Sensitivity of the low frequency facility experiment around 10 Hz
Year: 2004
Authors: Di Virgilio A., Braccini S., Ballardin G., Bradaschia C., Cella G., Cuoco, E., Dattilo V., Ferrante I., Fidecaro F., Frasconi F., Giazotto A., Gennai A., Holloway L. H., La Penna P., Losurdo G., Paoletti, F., Pasqualetti A., Passaquieti R., Passuello D., Porzio A., Puppo P., Raffaelli F., Rapagnani P., Ricci F., Ricciardi J., Solimeno S., Stanga R., Vetrano F., Zhang, Z.
Autors Affiliation: Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Pisa, Italy;
EGO, European Gravitational Observatory, Cascina (Pi), Italy
Università di Pisa, Pisa, Italy
INFN Sezione di Firenze, Sesto Fiorentino, Italy
Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Dipartimento di Scienze Fisiche, Università di Napoli “Federico II”, Napoli, Italy
Università di Roma, Roma 1, Roma, Italy
Università di Urbino, Urbino, Italy
Abstract: The reduction of thermal noise is a fundamental issue for the improvement of future gravitational wave antennas. The main purpose of the Low Frequency Facility (LFF) is to study pendulum thermal noise in the region of 10 Hz. Data at the LFF has been taking since the beginning of 2003 and has been analyzed in order to thoroughly understand the region around 10 Hz. Above 7 Hz. the displacement noise floor is at the level of 10(-14) m/rootHz, decreasing with frequency approximately as 1/v. Seismic noise contamination is not observed above a few Hz. (C) 2004 Elsevier B.V. All rights reserved.
Journal/Review: PHYSICS LETTERS A
Volume: 322 (1-2) Pages from: 1 to: 9
More Information: doi: 10.1016/j.physleta.2003.12.059KeyWords: Low Frequency FacilityDOI: 10.1016/j.physleta.2003.12.059ImpactFactor: 1.454Citations: 5data from “WEB OF SCIENCE” (of Thomson Reuters) are update at: 2024-11-24References taken from IsiWeb of Knowledge: (subscribers only)Connecting to view paper tab on IsiWeb: Click hereConnecting to view citations from IsiWeb: Click here
