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Advanced LIGO: the next generation of gravitational wave detectors

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Harry, Gregory M, the LIGO Scientific Collaboration·2010·Classical and Quantum Gravity

Abstract

The Advanced LIGO gravitational wave detectors are next generation instruments which will replace the existing initial LIGO detectors. They are currently being constructed and installed. Advanced LIGO strain sensitivity is designed to be about a factor 10 better than initial LIGO over a broad band and usable to 10 Hz, in contrast to 40 Hz for initial LIGO. This is expected to allow for detections and significant astrophysics in most categories of gravitational waves. To achieve this sensitivity, all hardware subsystems are being replaced with improvements. Designs and expected performance are presented for the seismic isolation, suspensions, optics and laser subsystems. Possible enhancements to Advanced LIGO, either to resolve problems that may arise and/or to allow for improved performance, are now being researched. Some of these enhancements are discussed along with some potential technology being considered for detectors beyond Advanced LIGO.

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Metadata

Authors
Harry, G. M., & the LIGO Scientific Collaboration
Venue
Classical and Quantum Gravity
Published
2010-04-06
Volume
27
Issue
8
Pages
084006
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2012291066
Cited by
1,301
References
0
FWCI
56.71
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Advanced LIGO: the next generation of gravitational wave detectors. https://app.cochat.ai/papers/10.1088/0264-9381/27/8/084006
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Harry, G. M., & the LIGO Scientific Collaboration. (2010). Advanced LIGO: the next generation of gravitational wave detectors. Classical and Quantum Gravity. https://doi.org/10.1088/0264-9381/27/8/084006

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