Note on magneto-hydrodynamic gravitational stability of a double fluids interface
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The Self
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The magneto–gravitational stability of double-fluid interface is discussed. The pressure in the unperturbed state is not constant because the self-gravitating force is a long-range force. The dispersion relation is derived and discussed. The self-gravitating model is unstable in the symmetric mode m = 0 (m is the transverse wave number), while it is stable in all other states. The effects of the densities, the liquid-fluid radii ratios, and the electromagnetic force on the stability of the present model are identified for all wavelengths.PACS Nos.: 47.35.Tv, 47.65.–d, 04.40.–b
STUDY ON ELECTROHYDRODYNAMIC CAPILLARY INSTABILITY OF VISCOELASTIC FLUIDS WITH RADIAL ELECTRIC FIELD
2014 ◽
Vol 06
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pp. 1450037
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2014 ◽
Vol 23
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pp. 1450013
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1990 ◽
Vol 18
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pp. 267-277
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1966 ◽
Vol 21
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pp. 1953-1959
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1998 ◽
Vol 4
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pp. 73-90
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