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Accelerated Reissner-Nordstrom black hole in a swirling, magnetic universe
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We present a new solution in Einstein's theory of relativity, found through the use of the symmetries of the Ernst equations and in particular the Harrison and Ehlers transformations. The new metric represents a Reissner-Nordstr\"om black hole immersed in a magnetic, rotating universe. We analyse the physical properties, such as conical singularities and ergoregions, and then proceed to immerse the accelerated version of the Reissner-Nordstr\"om black hole in the same background. We finally analyse its properties and attempt to regularise the spacetime.
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Cited by 1 Pith paper
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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.
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