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  Differential phase-noise properties of a ytterbium-doped fiber amplifier for the Laser Interferometer Space Antenna

Tröbs, M., Barke, S., Theeg, T., Kracht, D., Heinzel, G., & Danzmann, K. (2010). Differential phase-noise properties of a ytterbium-doped fiber amplifier for the Laser Interferometer Space Antenna. Optics Letters, 35(3), 435-437. doi:10.1364/OL.35.000435.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-64DC-1 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-64DF-C
Genre: Journal Article

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Tröbs, Michael1, Author              
Barke, S.1, Author
Theeg, Th., Author
Kracht, D., Author
Heinzel, Gerhard1, Author              
Danzmann, Karsten1, Author              
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, Hannover, DE, ou_24010              

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 Abstract: The interferometric gravitational-wave detector Laser Interferometer Space Antenna (LISA) needs to transfer clock information among its three spacecraft in the form of phase-modulation sidebands. For this reason phase noise introduced by the optical chain between the carrier and a sideband must be low. We have measured this differential phase noise for a ytterbium-doped fiber amplifier emitting up to 2 W. For 1 W of output power as required for LISA, the measured differential phase noise was within its requirement. For 2 W output power the amplifier exhibited stimulated Brillouin scattering and showed a differential phase-noise factor of up to 15 higher. Dependencies on operating parameters and optical length noise of the amplifier were also measured.

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 Dates: 2010
 Publication Status: Published in print
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 Identifiers: DOI: 10.1364/OL.35.000435
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Title: Optics Letters
Source Genre: Journal
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Publ. Info: New York, NY : The Society
Pages: - Volume / Issue: 35 (3) Sequence Number: - Start / End Page: 435 - 437 Identifier: Other: 954925474435
ISSN: 0146-9592