%0 Journal Article
%4 sid.inpe.br/mtc-m17@80/2007/12.19.12.59
%2 sid.inpe.br/mtc-m17@80/2007/12.19.12.59.44
%@doi 10.1007/s10714-007-0524-1
%@issn 0001-7701
%T Astrophysics from data analysis of spherical gravitational wave detectors
%D 2008
%8 Jan.
%A Lenzi, César H.,
%A Magalhães, Nadja S.,
%A Costa, César Augusto,
%A Marinho Júnior, Rubens M.,
%A Araújo, Helmo A. B.,
%A Aguiar, Odylio Denys de,
%@affiliation Departamento de Física, Instituto Tecnológico de Aeronáutica
%@affiliation Centro Federal de Educação Tecnológica de São Paulo
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Departamento de Física, Instituto Tecnológico de Aeronáutica
%@affiliation Departamento de Física, Instituto Tecnológico de Aeronáutica
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%B General Relativity and Gravitation
%V 40
%N 1
%P 183-190
%K Gravitational waves - Spherical gravitational wave detector - Inverse problem solution - Method of independent bars.
%X The direct detection of gravitational waves will provide valuable astrophysical information about many celestial objects. Also, it will be an important test to general relativity and other theories of gravitation. The gravitational wave detector SCHENBERG has recently undergone its first test run. It is expected to have its first scientific run soon. In this work the data analysis system of this spherical, resonant mass detector is tested through the simulation of the detection of gravitational waves generated during the inspiralling phase of a binary system. It is shown from the simulated data that it is not necessary to have all six transducers operational in order to determine the sources direction and the waves amplitudes.
%@language en
%3 astrophysics from data.pdf