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Pulsar Timing Observations and Tests of General Relativity in Double-Neutron-Star Binaries

I. H. Stairs
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Abstract

We describe the techniques used in pulsar timing observations, and show how these observations may be applied to tests of strong-field general relativity for double-neutron-star binary systems. We describe the tests of GR resulting from the PSRs B1913+16 and B1534+12 systems. For the latter pulsar, 5 "Post-Keplerian" timing parameters are measurable, including the orbital period derivative and the two Shapiro delay parameters.

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I. H. Stairs. 2001-05-04. Pulsar Timing Observations and Tests of General Relativity in Double-Neutron-Star Binaries. https://doi.org/10.1142/9789812777386_0377

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