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@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 = "15 jan. 2021"
}


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