Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32622
Title: | Seismic glitchness at Sos Enattos site: impact on intermediate black hole binaries detection efficiency | Authors: | Allocca, A. Berbellini, A. Boschi, L. Calloni, E. Cardello, G. L. Cardini, A. Carpinelli, M. Contu, A. D’Onofrio, L. D’Urso, D. Dell’Aquila, D. Rosa, R. De Fiore, L. Di Giovanni, M. Di Pace, S. Di ERRICO, Luigi Fiori, I. Giunchi, C. GRADO, ANIELLO Harms, J. Majorana, E. MANGANO, VALERIA Marsella, M. MIGONI, CARLO Naticchoni, L. Olivieri, M. Oggiano, G. Paoletti, F. Punturo, M. Puppo, P. Rapagnani, P. Ricci, F. Rozza, D. Saccorotti, G. Sequino, V. Sipala, V. Melo, I. Tosta E. Trozzo, L. |
Issue Date: | 2021 | Journal: | THE EUROPEAN PHYSICAL JOURNAL PLUS | Number: | 136 | Issue: | 5 | Abstract: | Third-generation gravitational wave observatories will extend the lower frequency limit of the observation band toward 2 Hz, where new sources of gravitational waves, in particular intermediate-mass black holes (IMBH), will be detected. In this frequency region, seismic noise will play an important role, mainly through the so-called Newtonian noise, i.e., the gravity-mediated coupling between ground motion and test mass displacements. The signal lifetime of such sources in the detector is of the order of tens of seconds. In order to determine whether a candidate site to host the Einstein Telescope observatory is particularly suitable to observe such sources, it is necessary to estimate the probability distributions that, in the characteristic time scale of the signal, the sensitivity of the detector is not perturbed by Newtonian noise. In this paper, a first analysis is presented, focused on the Sos Enattos site (Sardinia, Italy), a candidate to host the Einstein Telescope. Starting from a long data set of seismic noise, this distribution is evaluated considering both the presently designed triangular ET configuration and also the classical ”L” configuration. | URI: | http://hdl.handle.net/20.500.12386/32622 | URL: | https://link.springer.com/article/10.1140/epjp/s13360-021-01450-8 https://api.elsevier.com/content/abstract/scopus_id/85105757127 |
ISSN: | 2190-5444 | DOI: | 10.1140/epjp/s13360-021-01450-8 | Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista |
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s13360-021-01450-8.pdf | Pdf editoriale | 1.31 MB | Adobe PDF | View/Open |
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