Results 31 to 40 of about 18,093 (220)

The status of LIGO [PDF]

open access: yesAIP Conference Proceedings, 2000
<p>Published - <a href="/records/6nf4n-1p296/files/COLaipcp00.pdf?download=1">COLaipcp00.pdf</a></p>
openaire   +2 more sources

A Search for Gravitational Waves from Perturbed Black Hole Ringdowns in LIGO Data [PDF]

open access: yes, 2008
According to General Relativity a perturbed black hole will return to a stable configuration by the emission of gravitational radiation in a superposition of quasi-normal modes. Such a perturbation will occur due to the coalescence of a black hole binary,
Goggin, Lisa Maria
core   +1 more source

Search for gravitational-wave bursts in LIGO data from the fourth science run [PDF]

open access: yes, 2007
The fourth science run of the LIGO and GEO 600 gravitational-wave detectors, carried out in early 2005, collected data with significantly lower noise than previous science runs.
Abbott, B.   +4 more
core   +2 more sources

Tests of General Relativity with Binary Black Holes from the second LIGO–Virgo Gravitational-Wave Transient Catalog - Full Posterior Sample Data Release

open access: yes, 2021
Data release containing full posterior samples of the following analyses reported in the paper "Tests of General Relativity with Binary Black Holes from the second LIGO–Virgo Gravitational-Wave Transient Catalog" from the LIGO Scientific Collaboration ...
LIGO Scientific Collaboration and Virgo Collaboration
core   +1 more source

LIGO’s “science reach” [PDF]

open access: yesAIP Conference Proceedings, 2001
Technical discussions of the Laser Interferometer Gravitational Wave Observatory (LIGO) sensitivity often focus on its effective sensitivity to gravitational waves in a given band; nevertheless, the goal of the LIGO Project is to ``do science.'' Exploiting this new observational perspective to explore the Universe is a long-term goal, toward which LIGO'
openaire   +2 more sources

Broadband Quantum Enhancement of the LIGO Detectors with Frequency-Dependent Squeezing

open access: yesPhysical Review X, 2023
Quantum noise imposes a fundamental limitation on the sensitivity of interferometric gravitational-wave detectors like LIGO, manifesting as shot noise and quantum radiation pressure noise.
D. Ganapathy   +182 more
doaj   +1 more source

Compact Binary Coalescences: Astrophysical Processes and Lessons Learned

open access: yesGalaxies, 2022
On 11 February 2016, the LIGO and Virgo scientific collaborations announced the first direct detection of gravitational waves, a signal caught by the LIGO interferometers on 14 September 2015, and produced by the coalescence of two stellar-mass black ...
Mario Spera   +2 more
doaj   +1 more source

Combination of focused ultrasound blood‐brain barrier opening with Lecanemab therapy in mild Alzheimer's disease [PDF]

open access: yesAlzheimers Dement
Abstract Background Alzheimer's disease (AD) is a major neurodegenerative disorder affecting millions worldwide, with limited treatment options and significant challenges in drug delivery. Monoclonal antibody (mAb) therapies targeting β‐amyloid plaques have shown promise but are constrained by potential adverse effects, including amyloid‐related ...
Rezai A   +9 more
europepmc   +2 more sources

GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run - Candidate Data Release

open access: yes, 2021
Data associated with candidates in GWTC-2.1. These are gravitational-wave candidates from the first half of the third observing run (O3a) of the Advanced LIGO and Virgo detectors that pass a false alarm rate threshold of 2/day.
LIGO Scientific Collaboration and Virgo Collaboration
core   +1 more source

GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo during the First Half of the Third Observing Run [PDF]

open access: yes, 2021
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 1 April 2019 15∶00 UTC and 1 October 2019 15∶00 UTC.
et al. (Ligo and Virgo Collaborations)   +2 more
core   +1 more source

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