Abstract
The Rayleigh-Taylor instability (RTI) of a continuously stratified fluid has implica- tions on the stability of solar and planetary interiors. A nonlinear stage of the two-dimensional RTI is studied by including various effects. By using the multiple scale method, we derived a non- linear Schrodinger equation (NLSE) in 2+1 dimensions. We show the general soliton solutions of the NLSE and this allows to discuss their stability.
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