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Phys. Rev. D 72, 102003 (2005) [5 pages]

Can lightning be a noise source for a spherical gravitational wave antenna?

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Nadja Simão Magalhães1,2,*, Rubens de Melo Marinho, Jr.2, Odylio Denys de Aguiar3, and Carlos Frajuca1
1Centro Federal de Educação Tecnólogica de São Paulo, Rua Pedro Vicente 625, São Paulo, SP 01109-010, Brazil and
2Departamento de Física, Instituto Tecnológico de Aeronáutica, Pça. Mal. Eduardo Gomes 50, São José dos Campos, SP 12228-900, Brazil
3Divisão de Astrofísica, Instituto Nacional de Pesquisas Espaciais, Av . dos Astronautas 1758, São José dos Campos, SP 12227-010, Brazil

Received 31 July 2005; published 16 November 2005

The detection of gravitational waves is a very active research field at the moment. In Brazil the gravitational wave detector is called Mario SCHENBERG. Because of its high sensitivity it is necessary to model mathematically all known noise sources so that digital filters can be developed that maximize the signal-to-noise ratio. One of the noise sources that must be considered are the disturbances caused by electromagnetic pulses due to lightnings close to the experiment. Such disturbances may influence the vibrations of the antenna’s normal modes and mask possible gravitational wave signals. In this work we model the interaction between lightnings and SCHENBERG antenna and calculate the intensity of the noise due to a close lightning stroke in the detected signal. We find that the noise generated does not disturb the experiment significantly.

© 2005 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.72.102003
DOI:
10.1103/PhysRevD.72.102003
PACS:
04.80.Nn, 41.20.Jb, 42.25.Bs, 92.60.Pw

*Electronic address: nadjam@ig.com.br