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Rotating and twisting locally rotationally symmetric imperfect fluids
Published 17 Oct 2017 in gr-qc | (1710.06179v2)
Abstract: Rotating and twisting locally rotationally symmetric imperfect fluids in general relativity admit a much larger set of solutions than the self-similar ones recently suggested in the literature. Explicit forms of the metrics are given and the self-similar sub-cases are discussed.
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