ROLE OF THE HALL EFFECT ON THE MAGNETOROTATIONAL INSTABILITY

DOI10.1142/S0218271810016634zbMath1197.85020OpenAlexW2060167498MaRDI QIDQ4929694

Daniel Gómez, Cecilia Bejarano

Publication date: 23 September 2010

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0218271810016634

zbMATH Keywords

magnetohydrodynamicsinstabilitiesaccretion disks

Mathematics Subject Classification ID

Quantum field theory on curved space or space-time backgrounds (81T20) Magnetohydrodynamics and electrohydrodynamics (76W05) Electromagnetic fields in general relativity and gravitational theory (83C50) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

• Accretion disk instability revisited
• Hydrodynamic response of rotationally supported flows in the small shearing box model
• Hydrodynamic stability of rotationally supported flows: Linear and nonlinear 2D shearing box results
• On the relevance of subcritical hydrodynamic turbulence to accretion disk transport

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