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
General relativity and cosmology: Unsolved questions and future directions
For the last 100 years, General Relativity (GR) has taken over the gravitational theory mantle
held by Newtonian Gravity for the previous 200 years. This article reviews the status of GR in …
held by Newtonian Gravity for the previous 200 years. This article reviews the status of GR in …
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 …
gevolution: a cosmological N-body code based on General Relativity
J Adamek, D Daverio, R Durrer… - Journal of Cosmology and …, 2016 - iopscience.iop.org
We present a new N-body code, gevolution, for the evolution of large scale structure in the
Universe. Our code is based on a weak field expansion of General Relativity and calculates …
Universe. Our code is based on a weak field expansion of General Relativity and calculates …
Lessons for adaptive mesh refinement in numerical relativity
M Radia, U Sperhake, A Drew, K Clough… - … and Quantum Gravity, 2022 - iopscience.iop.org
We demonstrate the flexibility and utility of the Berger–Rigoutsos adaptive mesh refinement
(AMR) algorithm used in the open-source numerical relativity (NR) code GRC hombo for …
(AMR) algorithm used in the open-source numerical relativity (NR) code GRC hombo for …
Effects of nonlinear inhomogeneity on the cosmic expansion with numerical relativity
E Bentivegna, M Bruni - Physical review letters, 2016 - APS
We construct a three-dimensional, fully relativistic numerical model of a universe filled with
an inhomogeneous pressureless fluid, starting from initial data that represent a perturbation …
an inhomogeneous pressureless fluid, starting from initial data that represent a perturbation …
CTTK: a new method to solve the initial data constraints in numerical relativity
JC Aurrekoetxea, K Clough… - Classical and Quantum …, 2023 - iopscience.iop.org
In numerical relativity simulations with non-trivial matter configurations, one must solve the
Hamiltonian and momentum constraints of the ADM formulation for the metric variables in …
Hamiltonian and momentum constraints of the ADM formulation for the metric variables in …
Emerging spatial curvature can resolve the tension between high-redshift CMB and low-redshift distance ladder measurements of the Hubble constant
K Bolejko - Physical Review D, 2018 - APS
The measurements of the Hubble constant reveal a tension between high-redshift (CMB)
and low-redshift (distance ladder) constraints. So far neither observational systematics nor …
and low-redshift (distance ladder) constraints. So far neither observational systematics nor …
Einstein's Universe: Cosmological structure formation in numerical relativity
We perform large-scale cosmological simulations that solve Einstein's equations directly via
numerical relativity. Starting with initial conditions sampled from the cosmic microwave …
numerical relativity. Starting with initial conditions sampled from the cosmic microwave …
Backreaction in cosmology
S Schander, T Thiemann - Frontiers in Astronomy and Space …, 2021 - frontiersin.org
In this review, we investigate the question of backreaction in different approaches to
cosmological perturbation theory, and with a special focus on quantum theoretical aspects …
cosmological perturbation theory, and with a special focus on quantum theoretical aspects …