Absolute stability of axisymmetric perturbations in strongly-magnetized collisionless axisymmetric accretion disk plasmas

Abstract

The physical mechanism responsible for driving accretion flows in astrophysical accretion disks is commonly thought to be related to the development of plasma instabilities and turbulence. A key question is therefore the determination of consistent equilibrium configurations for accretion-disk plasmas and investigation of their stability properties. In the case of collisionless plasmas kinetic theory provides the appropriate theoretical framework. This paper presents a kinetic description of low-frequency and long-wavelength axisymmetric electromagnetic perturbations in non-relativistic, strongly-magnetized and gravitationally-bound axisymmetric accretion-disk plasmas in the collisionless regime. The analysis, carried out within the framework of the Vlasov-Maxwell description, relies on stationary kinetic solutions of the Vlasov equation which allow for the simultaneous treatment of non-uniform fluid fields, stationary accretion flows and temperature anisotropies. It is demonstrated that, for such solutions, no axisymmetric unstable perturbations can exist occurring on characteristic time and space scales which are long compared with the Larmor gyration time and radius. Hence, these stationary configurations are actually stable against axisymmetric kinetic instabilities of this type. As a fundamental consequence, this rules out the possibility of having the axisymmetric magneto-rotational or thermal instabilities to arise in these systems.

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Cited by in corpus (9)

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• Synchronous Lagrangian variational principles in General Relativity
• Theory of spatially non-symmetric kinetic equilibria for collisionless plasmas
• Collisionless kinetic regimes for quasi-stationary axisymmetric accretion disc plasmas
• Kinetic equilibria of relativistic collisionless plasmas in the presence of non-stationary electromagnetic fields
• Covariant formulation of spatially non-symmetric kinetic equilibria in magnetized astrophysical plasmas
• Inconsistency in the Standard Model for Thin Accretion Disks
• Carter-constant induced mechanism for generation of anisotropic kinetic equilibria in collisionless N-body systems
• Dynamics of charged particles and quasi-periodic oscillations in the vicinity of a distorted, deformed compact object embedded in a uniform magnetic field