Contribution to the angular momentum transport paradigm for accretion disks

DOI10.1016/j.physletb.2021.136769zbMath1483.85009arXiv2009.07215OpenAlexW3212378608MaRDI QIDQ824197

Giovanni Montani, Nakia Carlevaro

Publication date: 14 December 2021

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2009.07215

zbMATH Keywords

magneto-hydrodynamicsplasma astrophysicsaccretion and accretion disks

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Statistical mechanics of plasmas (82D10) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• Revised conditions for MRI due to isorotation theorem
• THE STABILITY OF NON-DISSIPATIVE COUETTE FLOW IN HYDROMAGNETICS
• Theory of Magnetically Powered Jets
• The Non-uniform Rotation of the Sun and its Magnetic Field

This page was built for publication: Contribution to the angular momentum transport paradigm for accretion disks