Hydromagnetic stability of a slim disc in a stationary geometry

@article{ArayaGchez2002HydromagneticSO,
  title={Hydromagnetic stability of a slim disc in a stationary geometry},
  author={Rafael Angel Araya-G{\'o}chez},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2002},
  volume={337},
  pages={795-807}
}
  • R. Araya-Góchez
  • Published 29 March 2002
  • Physics
  • Monthly Notices of the Royal Astronomical Society
The magnetorotational instability originates from the elastic coupling of fluid elements in orbit around a gravitational well. Since inertial accelerations play a fundamental dynamical role in the process, one may expect substantial modifications by strong gravity in the case of accretion on to a black hole. In this paper, we develop a fully covariant, Lagrangian displacement vector field formalism with the aim of addressing these issues for a disc embedded in a stationary geometry with… Expand

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