دورية أكاديمية

E-TEST: a compact low-frequency isolator for a large cryogenic mirror

التفاصيل البيبلوغرافية
العنوان: E-TEST: a compact low-frequency isolator for a large cryogenic mirror
المؤلفون: Sider, Ameer, Di Fronzo, Chiara, Amez-Droz, Loïc, Amorosi, Anthony, Badaracco, Francesca, Baer, Patrick, Bertolini, Alessandro, Bruno, Giacomo, Cebeci, Pelin, Collette, Christophe, Ebert, Johannes, Erben, Benjamin, Esteves, Rui, Ferreira, Elvis, Gatti, Alberto, Giesberts, Martin, Hebbeker, Thomas, van Heijningen, Joris, Hennig, Jan-Simon, Hennig, Margot, Hild, Stefan, Hoefer, Marco, Hoffmann, Hans-Dieter, Jamshidi, Rasa, Jacques, Lionel, Joppe, Robert, Kuhlbusch, Tim, Lakkis, Mouhamad Haidar, Lenaerts, Cedric, Locquet, Jean-Pierre, Loicq, Jerôme, Le Van, Bao, Loosen, Peter, Nesladek, Milos, Reiter, Melina, Stahl, Achim, Steinlechner, Jessia, Steinlechner, Sebastian, Tavernier, Filip, Teloi, Mayana, Vilaboa Perez, Jesus, Zeoli, Morgane
المصدر: Classical and Quantum Gravity (2023-06-27)
بيانات النشر: IOP Publishing
سنة النشر: 2023
المجموعة: University of Liège: ORBi (Open Repository and Bibliography)
مصطلحات موضوعية: E-TEST, radiative cooling, silicon mirror, coating, cryogenic sensor, active control, seismic, Engineering, computing & technology, Aerospace & aeronautics engineering, Ingénierie, informatique & technologie, Ingénierie aérospatiale
الوصف: peer reviewed ; Abstract To achieve the expected level of sensitivity of third-generation gravitational-wave observatories, more accurate and sensitive instruments than those of the second generation must be used to reduce all sources of noise. Amongst them, one of the most relevant is seismic noise, which will require the development of a better isolation system, especially at low frequencies (below 10 Hz), the operation of large cryogenic silicon mirrors, and the improvement of optical wavelength readouts. In this framework, this article presents the activities of the E-TEST (Einstein Telescope Euregio Meuse-Rhine Site & Technology) to develop and test new key technologies for the next generation of GW observatories. A compact isolator system for a large silicon mirror at a low frequency is proposed. The design of the isolator allows the overall height of the isolation system to be significantly compact and also suppresses seismic noise at low frequencies. To minimize the effect of thermal noise, the isolation system is provided with a 100-kg silicon mirror which is suspended in a vacuum chamber at cryogenic temperature (25-40 K). To achieve this temperature without inducing vibrations to the mirror, a radiation-based cooling strategy is employed. In addition, cryogenic sensors and electronics are being developed as part of the E-TEST to detect vibrational motion in the penultimate cryogenic stage. Since the used silicon material is not transparent below the wavelengths typically used for GW detectors, new optical components and lasers must be developed in the range above 1500 nm to reduce absorption and scattering losses. Therefore, solid-state and fiber lasers with a wavelength of 2090 nm, matching high-efficiency photodiodes, and low-noise crystalline coatings are being developed. Accordingly, the key technologies provided by E-TEST serve crucially to reduce the limitations of the current generation of GW observatories and to determine the technical design for the next generation.
نوع الوثيقة: article in journal/newspaper
اللغة: English
تدمد: 0264-9381
1361-6382
العلاقة: https://iopscience.iop.org/article/10.1088/1361-6382/ace230Test; urn:issn:0264-9381; urn:issn:1361-6382; https://orbi.uliege.be/handle/2268/305597Test; info:hdl:2268/305597; https://orbi.uliege.be/bitstream/2268/305597/1/CQG%20article.pdfTest; scopus-id:2-s2.0-85165380295
DOI: 10.1088/1361-6382/ace230
الإتاحة: https://doi.org/10.1088/1361-6382/ace230Test
https://orbi.uliege.be/handle/2268/305597Test
https://orbi.uliege.be/bitstream/2268/305597/1/CQG%20article.pdfTest
حقوق: open access ; http://purl.org/coar/access_right/c_abf2Test ; info:eu-repo/semantics/openAccess
رقم الانضمام: edsbas.58AAB81A
قاعدة البيانات: BASE
الوصف
تدمد:02649381
13616382
DOI:10.1088/1361-6382/ace230