Asymptotic behavior of a stratified perturbation in a three dimensional expanding Universe
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🌌 astro-ph
cond-mat
keywords
asymptoticmodeldimensionalexpandingnumericalperturbationstratifiedthree
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The non-linear evolution of a stratified perturbation in a three dimensional expanding Universe is considered. A general Lagrangian scheme (Q model) is introduced and numerical investigations are performed. The asymptotic contraction of the core of the agglomeration is studied. A power-law scaling is detected and an heuristic interpretation of the numerical findings is provided. An asymptotic equation for the multi-stream velocity flow is derived and it is shown to agree quantitatively with the dynamics of the Q model. The relation to the adhesion model is discussed.
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