Black holes, gravitational waves and fundamental physics: a roadmap
L Barack, V Cardoso, S Nissanke… - … and quantum gravity, 2019 - iopscience.iop.org
70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
The SXS Collaboration catalog of binary black hole simulations
Accurate models of gravitational waves from merging black holes are necessary for
detectors to observe as many events as possible while extracting the maximum science …
detectors to observe as many events as possible while extracting the maximum science …
[HTML][HTML] Continuum and discrete initial-boundary value problems and Einstein's field equations
Many evolution problems in physics are described by partial differential equations on an
infinite domain; therefore, one is interested in the solutions to such problems for a given …
infinite domain; therefore, one is interested in the solutions to such problems for a given …
Ghost instabilities in self-interacting vector fields: The problem with proca fields
Massive vector fields feature in several areas of particle physics, eg, as carriers of weak
interactions, dark matter candidates, or an effective description of photons in a plasma. Here …
interactions, dark matter candidates, or an effective description of photons in a plasma. Here …
Black holes and binary mergers in scalar Gauss-Bonnet gravity: scalar field dynamics
We study the nonlinear dynamics of black holes that carry scalar hair and binaries
composed of such black holes. The scalar hair is due to a linear or exponential coupling …
composed of such black holes. The scalar hair is due to a linear or exponential coupling …
GRChombo: An adaptable numerical relativity code for fundamental physics
GRChombo is an open-source code for performing Numerical Relativity time evolutions,
built on top of the publicly available Chombo software for the solution of PDEs. Whilst …
built on top of the publicly available Chombo software for the solution of PDEs. Whilst …
[LIBRO][B] 3+ 1 formalism in general relativity
E Gourgoulhon - 2012 - Springer
This monograph originates from lectures given at the General Relativity Trimester at the
Institut Henri Poincaré in Paris [1]; at the VII Mexican School on Gravitation and …
Institut Henri Poincaré in Paris [1]; at the VII Mexican School on Gravitation and …
Spin-induced dynamical scalarization, descalarization, and stealthness in scalar-Gauss-Bonnet gravity during a black hole coalescence
Particular couplings between a scalar field and the Gauss-Bonnet invariant lead to
spontaneous scalarization of black holes. Here, we continue our work on simulating this …
spontaneous scalarization of black holes. Here, we continue our work on simulating this …
Template bank for gravitational waveforms from coalescing binary black holes:<? format?> Nonspinning binaries
Gravitational waveforms from the inspiral and ring-down stages of the binary black-hole
coalescences can be modeled accurately by approximation/perturbation techniques in …
coalescences can be modeled accurately by approximation/perturbation techniques in …
3+ 1 formalism and bases of numerical relativity
E Gourgoulhon - arxiv preprint gr-qc/0703035, 2007 - arxiv.org
These lecture notes provide some introduction to the 3+ 1 formalism of general relativity,
which is the foundation of most modern numerical relativity. The text is rather self-contained …
which is the foundation of most modern numerical relativity. The text is rather self-contained …