Transducers for the Brazilian gravitational wave detector 'Mario Schenberg'

Details Transducers for the Brazilian gravitational wave detector 'Mario Schenberg' Transducers for the Brazilian gravitational wave detector 'Mario Schenberg'

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cqgra..19.1961f&link_type=abstract

Classical and Quantum Gravity, Volume 19, Issue 7, pp. 1961-1965 (2002).

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Scientific paper

'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 1 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.

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