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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 …
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
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 …
GWTC-1: a gravitational-wave transient catalog of compact binary mergers observed by LIGO and Virgo during the first and second observing runs
BP Abbott, R Abbott, TD Abbott, S Abraham… - Physical Review X, 2019 - APS
We present the results from three gravitational-wave searches for coalescing compact
binaries with component masses above 1 M⊙ during the first and second observing runs of …
binaries with component masses above 1 M⊙ during the first and second observing runs of …
GW170104: observation of a 50-solar-mass binary black hole coalescence at redshift 0.2
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley… - Physical review …, 2017 - APS
We describe the observation of GW170104, a gravitational-wave signal produced by the
coalescence of a pair of stellar-mass black holes. The signal was measured on January 4 …
coalescence of a pair of stellar-mass black holes. The signal was measured on January 4 …
GW170814: a three-detector observation of gravitational waves from a binary black hole coalescence
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley… - Physical review …, 2017 - APS
On August 14, 2017 at 10∶ 30: 43 UTC, the Advanced Virgo detector and the two Advanced
LIGO detectors coherently observed a transient gravitational-wave signal produced by the …
LIGO detectors coherently observed a transient gravitational-wave signal produced by the …
Binary black hole mergers in the first advanced LIGO observing run
BP Abbott, R Abbott, TD Abbott, MR Abernathy… - Physical Review X, 2016 - APS
The first observational run of the Advanced LIGO detectors, from September 12, 2015 to
January 19, 2016, saw the first detections of gravitational waves from binary black hole …
January 19, 2016, saw the first detections of gravitational waves from binary black hole …
Rates of compact object coalescences
Gravitational-wave detections are enabling measurements of the rate of coalescences of
binaries composed of two compact objects—neutron stars and/or black holes. The …
binaries composed of two compact objects—neutron stars and/or black holes. The …
The chemically homogeneous evolutionary channel for binary black hole mergers: rates and properties of gravitational-wave events detectable by advanced LIGO
We explore the predictions for detectable gravitational-wave signals from merging binary
black holes formed through chemically homogeneous evolution in massive short-period …
black holes formed through chemically homogeneous evolution in massive short-period …
Observational evidence for intermediate-mass black holes
M Mezcua - International Journal of Modern Physics D, 2017 - World Scientific
Intermediate-mass black holes (IMBHs), with masses in the range 1 0 0–1 0 6 M⊙, are the
link between stellar-mass BHs and supermassive BHs (SMBHs). They are thought to be the …
link between stellar-mass BHs and supermassive BHs (SMBHs). They are thought to be the …