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Proceedings Paper

Nonlinear optical effects in the LIGO gravitational-wave interferometer
Author(s): Phil Willems
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Paper Abstract

LIGO (Laser Interferometer Gravitational-wave Observatory) is a trio of sensitive Michelson interferometers designed to detect extremely relativistic astrophysical processes by the ripples they produce in spacetime. For best sensitivity, these interferometers are kilometers long, contain nearly unstable cavities, and operate at high optical power, making them uniquely susceptible to thermal aberrations and radiation-pressure-derived instabilities. We describe the LIGO interferometers, and their high power lasers and input optics, and described how thermal aberrations have been successfully controlled using adaptive corrective heating. The Advanced LIGO detectors, an upgrade to LIGO planned for installation in the year 2010, will operate with even higher optical power. We detail the additional challenges in construction and thermal compensation for Advanced LIGO, and detail how radiation-pressure derived instabilities influence the design, operation, and sensitivity ofAdvanced LIGO.

Paper Details

Date Published: 3 February 2006
PDF: 11 pages
Proc. SPIE 5975, Topical Problems of Nonlinear Wave Physics, 59750H (3 February 2006); doi: 10.1117/12.675551
Show Author Affiliations
Phil Willems, California Institute of Technology (United States)

Published in SPIE Proceedings Vol. 5975:
Topical Problems of Nonlinear Wave Physics
Alexander M. Sergeev, Editor(s)

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