Gravitational Waves from Quasi-Circular Black Hole Binaries in Dynamical   Chern-Simons Gravity
  Dynamical Chern-Simons gravity cannot be strongly constrained with current experiments because it reduces to General Relativity in the weak-field limit. This theory, however, introduces modifications in the non-linear, dynamical regime, and thus, it could be greatly constrained with gravitational waves from the late inspiral of black hole binaries. We complete the first self-consistent calculation of such gravitational waves in this theory. For favorable spin-orientations, advanced ground-based detectors may improve existing solar-system constraints by 6 orders of magnitude. 
Kent Yagi, Nicolas Yunes, Takahiro Tanaka
gr-qc astro-ph.CO