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- W1983993825 abstract "Abstract The instability of a rotating viscous hollow liquid cylinder endowed with surface tension is studied. The stability criterion is derived as valid for all possible modes of perturbations and the instability characteristics of that model are identified. The angular velocity of rotation plays an important role (but viscosity does not) in the stability restrictions. The model is just unstable for certain values of the perturbed wavelength and syable for all other values. The capillary non-rotating instability of the model is examined. The capillary force influence is the same as the viscous rotating state, as long as the inertia is dominant over the viscosity. As the viscosity is paramount over the inertia force, we have the same situation as the case in which the inertia is greater than the viscosity but, there is no finite maximum mode of instability. The model will not have a tendency to break-up at points separated by distances comparable to the circumference of the gas jet, but just to give way at a few distant places. Moreover, for any value of the growth rate of the instability, the viscosity has the effect of increasing the wavelength, in comparison with the corresponding value as the inertia force is predominant over the viscosity." @default.
- W1983993825 created "2016-06-24" @default.
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- W1983993825 date "1991-07-01" @default.
- W1983993825 modified "2023-10-18" @default.
- W1983993825 title "Capillary instability of a rotating viscous hollow jet" @default.
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- W1983993825 doi "https://doi.org/10.1016/0304-8853(91)90441-c" @default.
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