The gravitational instability of flow through porous medium for some systems of astrophysical interest

DOI10.1007/BF00676140zbMath0544.76048MaRDI QIDQ797405

R. C. Sharma, K. P. Thakur

Publication date: 1982

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

zbMATH Keywords

gravitational instabilityeffects of rotation, magnetic field, viscosity and finite electrical conductivityJeans's criterion

Mathematics Subject Classification ID

Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (5)

Magneto-gravitational instability of a rotating and finitely-conducting fluid ⋮ Gravitational stability of finitely conducting two-component plasma through porous medium ⋮ 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 ⋮ Self-gravitational instability of rotating viscous Hall plasma with arbitrary radiative heat-loss functions and electron inertia

Cites Work

• Rayleigh instability of a thermal boundary layer in flow through a porous medium
• Some effects of suspended particles on the onset of Bénard convection
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