Stairs (2003) provided an introduction to testing theories of gravity using pulsar observations. The search for gravitational wave (a prediction of general relativity and other theories of gravity) is discussed elsewhere. Here, we consider verifying the predictions of various theories of gravity and the possible violation of equivalence principles using binary pulsars. The majority of binary pulsar orbits are adequately described by the five Keplerian parameters:
the orbital period,
the projected semi-major axis,
the longitude of periastron,
the epoch of periastron,
However, in some cases significant residuals are still present are fitting for the Keplerian parameters. In such cases one or more post-Keplerian (PK) parameters are required in the timing model.