Abstract
We report analytical and numerical solutions describing the evolution of the coherent structure of bubbles and spikes in the Richtmyer-Meshkov instability in supernovae. It is shown that the dynamics of the flow is essentially non-local, and the nonlinear Richtmyer-Meshkov bubble flattens and decelerates.
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Abarzhi, S.I., Herrmann, M. (2005). Non-Linear Dynamics of the Richtmyer-Meshkov Instability in Supernovae. In: Kyrala, G. (eds) High Energy Density Laboratory Astrophysics. Springer, Dordrecht. https://doi.org/10.1007/1-4020-4162-4_57
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DOI: https://doi.org/10.1007/1-4020-4162-4_57
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Publisher Name: Springer, Dordrecht
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Online ISBN: 978-1-4020-4162-4
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