Magnetogravitational stability of self-gravitating plasma with thermal conduction and finite Larmor radius through porous medium

DOI10.1007/BF01094937zbMath0645.76059OpenAlexW2010246135MaRDI QIDQ1103471

D. S. Vaghela, R. K. Chhajlani

Publication date: 1987

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

Full work available at URL: https://doi.org/10.1007/bf01094937

zbMATH Keywords

instabilityStabilitylinearized equationsfinite ion-Larmor radiusfragmentation of interstellar matterJeans's instability conditionself- gravitating plasma

Mathematics Subject Classification ID

Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (4)

Gravitational stability of finitely conducting two-component plasma through porous medium ⋮ Stability of thermally conducting plasma in a variable magnetic field ⋮ Self-gravitational instability of rotating viscous Hall plasma with arbitrary radiative heat-loss functions and electron inertia ⋮ Gravitational instability of a homogeneous gas cloud with radiation

Cites Work

• The gravitational instability of flow through porous medium for some systems of astrophysical interest
• Instability of rotating isotropic and anisotropic plasmas
• Larmor radius effects on the instability of a rotating layer of a self- gravitating plasma
• Magnetohydrodynamic Equations for Finite Larmor Radius
• Use of the Logistic Model in Retrospective Studies

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