Physics and Astronomy (all); Gravitational Wave Detectors; Newtonian noise; Wiener Filters; Advanced Virgo
Abstract :
[en] Terrestrial gravity perturbations caused by seismic fields produce the so-called Newtonian noise in gravitational-wave detectors, which is predicted to limit their sensitivity in the upcoming observing runs. In the past, this noise was seen as an infrastructural limitation, i.e., something that cannot be overcome without major investments to improve a detector’s infrastructure. However, it is possible to have at least an indirect estimate of this noise by using the data from a large number of seismometers deployed around a detector’s suspended test masses. The noise estimate can be subtracted from the gravitational-wave data, a process called Newtonian noise cancellation (NNC). In this article, we present the design and implementation of the first NNC system at the Virgo detector as part of its AdV+ upgrade. It uses data from 110 vertical geophones deployed inside the Virgo buildings in optimized array configurations. We use a separate tiltmeter channel to test the pipeline in a proof-of-principle. The system has been running with good performance over months.
Disciplines :
Physics
Author, co-author :
Koley, Soumen ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Ondes gravitationnelles ; Gran Sasso Science Institute (GSSI), L’Aquila, Italy ; INFN, Laboratori Nazionali del Gran Sasso, Assergi, Italy
Harms, Jan; Gran Sasso Science Institute (GSSI), L’Aquila, Italy ; INFN, Laboratori Nazionali del Gran Sasso, Assergi, Italy
Allocca, Annalisa; Università di Napoli “Federico II”, Napoli, Italy ; INFN, Sezione di Napoli, Napoli, Italy
Badaracco, Francesca; INFN, Sezione di Genova, Genova, Italy
Bulik, Tomasz; Astronomical Observatory, University of Warsaw, Warsaw, Poland ; Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland
Calloni, Enrico; Università di Napoli “Federico II”, Napoli, Italy ; INFN, Sezione di Napoli, Napoli, Italy
Cieslar, Marek; Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland
De Rosa, Rosario; Università di Napoli “Federico II”, Napoli, Italy ; INFN, Sezione di Napoli, Napoli, Italy
Errico, Luciano; Università di Napoli “Federico II”, Napoli, Italy ; INFN, Sezione di Napoli, Napoli, Italy
Esposito, Marina; Università di Napoli “Federico II”, Napoli, Italy ; INFN, Sezione di Napoli, Napoli, Italy
Fiori, Irene; European Gravitational Observatory (EGO), Pisa, Italy
Open access funding provided by Gran Sasso Science Institute - GSSI within the CRUI-CARE Agreement.The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Netherlands Organization for Scientific Research (NWO), for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Spanish Agencia Estatal de Investigación, the Consellera d’Innovació, Universitats, Ciència i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, Spain, the National Science Centre of Poland and the European Union-European Regional Development Fund; Foundation for Polish Science (FNP), the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concertées (ARC) and Fonds Wetenschappelijk Onderzoek-Vlaanderen (FWO), Belgium, the European Commission. The authors gratefully acknowledge the support of the NSF, STFC, INFN, CNRS and Nikhef for provision of computational resources. Soumen Koley acknowledges the support through a collaboration agreement between Gran Sasso Science Institute and Nikhef and from the European Gravitational Observatory through a collaboration convention on Advanced Virgo +. The authors also gratefully acknowledge the support of the Italian Ministry of Education, University and Research within the PRIN 2017 Research Program Framework, n. 2017SYRTCN. Tomasz Bulik, Marek Cieslar, Mateusz Pietzak, and Mariusz Suchenek are supported by the grant “AstroCeNT: Particle Astrophysics Science and Technology Centre” (MAB/2018/7) carried out within the International Research Agendas programme of the Foundation for Polish Science (FNP) financed by the European Union under the European Regional Development Fund. Tomasz Bulik, Marek Cieslar, Mateusz Pietzak, and Mariusz Suchenek are supported by the funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 952480 (DarkWave). Tomasz Bulik and Bartosz Idzkowski were supported by the TEAM/2016-3/19 grant from the Foundation for Polish Science.
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