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Reconstructing the Dark Matter Equation of State with Compact Object Inspirals
general-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenahigh-energy-physics-phenomenology
We investigate the gravitational wave (GW) signatures of compact binaries embedded in extended dark matter (DM) configurations in hydrostatic equilibrium. If a neutron star is surrounded by a sufficiently massive and extended envelope, an inspiraling companion experiences dynamical friction (DF) in
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