Details
Original language | English |
---|---|
Article number | 84 |
Pages (from-to) | 1-13 |
Number of pages | 13 |
Journal | Galaxies |
Volume | 8 |
Issue number | 4 |
Publication status | Published - 8 Dec 2020 |
Abstract
The advanced LIGO gravitational wave detectors need high power laser sources with excellent beam quality and low-noise behavior. We present a pre-stabilized laser system with 70 W of output power that was used in the third observing run of the advanced LIGO detectors. Furthermore, the prototype of a 140 W pre-stabilized laser system for future use in the LIGO observatories is described and characterized.
Keywords
- Gravitational wave detector, Laser amplifier, Laser noise, Pre-modecleaner, Pre-stabilized laser system, Solid state amplifier
ASJC Scopus subject areas
- Physics and Astronomy(all)
- Astronomy and Astrophysics
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In: Galaxies, Vol. 8, No. 4, 84, 08.12.2020, p. 1-13.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - Advanced ligo laser systems for o3 and future observation runs
AU - Bode, Nina
AU - Briggs, Joseph
AU - Chen, Xu
AU - Frede, Maik
AU - Fritschel, Peter
AU - Fyffe, Michael
AU - Gustafson, Eric
AU - Heintze, Matthew
AU - King, Peter
AU - Liu, Jian
AU - Oberling, Jason
AU - Savage, Richard L.
AU - Spencer, Andrew
AU - Willke, Benno
N1 - Funding Information: Acknowledgments: The authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO; and the Science and Technology Facilities Council (STFC) of the United Kingdom and the Max-Planck-Society (MPS) for Funding Information: support of the construction of Advanced LIGO. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors acknowledge the LIGO Scientific Collaboration Fellows program for additional support. Funding Information: Funding: LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation, and operates under cooperative agreement PHY-1764464. aLIGO was built under award PHY-0823459. Funding Information: LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation, and operates under cooperative agreement PHY-1764464. aLIGO was built under award PHY-0823459.
PY - 2020/12/8
Y1 - 2020/12/8
N2 - The advanced LIGO gravitational wave detectors need high power laser sources with excellent beam quality and low-noise behavior. We present a pre-stabilized laser system with 70 W of output power that was used in the third observing run of the advanced LIGO detectors. Furthermore, the prototype of a 140 W pre-stabilized laser system for future use in the LIGO observatories is described and characterized.
AB - The advanced LIGO gravitational wave detectors need high power laser sources with excellent beam quality and low-noise behavior. We present a pre-stabilized laser system with 70 W of output power that was used in the third observing run of the advanced LIGO detectors. Furthermore, the prototype of a 140 W pre-stabilized laser system for future use in the LIGO observatories is described and characterized.
KW - Gravitational wave detector
KW - Laser amplifier
KW - Laser noise
KW - Pre-modecleaner
KW - Pre-stabilized laser system
KW - Solid state amplifier
UR - http://www.scopus.com/inward/record.url?scp=85097658230&partnerID=8YFLogxK
U2 - 10.3390/galaxies8040084
DO - 10.3390/galaxies8040084
M3 - Article
AN - SCOPUS:85097658230
VL - 8
SP - 1
EP - 13
JO - Galaxies
JF - Galaxies
IS - 4
M1 - 84
ER -