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  Laser development for LISA

Tröbs, M., Weßels, P., Fallnich, C., Bode, M., Freitag, I., Skorupka, S., et al. (2006). Laser development for LISA. Classical and Quantum Gravity, 23(8), S151-S158.

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cqg6_8_s20.pdf (Publisher version), 234KB
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 Creators:
Tröbs, Michael1, Author           
Weßels, P., Author
Fallnich, Carsten, Author
Bode, M., Author
Freitag, Ingo, Author
Skorupka, Sascha1, 2, Author
Heinzel, Gerhard1, Author           
Danzmann, Karsten1, Author           
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24010              
2AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24009              

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 Abstract: The two most promising configurations for the LISA laser are a stand-alone diode-pumped nonplanar ring oscillator (NPRO) or a fibre amplifier seeded by a low-power NPRO. The stand-alone laser was stabilized in frequency to a ULE cavity and in power to an electronic reference. For the first time the LISA requirement of relative power noise below 2 × 10-4/Hz1/2 was fulfilled in the whole frequency range from 0.1 mHz to 1 Hz. The LISA goal of frequency noise below 30 Hz/Hz1/2 was achieved for frequencies above 3 mHz. As a first step in the characterization of an oscillator-amplifier system, the excess frequency noise of an ytterbium-doped fibre amplifier was measured. For frequencies between 0.1 mHz and 1 Hz the excess noise was measured to be below 0.1 Hz/Hz1/2, which is significantly below the free-running frequency noise of NPROs.

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 Dates: 2006
 Publication Status: Issued
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 Identifiers: eDoc: 265181
DOI: 10.1088/0264-9381/23/8/S20
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Title: 6th Edoardo Amaldi Conference On Gravitational Waves
Place of Event: Okinawa, Japan
Start-/End Date: 2005-06-20 - 2005-06-24

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Title: Classical and Quantum Gravity
Source Genre: Journal
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Pages: - Volume / Issue: 23 (8) Sequence Number: - Start / End Page: S151 - S158 Identifier: ISSN: 0264-9381