Author(s): Alexander Haywood and Fatima Ebrahimi
Understanding the behavior of differentially rotating plasmas is important for the study of turbulence and transport in systems such as accretion disks and stellar interiors, as well as in laboratory experiments. The authors use various techniques to analyze the stability of these systems, in particular focusing on the competition between the magneto-rotational instability and the magneto-curvature instability.
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[Phys. Rev. E 112, 055207] Published Mon Nov 17, 2025