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Momentum transport from current-driven reconnection in astrophysical disks

Current-driven reconnection is investigated as a possible mechanism for angular momentum transport in astrophysical disks. A theoretical and computational study of angular momentum transport from current-driven magnetohydrodynamic instabilities is performed. It is found that both a single resistive tearing instability and an ideal instability can transport momentum in the presence of azimuthal Keplerian flow. The structure of the Maxwell stress is examined for a single mode through analytic quasilinear theory and computation. Full nonlinear multiple mode computation shows that a global Maxwell stress causes significant momentum transport.

preprint2011arXivOpen access
F. EbrahimiS. C. Prager
physics.plasm-phastro-ph.HE
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F. EbrahimiS. C. Prager

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