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Gravitational wave probes of dark matter: challenges and opportunities
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In this white paper, we discuss the prospects for characterizing and identifying dark matter using gravitational waves, covering a wide range of dark matter candidate types and signals. We argue that present and upcoming gravitational wave probes offer unprecedented opportunities for unraveling the nature of dark matter and we identify the most urgent challenges and open problems with the aim of encouraging a strong community effort at the interface between these two exciting fields of research.
Forward citations
Cited by 7 Pith papers
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BinaryGFH-v2: Improved method to search for gravitational waves from sub-solar-mass, ultra-compact binaries using the Generalized Frequency-Hough Transform
BinaryGFH-v2 is a modified GFH method that can search for inspiraling binaries with chirp masses 0.01–0.1 solar masses, validated in Gaussian noise and projected to constrain PBH dark matter.
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Tidal Love numbers and quasi-normal modes of the Schwarzschild-Hernquist black hole
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Static dark matter halos around Schwarzschild black holes are viable only if the dark matter pressure is negative, under two toy equations of state and a vanishing horizon-density boundary condition.
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