Revisiting the double-binary-pulsar probe of non-dynamical Chern-Simons gravity

@inproceedings{AliHaimoud2011RevisitingTD,
  title={Revisiting the double-binary-pulsar probe of non-dynamical Chern-Simons gravity},
  author={Yacine Ali-Haimoud},
  year={2011}
}
One of the popular modifications to the theory of general relativity is non-dynamical Chern-Simons (CS) gravity, in which the metric is coupled to an externally prescribed scalar field. Setting accurate constraints to the parameters of the theory is important owing to their implications for the scalar field and/or the underlying fundamental theory. The current best constraints rely on measurements of the periastron precession rate in the double-binary-pulsar system and place a very tight bound… 

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