Current-driven instabilities in weakly ionized disks
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Publication:3541280
DOI10.1002/ASNA.200811007zbMATH Open1255.85027arXiv0806.3855OpenAlexW3097990787MaRDI QIDQ3541280
Author name not available (Why is that?)
Publication date: 25 November 2008
Published in: (Search for Journal in Brave)
Abstract: Cool weakly ionized gaseous rotating disk form the basis for many models in astrophysics objects. Instabilities against perturbations in such disks play an important role in the theory of the formation of stars and planets. Traditionally, axisymmetric magnetohydrodynamic (MHD) and recently Hall-MHD instabilities have been thoroughly studied as providers of an efficient mechanism for radial transfer of angular momentum, and of density radial stratification. In the current work, the Hall instability against axisymmetric perturbations in incompressible rotating fluid in external poloidal and toroidal magnetic field is considered.
Full work available at URL: https://arxiv.org/abs/0806.3855
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