Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies
Abstract The standard Λ Cold Dark Matter (ΛCDM) cosmological model provides a good
description of a wide range of astrophysical and cosmological data. However, there are a …
description of a wide range of astrophysical and cosmological data. However, there are a …
Challenges for ΛCDM: An update
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 …
GWTC-3: Compact binary coalescences observed by LIGO and Virgo during the second part of the third observing run
R Abbott, TD Abbott, F Acernese, K Ackley, C Adams… - Physical Review X, 2023 - APS
The third Gravitational-Wave Transient Catalog (GWTC-3) describes signals detected with
Advanced LIGO and Advanced Virgo up to the end of their third observing run. Updating the …
Advanced LIGO and Advanced Virgo up to the end of their third observing run. Updating the …
Population of merging compact binaries inferred using gravitational waves through GWTC-3
R Abbott, TD Abbott, F Acernese, K Ackley, C Adams… - Physical Review X, 2023 - APS
We report on the population properties of compact binary mergers inferred from gravitational-
wave observations of these systems during the first three LIGO-Virgo observing runs. The …
wave observations of these systems during the first three LIGO-Virgo observing runs. 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 …
GW190521: A Binary Black Hole Merger with a Total Mass of
R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley… - Physical review …, 2020 - APS
On May 21, 2019 at 03: 02: 29 UTC Advanced LIGO and Advanced Virgo observed a short
duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise …
duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise …
Astrophysics with the laser interferometer space antenna
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
Quantum gravity phenomenology at the dawn of the multi-messenger era—A review
A Addazi, J Alvarez-Muniz, RA Batista… - Progress in Particle and …, 2022 - Elsevier
The exploration of the universe has recently entered a new era thanks to the multi-
messenger paradigm, characterized by a continuous increase in the quantity and quality of …
messenger paradigm, characterized by a continuous increase in the quantity and quality of …
Tests of general relativity with binary black holes from the second LIGO-Virgo gravitational-wave transient catalog
R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley… - Physical review D, 2021 - APS
Gravitational waves enable tests of general relativity in the highly dynamical and strong-field
regime. Using events detected by LIGO-Virgo up to 1 October 2019, we evaluate the …
regime. Using events detected by LIGO-Virgo up to 1 October 2019, we evaluate the …
Accurate Determination of the Neutron Skin Thickness of through Parity-Violation in Electron Scattering
We report a precision measurement of the parity-violating asymmetry A PV in the elastic
scattering of longitudinally polarized electrons from Pb 208. We measure A PV= 550±16 …
scattering of longitudinally polarized electrons from Pb 208. We measure A PV= 550±16 …