Computational aspects of the gravitational instability problem for a multicomponent cosmological medium
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🌌 astro-ph
keywords
cosmologicalmulticomponentanalyticaspectsclosed-formcomputablecomputationalderive
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The paper presents results for deriving closed-form analytic solutions of the non-relativistic linear perturbation equations, which govern the evolution of inhomogeneities in a homogeneous spatially flat multicomponent cosmological model. Mathematical methods to derive computable forms of the perturbations are outlined.
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