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The Brazilian gravitational wave detector Mario Schenberg: progress and plans

Authors :
S R Furtado
Odylio D. Aguiar
A U de Lucena
Nadja S. Magalhães
K M F Costa
A C Fauth
W F Velloso
W. de Paula
C Stellati
L A Carneiro
Joaquim J. Barroso
L A Andrade
C. A. Costa
Bruno Woltzenlogel Paleo
Nei F. Oliveira
J. C. N. de Araujo
M Remy
J. Weber
E C de Rey Neto
Carlos Frajuca
K L Ribeiro
Giorgio Frossati
Pedro J. Castro
S.L.T. de Souza
Oswaldo D. Miranda
J L Melo
E S Matos
Rubens M. Marinho
F. S. Bortoli
Source :
Classical and Quantum Gravity. 22:S209-S214
Publication Year :
2005
Publisher :
IOP Publishing, 2005.

Abstract

The Schenberg gravitational wave detector is almost completed for operation at its site in the Physics Institute of the University of Sao 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.

Details

ISSN :
13616382 and 02649381
Volume :
22
Database :
OpenAIRE
Journal :
Classical and Quantum Gravity
Accession number :
edsair.doi...........6b3052c586262ff39173c2d1a92a301f
Full Text :
https://doi.org/10.1088/0264-9381/22/10/011