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Gravitational Waves from Quasi-Circular Black Hole Binaries in Dynamical Chern-Simons Gravity

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arxiv 1208.5102 v4 pith:LTXRNNYB submitted 2012-08-25 gr-qc astro-ph.CO

Kent Yagi , Nicolas Yunes , Takahiro Tanaka This is my paper · ORCID
classification gr-qcastro-ph.CO
keywords dynamicalgravitationalwavesbinariesblackchern-simonsconstrainedgravity
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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.

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Cited by 6 Pith papers

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    Scalar hair on spinning compact objects is described by a conformal coupling of matter to a massless scalar, yielding matching waveforms and energy loss formulas for scalar-tensor gravity binaries.

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