Abstract
Turbulence generated by hydrodynamic instabilities is important in high-energydensity physics [1]. Examples in astrophysics include turbulent mixing processes during stellar core-collapse, where shock waves accelerate multiple perturbed gas interfaces.
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Morán-López, J.T., Schilling, O., Holloway, J.P. (2015). Reynolds-Averaged Navier–Stokes Modeling of Reshocked Richtmyer–Meshkov Instability Experiments and Simulations. In: Bonazza, R., Ranjan, D. (eds) 29th International Symposium on Shock Waves 2. ISSW 2013. Springer, Cham. https://doi.org/10.1007/978-3-319-16838-8_40
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DOI: https://doi.org/10.1007/978-3-319-16838-8_40
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