On the behaviour of the magnetorotational instability when the Rayleigh criterion is violated

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...

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Main Author: Balbus, S
Format: Journal article
Language:English
Published: 2012
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author Balbus, S
author_facet Balbus, S
author_sort Balbus, S
collection OXFORD
description 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. © 2012 The Author. Monthly Notices of the Royal Astronomical Society. © 2012 RAS.
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spelling oxford-uuid:7560e780-d5ac-48ce-a853-3bff8d98c1d12022-03-26T20:09:00ZOn the behaviour of the magnetorotational instability when the Rayleigh criterion is violatedJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:7560e780-d5ac-48ce-a853-3bff8d98c1d1EnglishSymplectic Elements at Oxford2012Balbus, SAn 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. © 2012 The Author. Monthly Notices of the Royal Astronomical Society. © 2012 RAS.
spellingShingle Balbus, S
On the behaviour of the magnetorotational instability when the Rayleigh criterion is violated
title On the behaviour of the magnetorotational instability when the Rayleigh criterion is violated
title_full On the behaviour of the magnetorotational instability when the Rayleigh criterion is violated
title_fullStr On the behaviour of the magnetorotational instability when the Rayleigh criterion is violated
title_full_unstemmed On the behaviour of the magnetorotational instability when the Rayleigh criterion is violated
title_short On the behaviour of the magnetorotational instability when the Rayleigh criterion is violated
title_sort on the behaviour of the magnetorotational instability when the rayleigh criterion is violated
work_keys_str_mv AT balbuss onthebehaviourofthemagnetorotationalinstabilitywhentherayleighcriterionisviolated