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Computational aspects of the gravitational instability problem for a multicomponent cosmological medium

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arxiv math/9307214 v1 pith:HBPQFIML submitted 1993-07-09 math.CA astro-ph

classification math.CAastro-ph
keywords cosmologicalmulticomponentanalyticaspectsclosed-formcomputablecomputationalderive
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The paper presents results for deriving closed-form analytic solutions of 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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