Ultra-Low-Noise, Single-Frequency, All-PM Thulium- and Holmium-Doped Fiber Amplifiers at 1950 nm and 2090 nm for Third-Generation Gravitational Wave Detectors

Ultra-Low-Noise, Single-Frequency, All-PM Thulium- and Holmium-Doped Fiber Amplifiers at 1950 nm and 2090 nm for Third-Generation Gravitational Wave Detectors

In the context of the E-TEST Interreg project, Fraunhofer ILT develops high stability, narrow linewidth laser seed sources and amplifiers at a wavelength of approx. 2 μm for potential usage in a third-generation gravitational wave detector: the Einstein telescope. While for such an applic...

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Bibliographic Details
Main Authors: Patrick Baer, Pelin Cebeci, Melina Reiter, Florian Bontke, Martin Giesberts, Hans-Dieter Hoffmann
Format: Article
Language:English
Published: IEEE 2024-01-01
Series:IEEE Photonics Journal
Subjects:
Holmium-doped fiber laser
thulium-doped fiber laser
ultra-high stability
ultra-low-noise
single-frequency
relative intensity noise
Online Access:https://ieeexplore.ieee.org/document/10400783/
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https://ieeexplore.ieee.org/document/10400783/

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