Recent development of a laser interferometer for Taiji space gravitational wave detection | Research Square window.SnipcartSettings = { analytics: { enabled: false } }; (function() { var accessVector = localStorage.getItem('access_vector') || ''; window.dataLayer = window.dataLayer || []; if (accessVector) { window.dataLayer.push({ user: { profile: { profileInfo: { snid: accessVector } } } }); } })(); (function(w,d,s,l,i){w[l]=w[l]||[];w[l].push({'gtm.start':new Date().getTime(),event:'gtm.js'});var f=d.getElementsByTagName(s)[0],j=d.createElement(s),dl=l!='dataLayer'?'&l='+l:'';j.async=true;j.src='https://www.googletagmanager.com/gtm.js?id='+i+dl;f.parentNode.insertBefore(j,f);})(window,document,'script','dataLayer','GTM-K279D39R'); Browse Preprints In Review Journals COVID-19 Preprints AJE Video Bytes Research Tools Research Promotion AJE Professional Editing AJE Rubriq About Preprint Platform In Review Editorial Policies Our Team Advisory Board Help Center Sign In Submit a Preprint Cite Share Download PDF Article Recent development of a laser interferometer for Taiji space gravitational wave detection Ziren Luo, He Shan Liu, Juan Wang, Wei Tao, Ke Qi Qi, Shao Xin Wang, and 5 more This is a preprint; it has not been peer reviewed by a journal. https://doi.org/ 10.21203/rs.3.rs-4776951/v1 This work is licensed under a CC BY 4.0 License Status: Posted Version 1 posted You are reading this latest preprint version Abstract In this study, we developed and constructed the first-generation ultrastable optical bench (OB) for the Taiji program. The OB uses optical bonding technology, and for the first time, noise testing and calibration were performed. A comprehensive analysis was carried out on the various noise sources impacting the interferometer system; these sources included laser frequency noise, laser power noise, thermal drift noise, and angular jitter noise. When the environmental conditions fell short of our stringent requirements, an advanced post-data processing technique was employed to effectively reduce both the thermal drift noise and angular coupling noise. The results revealed that the noise level of the interferometer system reached 1.1 pm/Hz 1/2 at 1 Hz, 5 pm/Hz 1/2 at 0.1 Hz, and 8 pm/Hz 1/2 at 0.01 Hz; these levels met the requirements of the Taiji pathfinder mission. Furthermore, a future research proposal was provided, with the aim to meet the full frequency range requirements of the Taiji program. Physical sciences/Optics and photonics/Other photonics/Optical metrology Physical sciences/Physics/Electronics, photonics and device physics/Photonic devices Full Text Additional Declarations (Not answered) Cite Share Download PDF Status: Posted Version 1 posted You are reading this latest preprint version Research Square lets you share your work early, gain feedback from the community, and start making changes to your manuscript prior to peer review in a journal. As a division of Research Square Company, we’re committed to making research communication faster, fairer, and more useful. We do this by developing innovative software and high quality services for the global research community. Our growing team is made up of researchers and industry professionals working together to solve the most critical problems facing scientific publishing. Also discoverable on Platform About Our Team In Review Editorial Policies Advisory Board Help Center Resources Author Services Accessibility API Access RSS feed Manage Cookie Preferences © Research Square 2026 | ISSN 2693-5015 (online) Privacy Policy Terms of Service Do Not Sell My Personal Information {"props":{"pageProps":{"initialData":{"identity":"rs-4776951","acceptedTermsAndConditions":true,"allowDirectSubmit":true,"archivedVersions":[],"articleType":"Article","associatedPublications":[],"authors":[{"id":339576728,"identity":"d243257f-0400-4f64-9a4b-cbae5a832f1a","order_by":0,"name":"Ziren 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