Astrophysics (index)

LIGO

(Laser Interferometer Gravitational-Wave Observatory)
(pair of observatories to detect gravitational waves)

LIGO (or Laser Interferometer Gravitational-Wave Observatory) is a pair of Gravitational Wave (GW) observatories that work in unison, in Livingston, Louisiana (LIGO L or LLO for LIGO Livingston Observatory) Hanford, Washington (LIGO H or LHO for LIGO Hanford Observatory), 3002 kilometers apart. They are Interferometers, looking for unexplained changes in distance between two lengths at right angles, i.e., Michelson Interferometers. The delta distance they aim to detect is on the order of 10-21, which less than the width of an atomic nucleus. Other sources of distance change such as ground movements like Earthquakes, are filtered out by detecting them independently, and by the use of two separated detectors which should both register something affecting the whole Earth at once, i.e., an actual gravitational wave. The use of two detectors also allows some determination of the direction from which the wave came. The two operated from 2002 to 2010, shutting down for a planned four year upgrade as Advanced LIGO (AdLIGO) which aims at a sensitivity that covers a thousand times the volume for a given wave-strength, thus can detect a thousand times the number of events, or see something a thousand times more often.

In Fall 2015, when Advanced LIGO first went live for testing, it detected a gravitational wave event suggesting a Black Hole (BH) merger. It had been predicted that the first detected waves would be from a Neutron Star merger. The second detection was in the Spring of 2016 and also appears to be a Compact Object merger.


(observatory,interferometer,NSF,gravitational waves,distributed)
http://en.wikipedia.org/wiki/LIGO
http://www.ligo.caltech.edu/
http://www.advancedligo.mit.edu/

Referenced by:
BlackGEM
Chirp
Gravitational Wave (GW)
LIGO-India

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