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Conferences > CLEO_SI > 2013 > CW3M > CW3M.5

Single-Frequency Fiber Amplifiers for Gravitational Wave Detection

P. Weßels, M. Karow, V. Kuhn, M. Steinke, H. Tünnermann, D. Kracht, and J. Neumann

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Abstract

Gravitational wave detectors require linearly-polarized, high-power, single-frequency laser sources and set demanding requirements on their stability and beam quality. We discuss current approaches to fulfill the requirements for the upcoming generation of gravitational wave detectors.

© 2013 Optical Society of America

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