Swirling-Kerr disks heat up in the inner region, dim in the outer region, shift their spectrum, and convert mass to radiation less efficiently as the swirl parameter grows.
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Thin accretion disk around a Kerr black hole immersed in swirling universes
Swirling-Kerr disks heat up in the inner region, dim in the outer region, shift their spectrum, and convert mass to radiation less efficiently as the swirl parameter grows.