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Updated: Jul 7, 2026

06:42
Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Comment on "Helical magnetorotational instability in magnetized Taylor-Couette flow"
Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics
|February 1, 2008
Abstract:
Liu [Phys. Rev. E 74, 056302 (2006)] have presented a WKB analysis of the helical magnetorotational instability (HMRI), and claim that it does not exist for Keplerian rotation profiles. We show that, if radial boundary conditions are included, the HMRI can exist even for rotation profiles as flat as Keplerian, provided only that at least one of the boundaries is sufficiently conducting.
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