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@InProceedings{LiccardoFerrAguiOliv:2016:OpHiSe,
               author = "Liccardo, Vincenzo and Ferreira, Elvis Camilo and Aguiar, Odylio 
                         Denys de and Oliveira, Rog{\'e}rio de Moraes",
          affiliation = "{Instituto Tecnol{\'o}gico de Aeron{\'a}utica (ITA)} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
                title = "Optimization of high sensitivity parametric transducers for the 
                         Gravitational Wave detector “Mario Schenberg”",
            booktitle = "Proceedings...",
                 year = "2016",
               editor = "Navarro, Ram{\'o}n and Burge, James H.",
         organization = "Advances in Optical and Mechanical Technologies for Telescopes and 
                         Instrumentation, 2.",
                 note = "{Proceedings of SPIE}",
             keywords = "Antennas, Instrument optimisation, Cryogenic detectors, Resonant 
                         Detectors, Implantation, Material treatment.",
             abstract = "Parametric transducers may be used to monitor vibrational modes of 
                         resonant-mass Gravitational Wave (GW) detectors. This work focuses 
                         on the development and optimization of electromechanical 
                         transducers for the brazilian GW detector Mario Schenberg. We 
                         present the design and preliminary results for the optimization 
                         process of the last generation of the Schenberg parametric 
                         transduction system. Thanks to the results obtained from the last 
                         run of tests improvements for the transduction system will be 
                         planned and performed, in order to make the detector suitable for 
                         the searching of GW signals. The aim would be to obtain 
                         information about the direction and polarization of waves produced 
                         by astrophysical sources in the frequency bands of the spherical 
                         detector resonant modes.",
  conference-location = "Edinburgh, United Kingdom",
      conference-year = "26 June - 01 July",
             language = "en",
               volume = "9912",
        urlaccessdate = "16 jan. 2021"
}


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