تقرير
Correlated 0.01Hz-40Hz seismic and Newtonian noise and its impact on future gravitational-wave detectors
| العنوان: | Correlated 0.01Hz-40Hz seismic and Newtonian noise and its impact on future gravitational-wave detectors |
|---|---|
| المؤلفون: | Janssens, Kamiel, Boileau, Guillaume, Christensen, Nelson, van Remortel, Nick, Badaracco, Francesca, Canuel, Benjamin, Cardini, Alessandro, Contu, Andrea, Coughlin, Michael W., Decitre, Jean-Baptiste, De Rosa, Rosario, Di Giovanni, Matteo, D'Urso, Domenico, Gaffet, Stéphane, Giunchi, Carlo, Harms, Jan, Koley, Soumen, Mangano, Valentina, Naticchioni, Luca, Olivieri, Marco, Paoletti, Federico, Rozza, Davide, Sabulsky, Dylan O., Shani-Kadmiel, Shahar, Trozzo, Lucia |
| سنة النشر: | 2024 |
| المجموعة: | Astrophysics General Relativity and Quantum Cosmology Physics (Other) |
| مصطلحات موضوعية: | General Relativity and Quantum Cosmology, Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Instrumentation and Detectors |
| الوصف: | We report correlations in underground seismic measurements with horizontal separations of several hundreds of meters to a few kilometers in the frequency range 0.01Hz to 40Hz. These seismic correlations could threaten science goals of planned interferometric gravitational-wave detectors such as the Einstein Telescope as well as atom interferometers such as MIGA and ELGAR. We use seismic measurements from four different sites, i.e. the former Homestake mine (USA) as well as two candidate sites for the Einstein Telescope, Sos Enattos (IT) and Euregio Maas-Rhein (NL-BE-DE) and the site housing the MIGA detector, LSBB (FR). At all sites, we observe significant coherence for at least 50% of the time in the majority of the frequency region of interest. Based on the observed correlations in the seismic fields, we predict levels of correlated Newtonian noise from body waves. We project the effect of correlated Newtonian noise from body waves on the capabilities of the triangular design of the Einstein Telescope's to observe an isotropic gravitational-wave background (GWB) and find that, even in case of the most quiet site, its sensitivity will be affected up to $\sim$20Hz. The resolvable amplitude of a GWB signal with a negatively sloped power-law behaviour would be reduced by several orders of magnitude. However, the resolvability of a power-law signal with a slope of e.g. $\alpha=0$ ($\alpha=2/3$) would be more moderately affected by a factor $\sim$ 6-9 ($\sim$3-4) in case of a low noise environment. Furthermore, we bolster confidence in our results by showing that transient noise features have a limited impact on the presented results. |
| نوع الوثيقة: | Working Paper |
| URL الوصول: | http://arxiv.org/abs/2402.17320 |
| رقم الأكسشن: | edsarx.2402.17320 |
| قاعدة البيانات: | arXiv |
| الوصف غير متاح. |