Timing Effects of Gravitational Waves from Localized Sources

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dc.creatorKopeikin, Sergei M.
dc.date1999-03-18
dc.date.accessioned2026-07-07T03:33:03Z
dc.date.available2026-07-07T03:33:03Z
dc.descriptionLocalized astronomical sources like a double stellar system, rotating neutron star, or a massive black hole at the center of the Milky Way emit periodic gravitational waves. For a long time only a far-zone contribution of gravitational fields of the localized sources (plane-wave-front approximation) were a matter of theoretical analysis. We demonstrate how this analysis can be extended to take into account near-zone and intermediate-zone contributions as well. The formalism is used to calculate gravitational-wave corrections to the Shapiro time delay in binary pulsars and low-frequency (LF) pulsar timing noise produced by an ensemble of double stars in our galaxy.
dc.description6 pages, 2 figures, a talk given at the XXXIVth Rencontres de Moriond on "Gravitational Waves and Experimental Gravity", Les Arcs, 23-30 January 1999
dc.identifierhttps://arxiv.org/abs/gr-qc/9903070
dc.identifierhttp://arxiv.org/abs/gr-qc/9903070
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36469
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleTiming Effects of Gravitational Waves from Localized Sources
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