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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]
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−0.8 × 10 47 joules or 5300 +900 −800 foes) in total radiated as gravitational waves, reaching a peak emission rate in its final few milliseconds of about 3.6 +0.5 −0.4 × 10 49 watts – a level greater than the combined power of all light radiated by all the stars in the observable universe. [3] [4] [15] [16] [d]
LIGO has been involved in all subsequent detections to date, with Virgo joining in August 2017. [2] Joint observation runs of LIGO and VIRGO, designated "O1, O2, etc." span many months, with months of maintenance and upgrades in-between designed to increase the instruments sensitivity and range.
Currently, the most sensitive ground-based laser interferometer is LIGO – the Laser Interferometer Gravitational Wave Observatory. LIGO is famous as the site of the first confirmed detections of gravitational waves in 2015. LIGO has two detectors: one in Livingston, Louisiana; the other at the Hanford site in Richland, Washington.
There are several ground-based laser interferometers which span several miles/kilometers, including: the two Laser Interferometer Gravitational-Wave Observatory (LIGO) detectors in WA and LA, USA; Virgo, at the European Gravitational Observatory in Italy; GEO600 in Germany, and the Kamioka Gravitational Wave Detector (KAGRA) in Japan. While ...
Adhikari is actively involved in the LIGO-India project, which aims to build a gravitational-wave observatory in India. [6] He was elected as a Fellow of the American Physical Society [8] and a member of Optica (formerly known as Optical Society of America). [9] Since 2019 he has been a member of the Infosys Prize jury for physical sciences. [10]
GW170104 was a gravitational wave signal detected by the LIGO observatory on 4 January 2017. On 1 June 2017, the LIGO and Virgo collaborations announced that they had reliably verified the signal, making it the third such signal announced, after GW150914 and GW151226, and fourth overall. [1] [2]