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Technology for the next gravitational wave detectors

MITROFANOV, V (Faculty of Physics, Moscow State University, Moscow 119991, Russia), CHAO, S (Institute of Photonics Technologies, “National” Tsing Hua University, Hsinchu 30013, China), PAN, H-W (Institute of Photonics Technologies, “National” Tsing Hua University, Hsinchu 30013, China), KUO, L-C (Institute of Photonics Technologies, “National” Tsing Hua University, Hsinchu 30013, China), COLE, G (Crystalline Mirror Solutions LLC, 114 E Haley St., Suite G, Santa Barbara, CA 93101, USA & Crystalline Mirror Solutions GmbH, Seestadtstr. 27, Top 1.05, A-1220 Vienna, Austria & Vienna Center for Quantum Science and Technology (VCQ), Faculty of Physics,), DEGALLAIX, J (Laboratoire des Matériaux Avancés, 7 Avenue Pierre de Coubertin, Villeurbanne 69100, France) and WILLKE, B (Max Planck Institute for Gravitational Physics (Albert Einstein Institute) and Leibniz Universit¨at Hannover, Germany)
Keywords:

gravitational waves, advanced techniques, thermal noise, coating, laser

Document typeArticle
Journal title / SourceSCIENCE CHINA Physics, Mechanics & Astronomy
Peer-reviewed articleYes
Volume58
Issue12
Page numbers / Article number120404
Publisher's nameScience China Press and Springer-Verlag
Publisher's address (city only)Berlin Heidelberg
Publication date 2015-12-4
ISSN1674-7348
DOI10.1007/s11433-015-5738-8
Web URLhttp://link.springer.com/article/10.1007%2Fs11433-015-5738-8
LanguageEnglish

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