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Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/12317

Detection of scalar gravitational waves with a hollow spherical antenna

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We study the response and cross sections for the absorption of GW energy generated in a Jordan-Brans-Dicke theory by a resonant mass detector shaped as a hollow sphere. As a source of the GW we take a binary system in the Newtonian approximation. For masses of the stars of the order of the solar mass, the emitted GW sweeps a range of frequencies which include the first resonant mode of the detector.

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COCCIA, E. (Eugenio), et al. Detection of scalar gravitational waves with a hollow spherical antenna. Physical Review D. 2000. Vol. 62, num. núm 4, pags. 044019-1-044019-7. ISSN 0556-2821. [consulted: 15 of August of 2026]. Available at: https://hdl.handle.net/2445/12317

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