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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Extending the range of the inductionless magnetorotational instability
Oleg N Kirillov1, Frank Stefani
1Helmholtz-Zentrum Dresden-Rossendorf, P.O. Box 510119, D-01314 Dresden, Germany. o.kirillov@hzdr.de
Physical Review Letters
|August 27, 2013
Summary
Inductionless magnetorotational instability (MRI) variants can destabilize accretion disks even in low magnetic Reynolds number regions. This research extends MRI applicability by analyzing helical and azimuthal MRI on Keplerian profiles.
Area of Science:
- Plasma Physics
- Astrophysical Fluid Dynamics
- Magnetohydrodynamics
Background:
- The magnetorotational instability (MRI) is crucial for angular momentum transport in accretion disks.
- A significant limitation of the MRI is its questionable effectiveness in regions with low magnetic Reynolds numbers.
- Previous studies established critical Rossby number limits (Liu limits) for MRI stability.
Purpose of the Study:
- To extend the applicability of the MRI to regions with low magnetic Reynolds numbers.
- To investigate the destabilizing effects of inductionless MRI variants on accretion disk profiles.
- To connect the lower and upper Liu limits of the critical Rossby number.
Main Methods:
- Utilized the WKB method for analyzing wave propagation and stability.
- Examined inductionless MRI variants, specifically helical and azimuthal MRI.
- Investigated the destabilization of Keplerian profiles (∝r(-3/2)) with modified azimuthal magnetic fields (∝r(-1)).
Main Results:
- Demonstrated that inductionless MRI variants can destabilize hydrodynamically stable Keplerian flows.
- Showed that slight modifications to the current-free azimuthal magnetic field profile enhance instability.
- Established a natural connection between the lower Liu limit (Ro≈-0.828) and the upper Liu limit (Ro≈+4.828).
Conclusions:
- Inductionless MRI variants significantly broaden the conditions under which MRI can operate in accretion disks.
- The study overcomes the limitations of low magnetic Reynolds number applicability for MRI.
- This work provides a unified understanding of MRI stability across a wider range of Rossby numbers.
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