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Gravitational wave
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Propagating spacetime ripple
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Gravitational-wave observatory
Device used to measure gravitational waves
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Gravitational wave background
Random background of gravitational waves permeating the Universe
Subject of 13
Status of the GEO600 gravitational wave detector
Toward the detection of gravitational waves under non-Gaussian noises II. Independent component analysis
scientific article
Gravitational-wave emission from compact galactic binaries
scientific article published in the Astrophysical Journal
Galaxy strategy for LIGO-Virgo gravitational wave counterpart searches
scientific article published in the Astrophysical Journal
Stable double-resonance optical spring in laser gravitational-wave detectors
scholarly article
Prospects for Detecting Gravitational Waves at 5 Hz with Ground-Based Detectors
scientific article published in Physical Review Letters
Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914
journal article from 'The Astrophysical Journal Letters' published in 2016
Networks of gravitational wave detectors and three figures of merit
Challenges of gravitational wave detection using long-baseline cavity-assisted large momentum transfer atom interferometry
scientific article published on 23 August 2018
Supplement: "Localization and broadband follow-up of the gravitational-wave transient GW150914" (2016, ApJL, 826, L13)
scientific article published on 20 July 2016
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Wikipedia

Gravitational waves are waves of the intensity of gravity that are generated by the accelerated masses of binary stars and other motions of gravitating masses, and propagate as waves outward from their source at the speed of light. They were first proposed by Oliver Heaviside in 1893 and then later by Henri Poincaré in 1905 as the gravitational...

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Event (relativity)
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Spacetime
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