@Article{FrajucaRiAnVeAgMa:2002:TrBrGr,
author = "Frajuca, Carlos and Ribeiro, Kilder Leite and Andrade, Luiz A. de
and Velloso J{\'u}nior, Walter Ferreira and Aguiar, Odylio Denys
de and Magalh{\~a}es, Nadja Sim{\~a}o",
title = "Transducers for the Brazilian gravitational wave detector {"}Mario
Schenberg{"}",
journal = "Classical and Quantum Gravity",
year = "2002",
volume = "19",
number = "7",
pages = "1961--1965",
month = "Abr.",
keywords = "ASTROF{\'{\I}}SICA, radiation, gravitational waves, detectors,
radia{\c{c}}{\~a}o, ondas gravitacionais, detectores.",
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 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 lie below I kHz, making
the transducer development much more complex. In this paper, the
design of the mechanical part of the transducer will be shown, as
well as the attachment method to the sphere and the expected
sensitivity.",
doi = "10.1088/0264-9381/19/7/399",
url = "http://dx.doi.org/10.1088/0264-9381/19/7/399",
issn = "0264-9381",
label = "9964",
language = "en",
targetfile = "0264-9381_19_7_399.pdf",
urlaccessdate = "27 abr. 2024"
}