Cosmology with the laser interferometer space antenna
Abstract The Laser Interferometer Space Antenna (LISA) has two scientific objectives of
cosmological focus: to probe the expansion rate of the universe, and to understand …
cosmological focus: to probe the expansion rate of the universe, and to understand …
Challenges for ΛCDM: An update
L Perivolaropoulos, F Skara - New Astronomy Reviews, 2022 - Elsevier
A number of challenges to the standard Λ CDM model have been emerging during the past
few years as the accuracy of cosmological observations improves. In this review we discuss …
few years as the accuracy of cosmological observations improves. In this review we discuss …
Science with the Einstein Telescope: a comparison of different designs
M Branchesi, M Maggiore, D Alonso… - … of Cosmology and …, 2023 - iopscience.iop.org
Abstract The Einstein Telescope (ET), the European project for a third-generation
gravitational-wave detector, has a reference configuration based on a triangular shape …
gravitational-wave detector, has a reference configuration based on a triangular shape …
[HTML][HTML] Observation of gravitational waves from two neutron star–black hole coalescences
R Abbott, TD Abbott, S Abraham… - The Astrophysical …, 2021 - iopscience.iop.org
New horizons for fundamental physics with LISA
KG Arun, E Belgacem, R Benkel, L Bernard… - Living Reviews in …, 2022 - Springer
Abstract The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders
about the fundamental theory of nature at play in the extreme gravity regime, where the …
about the fundamental theory of nature at play in the extreme gravity regime, where the …
The H0 Olympics: A fair ranking of proposed models
N Schöneberg, GF Abellán, AP Sánchez, SJ Witte… - Physics Reports, 2022 - Elsevier
Despite the remarkable success of the Λ Cold Dark Matter (Λ CDM) cosmological model, a
growing discrepancy has emerged (currently measured at the level of∼ 4− 6 σ) between the …
growing discrepancy has emerged (currently measured at the level of∼ 4− 6 σ) between the …
GWTC-2: compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run
R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley… - Physical Review X, 2021 - APS
We report on gravitational-wave discoveries from compact binary coalescences detected by
Advanced LIGO and Advanced Virgo in the first half of the third observing run (O3a) between …
Advanced LIGO and Advanced Virgo in the first half of the third observing run (O3a) between …
The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023
We review the current status of Early Dark Energy (EDE) models proposed to resolve the
“Hubble tension”, the discrepancy between “direct” measurements of the current expansion …
“Hubble tension”, the discrepancy between “direct” measurements of the current expansion …
Gravitational-wave physics and astronomy in the 2020s and 2030s
The 100 years since the publication of Albert Einstein's theory of general relativity saw
significant development of the understanding of the theory, the identification of potential …
significant development of the understanding of the theory, the identification of potential …
Constraints on the cosmic expansion history from GWTC-3
R Abbott, H Abe, F Acernese, K Ackley… - Astrophysical …, 2023 - iopscience.iop.org
The discovery of a gravitational wave (GW) signal from a binary neutron star (BNS) merger
(Abbott et al. 2017a) and the kilonova emission from its remnant (Coulter et al. 2017; Abbott …
(Abbott et al. 2017a) and the kilonova emission from its remnant (Coulter et al. 2017; Abbott …