@Article{AguiarLPRSFFFFMMAMMMOPRRSVWBBCCCCA:2005:PrPl,
author = "Aguiar, Odylio Denys de and Lucena, Ant{\^o}nio Unias de and de
Paula, W. and de Rey Neto, E. C and de Souza, S. T. and Fauth, A.
C. and Frajuca, C. and Frossati, G. and Furtado, Sergio Ricardo
and Magalh{\~a}es, N. S. and Marinho Jr., R. M. and Andrade, L. A
and Matos, E. S. and Melo, Jos{\'e} Luiz and Miranda, Oswaldo
Duarte and Oliveira Jr., N. F. and Paleo, B. W. and Remy, M. and
Ribeiro, K. L. and Stellati, C. and Velloso Jr., W. F. and Weber,
Jorge and Barroso, Joaquim Jos{\'e} and Bortoli, F. and Carneiro,
Leandro Alves and Castro, Pedro Jose de and Costa, Cesar Augusto
and Costa, K. M. F and Ara{\'u}jo, Jos{\'e} Carlos Neves de",
affiliation = "Instituto Nacional de Pesquisas Espaciais, Divis{\~a}o de
Astrof{\'{\i}}sica (INPE, DAS)",
title = "The brazilian gravitational wave detector Mario Schenberg:
progress and plans",
journal = "Classical and Quantum Gravity",
year = "2005",
volume = "22",
number = "10",
pages = "S209--S214",
month = "Sept",
abstract = "The Schenberg gravitational wave detector is almost completed for
operation at its site in the Physics Institute of the University
of S{\~a}o Paulo, under the full support of FAPESP (the Sao Paulo
State Foundation for Research Support). We have been working on
the development of a transducer system, which will be installed
after the arrival of all the microwave components and the
completion of the transducer mechanical parts. The initial plan is
to operate a CuAl6% two-mode parametric transducer in a first
operational run at 4.2 K with nine transducers and an initial
target sensitivity of h \∼ 2 × 10\−21 Hz\−1/2
in a 50 Hz bandwidth around 3.2 kHz. Here we present details of
this plan and some recent results of the development of this
project.",
copyholder = "SID/SCD",
issn = "0264-9381",
language = "en",
targetfile = "aguiar-brazilian.pdf",
urlaccessdate = "27 abr. 2024"
}