@Article{CostaAgui:2014:MiMaSc,
author = "Costa, Carlos Filipe da Silva and Aguiar, Odylio Denys de",
affiliation = "{Universidade de S{\~a}o Paulo (USP)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)}",
title = "Spherical gravitational wave detectors: MiniGRAIL and Mario
Schenberg",
journal = "Journal of Physics: Conference Series",
year = "2014",
volume = "484",
number = "1",
note = "{Proceedings of the 7th International Conference on Gravitation
and Cosmology (ICGC201}",
keywords = "Gravitational effects, Gravity waves, Spheres, Data analysis
techniques, Directional detections, Gravitational wave detectors,
Independent channels, Low latency, Off-line analysis, Sensitivity
improvements, Spherical detectors, Detectors.",
abstract = "Spherical gravitational wave detectors allow the analysis of
multiple independent channels and, therefore, are able to
determine gravitational wave directions and polarizations. There
are two spherical detectors being developed now: MiniGRAIL
(Netherlands) and Mario Schenberg (Brazil). Both share the same
principle of detection and main features. They have done
commissioning runs and shown progress in their development. We
have presented here the status of Mario Schenberg. Its transducers
have been redesigned for sensitivity improvements. While an
offline analysis was already developed for MiniGRAIL, we have
investigated a low latency data analysis technique for Mario
Schenberg. Both analysis are based on directional detection. ©
Published under licence by IOP Publishing Ltd.",
doi = "10.1088/1742-6596/484/1/012012",
url = "http://dx.doi.org/10.1088/1742-6596/484/1/012012",
issn = "1742-6588",
label = "scopus 2014-05 DaSilvaCostaAgui:2014:MiMaSc",
language = "en",
targetfile = "1742-6596_484_1_012012.pdf",
urlaccessdate = "27 abr. 2024"
}