Effect of rotation and FLR corrections with radiative heat-loss functions on transverse thermal instability of astrophysical porous plasma in interstellar medium (ISM)

DOI10.1016/J.CJPH.2022.05.018MaRDI QIDQ6496430

Shankar Prasad Mishra, Suhas Phadke, Sachin Kaothekar

Publication date: 3 May 2024

Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)

zbMATH Keywords

rotationthermal instabilityflow through porous mediaFLR correctionradiative heat-loss functions

Mathematics Subject Classification ID

Fluid mechanics (76-XX) Hydrodynamic stability (76Exx) Astronomy and astrophysics (85Axx)

Cites Work

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• The gravitational instability of flow through porous medium for some systems of astrophysical interest
• Self-gravitational instability of rotating viscous Hall plasma with arbitrary radiative heat-loss functions and electron inertia
• Magnetogravitational instability of an infinite homogeneous rotating plasma through a porous medium with finite electrical and thermal conductivities
• Magnetohydrodynamic Equations for Finite Larmor Radius
• An application of Thomson s theorem to the determination of induced charge density

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