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Inertial phase separation in rotating self-gravitating media

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Publication:2269407
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DOI10.1007/S10697-004-0008-XzbMath1184.76883OpenAlexW1965038192MaRDI QIDQ2269407

Yanyan Li

Publication date: 16 March 2010

Published in: Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10697-004-0008-x


zbMATH Keywords

particlesswirling flowsfull Lagrangian approachcentrifugal separationdensity anisotropy


Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Dusty-gas two-phase flows (76T15)


Related Items (1)

Comparison of the Eulerian and Lagrangian approaches to studying the peculiarities of the interstellar dust distribution in the heliosphere in the framework of the cold gas model




Cites Work

  • Investigation of regions of unbounded growth of the particle concentration in disperse flows
  • Equation of motion for a small rigid sphere in a nonuniform flow
  • The force on a bubble, drop, or particle in arbitrary time-dependent motion at small Reynolds number
  • Lagrangian modelling of dust admixture in gas flows




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