Initial data in numerical relativity. The constraints are formulated as elliptic equations, parabolic equations and strongly hyperbolic equations. This presentation is about a different approach to initial data for black holes, the strongly hyperbolic method
This thesis is concerned with the development of better techniques for the 3 + 1 numerical relativit...
We discuss several closely connected open questions central to Numerical Relativity. These involve ...
textBinary black hole mergers are the strongest expected producers of graviational radiation in the...
We describe a numerical code that solves Einstein’s equations for a Schwarzschild black hole in sphe...
We describe a numerical code that solves Einstein’s equations for a Schwarzschild black hole in sphe...
We use rigorous techniques from numerical analysis of hyperbolic equations in bounded domains to con...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutor: ...
Construction of binary black hole initial data is a prerequisite for numerical evolutions of binary ...
Construction of binary black hole initial data is a prerequisite for numerical evolutions of binary ...
We present a new many-parameter family of hyperbolic representations of Einstein’s equations, which ...
We present a new many-parameter family of hyperbolic representations of Einstein’s equations, which ...
We solve the elliptic equations associated with the Hamiltonian and momentum constraints, correspond...
Various topics in numerical relativity will be discussed, including solving the initial value proble...
We present a new class of 3D black hole initial data sets for numerical relativity. These data sets ...
This thesis is concerned with the development of better techniques for the 3 + 1 numerical relativit...
This thesis is concerned with the development of better techniques for the 3 + 1 numerical relativit...
We discuss several closely connected open questions central to Numerical Relativity. These involve ...
textBinary black hole mergers are the strongest expected producers of graviational radiation in the...
We describe a numerical code that solves Einstein’s equations for a Schwarzschild black hole in sphe...
We describe a numerical code that solves Einstein’s equations for a Schwarzschild black hole in sphe...
We use rigorous techniques from numerical analysis of hyperbolic equations in bounded domains to con...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutor: ...
Construction of binary black hole initial data is a prerequisite for numerical evolutions of binary ...
Construction of binary black hole initial data is a prerequisite for numerical evolutions of binary ...
We present a new many-parameter family of hyperbolic representations of Einstein’s equations, which ...
We present a new many-parameter family of hyperbolic representations of Einstein’s equations, which ...
We solve the elliptic equations associated with the Hamiltonian and momentum constraints, correspond...
Various topics in numerical relativity will be discussed, including solving the initial value proble...
We present a new class of 3D black hole initial data sets for numerical relativity. These data sets ...
This thesis is concerned with the development of better techniques for the 3 + 1 numerical relativit...
This thesis is concerned with the development of better techniques for the 3 + 1 numerical relativit...
We discuss several closely connected open questions central to Numerical Relativity. These involve ...
textBinary black hole mergers are the strongest expected producers of graviational radiation in the...