3D simulations of Rayleigh-Taylor instability using ``VULCAN/3D

DOI10.1007/S10509-005-3970-9zbMath1132.76300OpenAlexW4253237173MaRDI QIDQ815908

Lior Metzker, E. Livne, Shimon M. Asida, Josef Stein

Publication date: 31 March 2006

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-005-3970-9

zbMATH Keywords

instabilitysimulationhydrodynamics

Mathematics Subject Classification ID

Software, source code, etc. for problems pertaining to fluid mechanics (76-04)

Related Items (1)

Rayleigh-Taylor and Richtmyer-Meshkov instability induced flow, turbulence, and mixing. II

Cites Work

• Density ratio dependence of Rayleigh–Taylor mixing for sustained and impulsive acceleration histories
• Vorticity production and turbulent cooling of “hot channels” in gases: Three dimensions versus two dimensions

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