Open AccessOn the behaviour of the magnetorotational instability when the Rayleigh criterion is violated
Author(s) -
Balbus Steven A.
Publication year - 2012
Publication title -
monthly notices of the royal astronomical society: letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.067
H-Index - 122
eISSN - 1745-3933
pISSN - 1745-3925
DOI - 10.1111/j.1745-3933.2012.01255.x
Subject(s) - magnetorotational instability , physics , wavenumber , instability , radius , mechanics , viscous stress tensor , discriminant , tensor (intrinsic definition) , eigenvalues and eigenvectors , stress (linguistics) , dispersion relation , cauchy stress tensor , rayleigh scattering , classical mechanics , geometry , magnetic field , mathematics , magnetohydrodynamics , optics , quantum mechanics , artificial intelligence , computer security , computer science , linguistics , philosophy
An elementary but revealing analysis of the dispersion relation of the magnetorotational instability (MRI) in the Ralyeigh‐unstable regime is described. The defining properties of the MRI – its maximum growth rate and the direction of the associated eigenvector displacement – remain unchanged as the Rayleigh discriminant passes from positive to negative values. At sufficiently negative discriminant values, however, the spectrum of unstable modes becomes dominated by zero wavenumber disturbances, and the problem loses its local character. These results may be relevant to understanding the level of turbulent fluid stress near the innermost stable circular orbit (ISCO) in an accretion disc around a black hole, since the Rayleigh discriminant changes sign at this location. Our conclusions are consistent with numerical simulations that find finite stress at the ISCO, some dependence of the stress magnitude with scale height, and a plunging region much closer to the event horizon than the ISCO radius.