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Stabilized High Power Laser for Advanced Gravitational Wave Detectors

Willke, B. and Danzmann, K. and Fallnich, C. and Frede, M. and Heurs, M. and King, P. and Kracht, D. and Kwee, P. and Savage, R. and Seifert, F. and Wilhelm, R. (2006) Stabilized High Power Laser for Advanced Gravitational Wave Detectors. Journal of Physics: Conference Series, 32 (1). pp. 270-275. ISSN 1742-6596. http://resolver.caltech.edu/CaltechAUTHORS:WILjpcs06

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Abstract

Second generation gravitational wave detectors require high power lasers with several 100W of output power and with very low temporal and spatial fluctuations. In this paper we discuss possible setups to achieve high laser power and describe a 200W prestabilized laser system (PSL). The PSL noise requirements for advanced gravitational wave detectors will be discussed in general and the stabilization scheme proposed for the Advanced LIGO PSL will be described. Special emphasis will be given to the most demanding power stabilization requiremets and new results (RIN ≤ 4×10-9/surdHz) will be presented.


Item Type:Article
Additional Information:© IOP Publishing Limited 2006. Proceedings of the Sixth Edoardo Amaldi Conference on Gravitational Waves, 20–24 June 2005, Bankoku Shinryoukan, Okinawa, Japan
Issue or Number:1
Record Number:CaltechAUTHORS:WILjpcs06
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:WILjpcs06
Alternative URL:http://dx.doi.org/10.1088/1742-6596/32/1/040
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:2683
Collection:CaltechAUTHORS
Deposited By: Archive Administrator
Deposited On:17 Apr 2006
Last Modified:26 Dec 2012 08:50

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