Differential phase-noise properties of a ytterbium-doped fiber amplifier for the Laser Interferometer Space Antenna
Optics Letters, Vol. 35, Issue 3, pp. 435-437 (2010)
http://dx.doi.org/10.1364/OL.35.000435
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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
© 2010 Optical Society of America
OCIS Codes
(060.2320) Fiber optics and optical communications : Fiber optics amplifiers and oscillators
(270.2500) Quantum optics : Fluctuations, relaxations, and noise
ToC Category:
Quantum Optics
History
Original Manuscript: October 20, 2009
Revised Manuscript: December 22, 2009
Manuscript Accepted: December 23, 2009
Published: January 29, 2010
Citation
M. Tröbs, S. Barke, Th. Theeg, D. Kracht, G. Heinzel, and K. Danzmann, "Differential phase-noise properties of a ytterbium-doped fiber amplifier for the Laser Interferometer Space Antenna," Opt. Lett. 35, 435-437 (2010)
http://www.opticsinfobase.org/ol/abstract.cfm?URI=ol-35-3-435
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