Detectability of compact intermediate-mass black hole binaries as low-frequency gravitational wave sources: The influence of dynamical friction of dark matter

Open Access

Fig. 1.

Dark matter density profiles with different spike indices around an IMBH of M_BH = 1000 M_⊙. The vertical dashed orange line indicates a radius of r = 2.93 × 10¹² cm, which is the orbital separation of a system consisting of a 1000 M_⊙ IMBH and a 1 M_⊙ MS star in a 1.0-day orbit.

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