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Seismic glitchness at Sos Enattos site: impact on intermediate black hole binaries detection efficiency

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, L. ; Fiori, I. ; Giunchi, C. ; Grado, A. ; Harms, J. ; Majorana, E. ; Mangano, V. ; Marsella, M ; Migoni, C. ; Naticchioni, 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.

European physical journal plus, 2021-05, Vol.136 (5), p.511, Article 511 [Periódico revisado por pares]

Berlin/Heidelberg: Springer Berlin Heidelberg

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Título:
Seismic glitchness at Sos Enattos site: impact on intermediate black hole binaries detection efficiency
Autor: 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, L. ; Fiori, I. ; Giunchi, C. ; Grado, A. ; Harms, J. ; Majorana, E. ; Mangano, V. ; Marsella, M ; Migoni, C. ; Naticchioni, 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.
Assuntos: Applied and Technical Physics ; Atomic ; Bandwidths ; Binary system ; Black holes ; Complex Systems ; Condensed Matter Physics ; Configurations ; Earth Sciences ; Gravitational waves ; Ground motion ; Mathematical and Computational Physics ; Molecular ; Noise ; Observatories ; Optical and Plasma Physics ; Physics ; Physics and Astronomy ; Regular Article ; Sciences of the Universe ; Sensors ; Spectrum allocation ; Theoretical ; Xylophone music
É parte de: European physical journal plus, 2021-05, Vol.136 (5), p.511, Article 511
Descrição: 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.
Editor: Berlin/Heidelberg: Springer Berlin Heidelberg
Idioma: Inglês

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Seismic glitchness at Sos Enattos site: impact on intermediate black hole binaries detection efficiency

Berlin/Heidelberg: Springer Berlin Heidelberg

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