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The Virgo interferometer is a large-scale scientific instrument near Pisa, Italy, for detecting gravitational waves.The detector is a Michelson interferometer, which can detect the minuscule length variations in its two 3-km (1.9 mi) arms induced by the passage of gravitational waves.
While a lot of efforts were dedicated to improving the resonant bar design, the idea of using a large interferometer for gravitational wave detection was formulated in the 1970s and began to gain traction in the 1980s, leading to the foundation of LIGO in 1984 and Virgo in 1989. [3] [4]
The European Gravitational Observatory (EGO) is a consortium established to manage the Virgo interferometer and its related infrastructure, as well as to promote cooperation in the field of gravitational wave research in Europe.
Upgrades to LIGO and other detectors such as Virgo, GEO600, and TAMA 300 should increase the sensitivity further, and the next generation of instruments (Advanced LIGO Plus and Advanced Virgo Plus) will be more sensitive still. Another highly sensitive interferometer began operations in 2020.
The Virgo interferometer is a large-scale scientific instrument near Pisa, Italy, for detecting gravitational waves.The detector detects minuscule length variations in its two 3-km (1.9 mi) arms induced by the passage of gravitational waves.
He is most famous for being one of the two fathers of the Virgo interferometer with Adalberto Giazotto, directing the consortium during its design and construction between 1989 and 2003. [1] He was awarded the Ampère Prize in 2016 [2] and the CNRS Gold Medal in 2017 [1] for his work on the Virgo detector.
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The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool. [1]