Add to ORKGA numerical relativity code designed to evolve rotating axisymmetric spacetimes is constructed. Both polarization states of gravitational radiation can be tracked. The source of the gravitational field is chosen to be a configuration of collisionless particles. The code is used to evaluate the stability of polytropic and toroidal star clusters. The formation of Kerr black holes by the collapse of unstable clusters is demonstrated. Unstable clusters with J/(M^2) 1 collapse to new equilibrium configurations
We present a new three-dimensional fully general-relativistic hydrodynamics code using high-resoluti...
In this thesis I consider three different projects in numerical relativity. The first one is a study...
This is the second in a series of papers on the construction and validation of a three-dimensional c...
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...
The radial collapse of a homogeneous disk of collisionless particles can be solved analytically in N...
We present preliminary results in our long-term project of studying the evolution of matter in a dyn...
The radial collapse of a homogeneous disk of collisionless particles can be solved analytically in N...
We perform numerical simulations of head-on collisions of relativistic clusters. The cluster particl...
We perform numerical simulations of head-on collisions of relativistic clusters. The cluster particl...
We describe an axisymmetric general relativistic code for rotational core collapse. The code evolves...
We describe an axisymmetric general relativistic code for rotational core collapse. The code evolves...
We have developed a numerical code to study the evolution of self-gravitating matter in dynamic blac...
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...
We present a new three-dimensional fully general-relativistic hydrodynamics code using high-resoluti...
In this thesis I consider three different projects in numerical relativity. The first one is a study...
This is the second in a series of papers on the construction and validation of a three-dimensional c...
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...
The radial collapse of a homogeneous disk of collisionless particles can be solved analytically in N...
We present preliminary results in our long-term project of studying the evolution of matter in a dyn...
The radial collapse of a homogeneous disk of collisionless particles can be solved analytically in N...
We perform numerical simulations of head-on collisions of relativistic clusters. The cluster particl...
We perform numerical simulations of head-on collisions of relativistic clusters. The cluster particl...
We describe an axisymmetric general relativistic code for rotational core collapse. The code evolves...
We describe an axisymmetric general relativistic code for rotational core collapse. The code evolves...
We have developed a numerical code to study the evolution of self-gravitating matter in dynamic blac...
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...
We present a new three-dimensional fully general-relativistic hydrodynamics code using high-resoluti...
In this thesis I consider three different projects in numerical relativity. The first one is a study...
This is the second in a series of papers on the construction and validation of a three-dimensional c...