We present preliminary results in our long-term project of studying the evolution of matter in a dynamical spacetime. To achieve this, we have developed a new code to evolve axisymmetric initial data sets corresponding to a black hole surrounded by matter fields. The code is based on the coupling of two previously existing codes. The matter fields are evolved with a 2D shock-capturing method which uses the characteristic information of the GR hydro equations to build up a linearized Riemann solver. The spacetime is evolved with a 2D ADM code designed to evolve a wormhole in full general relativity. An example of the kind of problems we are currently investigating is the on axis collision of a star with a black hole
We present a new class of 3D black hole initial data sets for numerical relativity. These data sets ...
We present a new class of 3D black hole initial data sets for numerical relativity. These data sets ...
We have constructed a numerical code that finds black hole event horizons in an axisymmetric rotatin...
We present preliminary results in our long-term project of studying the evolution of matter in a dyn...
We have developed a numerical code to study the evolution of self-gravitating matter in dynamic blac...
We have developed a numerical code to study the evolution of self-gravitating matter in dynamic blac...
We have developed a numerical code to study the evolution of self-gravitating matter in dynamic blac...
We describe the first axisymmetric numerical code based on the generalized harmonic formulation of t...
We present results from numerical evolutions of vacuum black hole spacetimes in 3D Cartesian coordin...
We describe a grid generation procedure designed to construct new classes of orthogonal coordinate s...
In this thesis I consider three different projects in numerical relativity. The first one is a study...
We have constructed a numerical code that finds black hole event horizons in an axisymmetric rotatin...
We have constructed a numerical code that finds black hole event horizons in an axisymmetric rotatin...
A numerical relativity code designed to evolve rotating axisymmetric spacetimes is constructed. Both...
A numerical relativity code designed to evolve rotating axisymmetric spacetimes is constructed. Both...
We present a new class of 3D black hole initial data sets for numerical relativity. These data sets ...
We present a new class of 3D black hole initial data sets for numerical relativity. These data sets ...
We have constructed a numerical code that finds black hole event horizons in an axisymmetric rotatin...
We present preliminary results in our long-term project of studying the evolution of matter in a dyn...
We have developed a numerical code to study the evolution of self-gravitating matter in dynamic blac...
We have developed a numerical code to study the evolution of self-gravitating matter in dynamic blac...
We have developed a numerical code to study the evolution of self-gravitating matter in dynamic blac...
We describe the first axisymmetric numerical code based on the generalized harmonic formulation of t...
We present results from numerical evolutions of vacuum black hole spacetimes in 3D Cartesian coordin...
We describe a grid generation procedure designed to construct new classes of orthogonal coordinate s...
In this thesis I consider three different projects in numerical relativity. The first one is a study...
We have constructed a numerical code that finds black hole event horizons in an axisymmetric rotatin...
We have constructed a numerical code that finds black hole event horizons in an axisymmetric rotatin...
A numerical relativity code designed to evolve rotating axisymmetric spacetimes is constructed. Both...
A numerical relativity code designed to evolve rotating axisymmetric spacetimes is constructed. Both...
We present a new class of 3D black hole initial data sets for numerical relativity. These data sets ...
We present a new class of 3D black hole initial data sets for numerical relativity. These data sets ...
We have constructed a numerical code that finds black hole event horizons in an axisymmetric rotatin...