Non-Linear Dynamics of the Richtmyer Meshkov Instability in Supernovae

Details Non-Linear Dynamics of the Richtmyer Meshkov Instability in Supernovae Non-Linear Dynamics of the Richtmyer Meshkov Instability in Supernovae

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.298..379a&link_type=abstract

Astrophysics and Space Science, Volume 298, Issue 1-2, pp. 379-383

Astronomy and Astrophysics

Astrophysics

Richtmyer–Meshkov, Supernovae, Singularities, Non-Local, Richtmyer&Ndash, Meshkov

Scientific paper

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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