A Kerr-like rotating black hole spacetime with an added Dehnen halo term is analyzed for horizon, shadow, and quasinormal mode signatures.
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Investigating Optical and Ring-Down Gravitational Wave Properties of a Rotating Black Hole in a Dehnen Galactic Dark Matter Halo
A Kerr-like rotating black hole spacetime with an added Dehnen halo term is analyzed for horizon, shadow, and quasinormal mode signatures.