@Article{FrajucaLeAnAgMaMa:2004:NoMoBr,
author = "Frajuca, Carlos and Leite, Ribeiro Kilder and Andrade, Luiz A and
Aguiar, Odylio Denys de and Magalh{\~a}es, Nadja Sim{\~a}o and
Marino Jr, Rubens de Melo",
affiliation = "{Centro Federal de Educacao Tecnologica de Sao Paulo} and {Divisao
de Astrofisica - Instituto Nacional de Pesquisas Espaciais} and
{Instituto Tecnologica de Aeronautica - Departamento de
F{\'{\i}}sica}",
title = "A noise model for the Brazilian gravitational wave detector
{"}Mario Schenberg{"}",
journal = "Classical and Quantum Gravity",
year = "2004",
volume = "21",
number = "5",
pages = "S1107 - S1111",
month = "Mar.",
keywords = "parametric transducer, antena, radiation.",
abstract = "{"}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.",
copyholder = "SID/SCD",
isbn/issn = "0264-938",
issn = "0264-9381",
language = "en",
targetfile = "A noise model for the Brazilian gw detector.pdf",
urlaccessdate = "27 abr. 2024"
}