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

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

1999-11-22

arxiv.org/abs/astro-ph/9911408v1

Astronomy and Astrophysics

Astrophysics

4 pages, contributed paper to the proceedings of the IAU167 colloquium on pulsars, Bonn, August-September 1999

Scientific paper

The 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.

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