date: 2022-03-07T05:41:15Z
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pdf:docinfo:title: Characterization of Laser Systems at 1550 nm Wavelength for Future Gravitational Wave Detectors
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Keywords: 1550 nm; laser system; gravitational wave detector
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subject: The continuous improvement of current gravitational wave detectors (GWDs) and the preparations for next generation GWDs place high demands on their stabilized laser sources. Some of the laser sources need to operate at laser wavelengths between 1.5 µm and 2.2 µm to support future detectors based on cooled silicon test masses for thermal noise reduction. We present detailed characterizations of different commercial low power seed laser sources and power amplifiers at the wavelength of 1550 nm with respect to performance parameters needed in GWDs. A combination with the most complete set of actuators was arranged as a master-oscillator power amplifier (MOPA), integrated into a stabilization environment and characterized. We present the results of this characterization that make this stabilized MOPA a highly relevant prototype for future GWDs as well as a low noise light source for other experiments in high precision metrology.
dc:creator: Fabian Meylahn and Benno Willke
dcterms:created: 2022-03-07T04:57:57Z
Last-Modified: 2022-03-07T05:41:15Z
dcterms:modified: 2022-03-07T05:41:15Z
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title: Characterization of Laser Systems at 1550 nm Wavelength for Future Gravitational Wave Detectors
Last-Save-Date: 2022-03-07T05:41:15Z
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pdf:docinfo:keywords: 1550 nm; laser system; gravitational wave detector
pdf:docinfo:modified: 2022-03-07T05:41:15Z
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dc:title: Characterization of Laser Systems at 1550 nm Wavelength for Future Gravitational Wave Detectors
modified: 2022-03-07T05:41:15Z
cp:subject: The continuous improvement of current gravitational wave detectors (GWDs) and the preparations for next generation GWDs place high demands on their stabilized laser sources. Some of the laser sources need to operate at laser wavelengths between 1.5 µm and 2.2 µm to support future detectors based on cooled silicon test masses for thermal noise reduction. We present detailed characterizations of different commercial low power seed laser sources and power amplifiers at the wavelength of 1550 nm with respect to performance parameters needed in GWDs. A combination with the most complete set of actuators was arranged as a master-oscillator power amplifier (MOPA), integrated into a stabilization environment and characterized. We present the results of this characterization that make this stabilized MOPA a highly relevant prototype for future GWDs as well as a low noise light source for other experiments in high precision metrology.
pdf:docinfo:subject: The continuous improvement of current gravitational wave detectors (GWDs) and the preparations for next generation GWDs place high demands on their stabilized laser sources. Some of the laser sources need to operate at laser wavelengths between 1.5 µm and 2.2 µm to support future detectors based on cooled silicon test masses for thermal noise reduction. We present detailed characterizations of different commercial low power seed laser sources and power amplifiers at the wavelength of 1550 nm with respect to performance parameters needed in GWDs. A combination with the most complete set of actuators was arranged as a master-oscillator power amplifier (MOPA), integrated into a stabilization environment and characterized. We present the results of this characterization that make this stabilized MOPA a highly relevant prototype for future GWDs as well as a low noise light source for other experiments in high precision metrology.
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pdf:docinfo:creator: Fabian Meylahn and Benno Willke
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creator: Fabian Meylahn and Benno Willke
meta:author: Fabian Meylahn and Benno Willke
dc:subject: 1550 nm; laser system; gravitational wave detector
meta:creation-date: 2022-03-07T04:57:57Z
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meta:keyword: 1550 nm; laser system; gravitational wave detector
Author: Fabian Meylahn and Benno Willke
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pdf:docinfo:created: 2022-03-07T04:57:57Z