Part textbook, part exploratory work, this book aims to raise
the awareness of students, physicists, and engineers in turbulence
on the modeling of gravitationally induced turbulent mixing flows
as produced, for instance, by Rayleigh-Taylor instabilities. The
discussion is centered on the differences between single-fluid and
two-fluid approaches, and it is illustrated with a 0D analysis of
two specific elementary models in common use. Important deviations
are shown to appear on many features, among others the prominence
of directed energy, the simultaneous restitution of test cases, the
responses to variable acceleration and shocks, and the behavior of
various length scales.
General
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