boundary conditions are constructed and tested numerically for a general first-order form of the...
We show how the use of the normal projection of the Einstein tensor as a set of boundary conditions ...
New boundary conditions are constructed and tested numerically for a general first-order form of the...
In this paper we address the problem of specifying boundary conditions for Einstein\u27s equations w...
AbstractIn this paper, we address the problem of artificial boundary conditions for the symmetric li...
Techniques are developed for projecting the solutions of symmetric-hyperbolic evolution systems onto...
Specifying boundary conditions continues to be a challenge in numerical relativity in order to obtai...
The principle part of Einstein equations in the harmonic gauge consists of a constrained system of 1...
Computational techniques which establish the stability of an evolution-boundary algorithm for a mode...
The technique of maximally dissipative boundary conditions is applied to establish a simple, well-po...
We analyze Einstein's vacuum field equations in generalized harmonic coordinates on a compact spatia...
Rapid growth of constraints is often observed in free evolutions of highly gravitating systems. To a...