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2018

Hidden-Sector Modifications to Gravitational Waves From Binary Inspirals

Alexander, Stephon, McDonough, Evan, Sims, Robert et al.

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Gravitational wave astronomy has placed strong constraints on fundamental physics, and there is every expectation that future observations will continue to do so.

In this work we quantify this expectation for future binary merger observations to constrain hidden sectors, such as scalar-tensor gravity or dark matter, which induce a Yukawa-type modification to the gravitational potential.
We explicitly compute the gravitational waveform, and perform a Fisher information matrix analysis to estimate the sensitivity of next generation gravitational wave detectors to these modifications.
We find an optimal sensitivity to the Yukawa interaction strength of $10^{-5}$ and to the associated dipole emission parameter of $10^{-7}$, with the best constraints arising from the Einstein Telescope.

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