No CrossRef data available.
Article contents
Binary Pulsar Tests of General Relativity in the Presence of Low-Frequency Noise
Published online by Cambridge University Press: 12 April 2016
Abstract
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.
- Type
- Part 2. Timing, General Relativity and Astrometry
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 117 - 120
- Copyright
- Copyright © Astronomical Society of the Pacific 2000