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-Reference-Cited by-同舟云学术

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

Published:2024-02 Issue:1 Volume:16 Page:1-9
ISSN:1943-0655
Container-title:IEEE Photonics Journal
language:
Short-container-title:IEEE Photonics J.

Author:

Baer Patrick¹^ORCID,Cebeci Pelin¹^ORCID,Reiter Melina¹,Bontke Florian¹^ORCID,Giesberts Martin¹^ORCID,Hoffmann Hans-Dieter¹

Affiliation:

1. Fraunhofer ILT-Institute for Laser Technology, Aachen, Germany

Funder

Interreg EMR, European Regional Development Fund

Ministry for Economic Affairs, Innovation, Digitalization and Energy of the State of North Rhine-Westphalia

Publisher

Institute of Electrical and Electronics Engineers (IEEE)

Link

http://xplorestaging.ieee.org/ielx7/4563994/10375286/10400783.pdf?arnumber=10400783

Reference17 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. E-TEST prototype design report;Sider,2022

3. A cryogenic silicon interferometer for gravitational-wave detection

4. Silicon-Based Optical Mirror Coatings for Ultrahigh Precision Metrology and Sensing

5. Stabilized high-power laser system for the gravitational wave detector advanced LIGO

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