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.
Font, Numerical Hydrodynamics and Magnetohydrodynamics in General Relativity , Living Rev
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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.