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arXiv · 1810.01421

A New Probe of Dark Matter-Induced Fifth Force with Neutron Star Inspirals

Han Gil Choi·Sunghoon Jung
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Abstract

A light scalar dark matter (DM) is allowed in a wide range of the mass and interaction types. We show that the light scalar DM may be probed in a new way from final years of neutron-star (NS) binary inspirals. If the DM interacts with the neutron, its long wave coherence in the background can induce the time-oscillating mass shift, to which the binary inspiral is inherently sensitive. But the sensitivity is found to be significantly enhanced by a large number of gravitational-wave (GW) cycles during year-long highest-frequency measurements in the broadband $f \simeq 0.01-1000$ Hz. The future broadband detector networks including LIGO-band detectors can probe unconstrained parameter space of the light scalar DM.

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BibTeXRIS

Han Gil Choi, Sunghoon Jung. 2018-10-02. A New Probe of Dark Matter-Induced Fifth Force with Neutron Star Inspirals. https://doi.org/10.1103/physrevd.99.015013

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