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Advanced LIGO

Aasi, J.; Abbott, B.; Abbott, Robert; Abbott, T.; Abernathy, M.; Ackley, K.; Adams, C.; Adams, T.; Addesso, P.; Adhikari, Rana; Adya, V.; Bartos, I.; Charlton, Philip; Chow, Jong; Coward, D.; Dhurandhar, S.; Factourovich, M.; Fairhurst, S.; Giaime, J.; Greenhalgh, R. J. S.; Hosken, Dave; Iyer, B. R.; Jones, D. I.; Mandic, V.; Mansell, Georgia; McClelland, David; Meadors, G. D.; Melatos, Andrew; Mendell, G.; Nguyen, Thanh; Ottaway, D. J.; Owen, Benjamin; Penn, S.; Rabeling, David; Rajalakshmi, G.; Reed, C. M.; Reitze, D.; Riles, K.; Sammut, L.; Sathyaprakash, B.; Saulson, P.; Schofield, R.; Scott, Susan M.; Shaddock, Daniel; Sigg, D.; Sintes, A.; Slagmolen, Bram; Souradeep, T.; Staley, A.; Summerscales, T. Z.; Unnikrishnan, C. S.; Veitch, Peter John; Vorvick, C.; Wade, Andrew; Ward, Robert; Whiting, B. F.

Description

The Advanced LIGO gravitational wave detectors are second-generation instruments designed and built for the two LIGO observatories in Hanford, WA and Livingston, LA, USA. The two instruments are identical in design, and are specialized versions of a Michelson interferometer with 4 km long arms. As in Initial LIGO, Fabry-Perot cavities are used in the arms to increase the interaction time with a gravitational wave, and power recycling is used to increase the effective laser power. Signal...[Show more]

CollectionsANU Research Publications
Date published: 2015
Type: Journal article
URI: http://hdl.handle.net/1885/102579
Source: Classical and Quantum Gravity
DOI: 10.1088/0264-9381/32/7/074001

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