Dark matter bar strength in Milky Way analogs grows with initial halo spin and saturates at a spin-dependent level, while the final bar pattern speed is nearly spin-independent.
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The Role of Inner Halo Angular Momentum (Spin) in Shaping Dark Matter Bars in Milky Way Analogs
Dark matter bar strength in Milky Way analogs grows with initial halo spin and saturates at a spin-dependent level, while the final bar pattern speed is nearly spin-independent.