Search for continuous gravitational wave signals from sources in binary systems

Simple item page
dc.creatorDhurandhar, S. V.
dc.creatorVecchio, A.
dc.date1999-11-26
dc.date.accessioned2026-07-07T03:33:44Z
dc.date.available2026-07-07T03:33:44Z
dc.descriptionWe analyze the computational costs of searches for continuous monochromatic gravitational waves emitted by rotating neutron stars orbiting a companion object. As a function of the relevant orbital parameters, we address the computational load involved in targeted searches, where the position of the source is known; the results are applied to known binary radio pulsars and Sco-X1.
dc.description6 pages, 1 figure, To appear in the proceedings of the Second Tama Workshop
dc.identifierhttps://arxiv.org/abs/gr-qc/9911102
dc.identifierhttp://arxiv.org/abs/gr-qc/9911102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36693
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSearch for continuous gravitational wave signals from sources in binary systems
dc.typetext

Files

Collections

arXiv