Please use this identifier to cite or link to this item: http://hdl.handle.net/1942/40775
Title: E-TEST prototype design report
Data Creator - person: Sider, Ameer
Amez-Droz, L.
Amorosi, A.
Badaracco, F.
Baer, P.
Bruno, G.
Bertolini, A.
Collette, C.
Cebeci, P.
Di Fronzo, C.
Ebert, J.
Erben, B.
Esteves, R.
Ferreira, E.
Gatti, A.
Giesberts, M.
Hebbeker, T.
Hennig, J. S.
Hennig, M.
Hild, S.
Hoefer, M.
Hoffmann, H. D.
Jacques, L.
Jamshidi, R.
Joppe, R.
Kuhlbusch, T.
Lenaert, C.
Lakkis, M. H.
Van, B. L. Le
Loicq, J.
Locquet, J. P.
Loosen, P.
NESLADEK, Milos 
Reiter, M.
Stahl, A.
Steinlechner, J.
Steinlechner, S.
Teloi, M.
Perez, J. Villaboa
van Heijningen, J.
Zeoli, M.
Data Creator - organization: Université de Liège
TU Delft
Fraunhofer Institute for Laser Technology
Hasselt University
Nikhef
Maastricht University
UCLouvain
RWTH Aachen University
KU Leuven
Data Curator - person: Sider, Ameer
Data Curator - organization: Université de Liège
Rights Holder - person: Sider, Ameer
Rights Holder - organization: Université de Liège
Publisher: arXiv
Issue Date: 2022
Abstract: E-TEST (Einstein Telescope Euregio-Meuse-Rhin Site and Technology) is a project recently funded by the European program Ineterreg Euregio Meuse-Rhine. This program is dedicated to innovative cross boarder activities between Belgium, The Netherlands and Germany. With a total budget of15MC and a consortium of 11 partners from the three countries, the objective of the project is twofold. Firstly, to develop an eco-friendly and non-invasive imaging of the geological conditions as well as the development of an observatory of the underground in the EMR region. Secondly, to develop technologies necessary for 3rd generation gravitational wave detectors. In particular, it is proposed to develop a prototype of large suspended cryogenic silicon mirror, isolated from seismic vibrations at low frequency. The total budget of the project is equally spread over the two activities. The first activity is not discussed at all in this report. The E-TEST prototype will have some key unique features: a silicon mirror of 100 kg, a radiative cooling strategy (non contact), a low-frequency hybrid isolation stage, cryogenic sensors and electronics, a laser and optics at 2 microns, a low thermal noise coating.
Research Discipline: Natural sciences > Physical sciences > Quantum physics > Quantum optics (01031104)
Keywords: Instrumentation and Methods for Astrophysics (astro-ph.IM);General Relativity and Quantum Cosmology (gr-qc);FOS: Physical sciences;FOS: Physical sciences
DOI: 10.48550/arXiv.2212.10083
Link to publication/dataset: https://arxiv.org/abs/2212.10083
Source: arXiv. 10.48550/arXiv.2212.10083 https://arxiv.org/abs/2212.10083
Publications related to the dataset: 10.1088/1361-6382/ace230
License: Creative Commons Attribution 4.0 International (CC-BY-4.0)
Access Rights: Open Access
Category: DS
Type: Dataset
Appears in Collections:Datasets

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