Accès ouvert
2023
article
OpenAlex
R Abbott, H Abe, F Acernese, K Ackley et autres
ABSTRACT We describe a search for gravitational waves from compact binaries with at least one component with mass $0.2$–$1.0 \, \mathrm{M}_\odot$ and mass ratio q ≥ 0.1 in Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) and Advanced Virgo data collected between 2019 November …
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Accès ouvert
2022
article
OpenAlex
R. Abbott, H. Abe, F. Acernese, K. Ackley et autres
This paper describes the first all-sky search for long-duration, quasimonochromatic gravitational-wave signals emitted by ultralight scalar boson clouds around spinning black holes using data from the third observing run of Advanced LIGO. We analyze the frequency range from 20 to 610 Hz, …
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Accès ouvert
2022
article
OpenAlex
R. Abbott, T. D. Abbott, F. Acernese, K. Ackley et autres
We present a search for dark photon dark matter that could couple to gravitational-wave interferometers using data from Advanced LIGO and Virgo's third observing run. To perform this analysis, we use two methods, one based on cross-correlation of the strain channels in …
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Accès ouvert
2021
preprint
OpenAlex
The LIGO Scientific Collaboration, the KAGRA Collaboration, R. Abbott, H. Abe et autres
This paper describes the first all-sky search for long-duration, quasi-monochromatic gravitational-wave signals emitted by ultralight scalar boson clouds around spinning black holes using data from the third observing run of Advanced LIGO. We analyze the frequency range from 20~Hz to 610~Hz, over …
Accès ouvert
2021
preprint
OpenAlex
The LIGO Scientific Collaboration, the KAGRA Collaboration, R. Abbott, H. Abe et autres
We use 47 gravitational-wave sources from the Third LIGO-Virgo-KAGRA Gravitational-Wave Transient Catalog (GWTC-3) to estimate the Hubble parameter $H(z)$, including its current value, the Hubble constant $H_0$. Each gravitational-wave (GW) signal provides the luminosity distance to the source and we estimate the …
Accès ouvert
2021
article
OpenAlex
LIGO Scientific and Virgo Collaboration, KAGRA Collaboration, the KAGRA Collaboration, R. Abbott et autres
After the detection of gravitational waves from compact binary coalescences, the search for transient gravitational-wave signals with less well-defined waveforms for which matched filtering is not well-suited is one of the frontiers for gravitational-wave astronomy. Broadly classified into "short" $ \lesssim 1~$\,s …
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