2022
DOI: 10.48550/arxiv.2204.04150
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A cryogenic and superconducting inertial sensor for the Lunar Gravitational--Wave Antenna, the Einstein Telescope and Selene-physics

Abstract: The Lunar Gravitational-Wave Antenna is a proposed low-frequency gravitational-wave detector on the Moon surface. It will be composed of an array of high-end cryogenic superconducting inertial sensors (CSISs). A cryogenic environment will be used in combination with superconducting materials to open up pathways to low-loss actuators and sensor mechanics. CSIS revolutionizes the (cryogenic) inertial sensor field with a modelled displacement sensitivity at 0.5 Hz of 3 orders of magnitude better than the current … Show more

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“…The E-TEST prototype aspires to acquire a substrate with a mass, purity and dimensions well on track towards the ET mirrors (45 cm diameter, 210 kg). After polishing, characterisation of the substrate will take place using three experiments of which two are shown in Figure 20: a white light interferometer for precise mirror surface quality characterisation, an interferometric measurement scheme using the silicon substrate as a Fabry-Perot etalon to determine its temperature [100] and mechanical loss measurements of internal mechanical modes using a fm/ √ Hz interferometer [101] excited by a tiny hammer, i.e., a small mass-spring element. Finally, crystalline coating layers are characterised regarding, e.g., their optical and elastic properties, which are important to estimate the noise behaviour of the ultimate coatings.…”
Section: Optical Engineeringmentioning
confidence: 99%
“…The E-TEST prototype aspires to acquire a substrate with a mass, purity and dimensions well on track towards the ET mirrors (45 cm diameter, 210 kg). After polishing, characterisation of the substrate will take place using three experiments of which two are shown in Figure 20: a white light interferometer for precise mirror surface quality characterisation, an interferometric measurement scheme using the silicon substrate as a Fabry-Perot etalon to determine its temperature [100] and mechanical loss measurements of internal mechanical modes using a fm/ √ Hz interferometer [101] excited by a tiny hammer, i.e., a small mass-spring element. Finally, crystalline coating layers are characterised regarding, e.g., their optical and elastic properties, which are important to estimate the noise behaviour of the ultimate coatings.…”
Section: Optical Engineeringmentioning
confidence: 99%