A noise model for the Brazilian gravitational wave detector 'Mario Schenberg'

Details A noise model for the Brazilian gravitational wave detector 'Mario Schenberg' A noise model for the Brazilian gravitational wave detector 'Mario Schenberg'

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cqgra..21s1107f&link_type=abstract

Classical and Quantum Gravity, Volume 21, Issue 5, pp. S1107-S1111 (2004).

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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 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.

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