Abstract
This chapter begins with a discussion of buoyancy as a driving force and proceeds to derive the dispersion relation for the Rayleigh-Taylor instability. It considers Rayleigh-Taylor in several specific contexts, the generalization of Rayleigh Taylor, sometimes called the entropy mode , and the nonlinear behavior of Rayleigh-Taylor-unstable systems. It hen discusses lift as a driving force, proceeds to derive the dispersion relation for the Kelvin-Helmholtz instability, and discusses Kelvin-Helmholtz in several specific contexts. Following that, it discusses the stability of shock waves and then the Richtmyer-Meshkov process, through which deposition of vorticity leads to evolving structure. The chapter concludes with a discussion of hydrodynamic turbulence.
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Drake, R.P. (2018). Hydrodynamic Instabilities. In: High-Energy-Density Physics. Graduate Texts in Physics. Springer, Cham. https://doi.org/10.1007/978-3-319-67711-8_5
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DOI: https://doi.org/10.1007/978-3-319-67711-8_5
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