Noisy Spherical Resonant Detector of Gravitational Waves: Veto on the Longitudinal Part of the Signal

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dc.creatorMontanari, Enrico
dc.date1998-01-05
dc.date.accessioned2026-07-07T03:32:08Z
dc.date.available2026-07-07T03:32:08Z
dc.descriptionThe equations of a resonant sphere in interaction with $N$ secondary radial oscillators (transducers) on its surface have been found in the context of Lagrangian formalism. It has been shown the possibility to exert a veto against spurious events measuring the longitudinal component of a signal. Numerical simulations has been performed, which take into account thermal noise between resonators and the sphere surface, for a particular configuration of the transducers.
dc.description16 pages 2 ps-figures; revtex; accepted for publication in Nuovo Cimento B
dc.identifierhttps://arxiv.org/abs/gr-qc/9801006
dc.identifierhttp://arxiv.org/abs/gr-qc/9801006
dc.identifierNuovo Cim. B113 (1998) 1025-1046
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36117
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleNoisy Spherical Resonant Detector of Gravitational Waves: Veto on the Longitudinal Part of the Signal
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