Self-gravitational instability of rotating viscous Hall plasma with arbitrary radiative heat-loss functions and electron inertia

DOI10.1007/S10509-010-0273-6zbMath1187.85027OpenAlexW2077417396MaRDI QIDQ973713

R. K. Pensia, R. P. Prajapati, S. Kaothekar, R. K. Chhajlani

Publication date: 26 May 2010

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-010-0273-6

zbMATH Keywords

rotationviscositymagnetohydrodynamics (MHD)Jeans instabilityHall parameterthermally conductingheat-loss functions

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (2)

Self-gravitational instability in magnetized finitely conducting viscoelastic fluid ⋮ Effect of rotation and FLR corrections with radiative heat-loss functions on transverse thermal instability of astrophysical porous plasma in interstellar medium (ISM)

Cites Work

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• Jeans' gravitational instability of a thermally conducting plasma
• The gravitational instability of flow through porous medium for some systems of astrophysical interest
• Magnetogravitational stability of self-gravitating plasma with thermal conduction and finite Larmor radius through porous medium
• Magnetogravitational instability of an infinite homogeneous rotating plasma through a porous medium with finite electrical and thermal conductivities
• Stability of thermally conducting plasma in a variable magnetic field
• Jeans instability in a plasma with positive–negative charged and neutral dust components

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