A noise model for the Brazilian gravitational wave detector Mario Schenberg

Autor:	Odylio D. Aguiar, Nadja S. Magalhães, Carlos Frajuca, Rubens M. Marinho, K L Ribeiro, Luiz Alberto de Andrade
Rok vydání:	2004
Předmět:	Mechanical system Physics Gravitational-wave observatory Optics Physics and Astronomy (miscellaneous) Physics::Instrumentation and Detectors business.industry Gravitational wave Bandwidth (signal processing) Detector High Energy Physics::Experiment business
Zdroj:	Classical and Quantum Gravity. 21:S1107-S1111
ISSN:	1361-6382 0264-9381
DOI:	10.1088/0264-9381/21/5/107
Popis:	'Mario Schenberg' is a spherical resonant-mass gravitational wave (GW) detector that will be part of a GW detection array of three detectors. The other two will be built in Italy and in The Netherlands. Their resonant frequencies will be around 3.2 kHz with a bandwidth of about 200 Hz. This range of frequencies is new in a field where the typical frequencies lay below 1 kHz, making the development of the mechanical system much more complex. In this work, a noise model of the detector is presented, where all main sources of noise were taken into account. The final goal is to calculate the expected sensitivity of the detector, analysing which parameters must be changed to improve this.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::79f7bf8e78b09c39b28b2726fa4f9d75 https://doi.org/10.1088/0264-9381/21/5/107 Zobrazit plný text záznamu