Binary Pulsar Tests of General Relativity in the Presence of Low-Frequency Noise

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dc.creatorKopeikin, Sergei M.
dc.creatorPotapov, Vladimir A.
dc.date1999-11-22
dc.date.accessioned2026-07-07T02:34:35Z
dc.date.available2026-07-07T02:34:35Z
dc.descriptionThe influence of the low-frequency timing noise on the precision of measurements of the Keplerian and post-Keplerian orbital parameters in binary pulsars is studied. Fundamental limits on the accuracy of tests of alternative theories of gravity in the strong-field regime are established. The gravitational low-frequency timing noise formed by an ensemble of binary stars is briefly discussed.
dc.description4 pages, contributed paper to the proceedings of the IAU167 colloquium on pulsars, Bonn, August-September 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/9911408
dc.identifierhttp://arxiv.org/abs/astro-ph/9911408
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15301
dc.subjectAstrophysics
dc.titleBinary Pulsar Tests of General Relativity in the Presence of Low-Frequency Noise
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