%0 Journal Article
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%@nexthigherunit 8JMKD3MGPCW/3ETR8EH
%@archivingpolicy denypublisher denyfinaldraft12
%@issn 0264-9381
%@resumeid
%@resumeid
%@resumeid
%@resumeid 8JMKD3MGP5W/3C9JJ2A
%@usergroup administrator
%@usergroup marciana
%@usergroup valdirene
%3 A noise model for the Brazilian gw detector.pdf
%B Classical and Quantum Gravity
%@dissemination WEBSCI; PORTALCAPES; COMPENDEX.
%X "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.
%8 Mar.
%N 5
%@secondarydate 20040212
%T A noise model for the Brazilian gravitational wave detector "Mario Schenberg"
%K parametric transducer, antena, radiation.
%@secondarytype PRE PI
%@group DAS-INPE-MCT-BR
%@e-mailaddress frajuca@cefetsp.br
%@copyholder SID/SCD
%@secondarykey INPE-10786-PRE/6243
%2 sid.inpe.br/jeferson/2004/06.29.10.54.24
%@affiliation Centro Federal de Educacao Tecnologica de Sao Paulo
%@affiliation Divisao de Astrofisica - Instituto Nacional de Pesquisas Espaciais
%@affiliation Instituto Tecnologica de Aeronautica - Departamento de Física
%P S1107 - S1111
%4 sid.inpe.br/jeferson/2004/06.29.10.54
%D 2004
%V 21
%A Frajuca, Carlos,
%A Leite, Ribeiro Kilder,
%A Andrade, Luiz  A,
%A Aguiar, Odylio Denys de,
%A Magalhães, Nadja Simão,
%A Marino Jr, Rubens de Melo,
%@ 0264-938
%@area CEA