Search for periodic gravitational radiation with the ALLEGRO gravitational wave detector

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dc.creatorMauceli, E.
dc.creatorMcHugh, M. P.
dc.creatorHamilton, W. O.
dc.creatorJohnson, W. W.
dc.creatorMorse, A.
dc.date2000-07-11
dc.date.accessioned2026-07-07T03:25:08Z
dc.date.available2026-07-07T03:25:08Z
dc.descriptionWe describe the search for a continuous signal of gravitational radiation from a rotating neutron star in the data taken by the ALLEGRO gravitational wave detector in early 1994. Since ALLEGRO is sensitive at frequencies near 1 kHz, only neutron stars with spin periods near 2 ms are potential sources. There are no known sources of this typ e for ALLEGRO, so we directed the search towards both the galactic center and the globular clus ter 47 Tucanae. The analysis puts a constraint of roughly $8 \times 10^{-24}$ at frequencies near 1 kHz on the gravitational strain emitted from pulsar spin-down in either 47 Tucanae or the galactic center.
dc.description14 pages, 10 figures. Submitted to PRD
dc.identifierhttps://arxiv.org/abs/gr-qc/0007023
dc.identifierhttp://arxiv.org/abs/gr-qc/0007023
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33595
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSearch for periodic gravitational radiation with the ALLEGRO gravitational wave detector
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