arXiv · math/9307214
Computational aspects of the gravitational instability problem for a multicomponent cosmological medium
Abstract
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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Hans J. Haubold, Arak Mathai Mathai. 1993-07-09. Computational aspects of the gravitational instability problem for a multicomponent cosmological medium. https://arxiv.org/abs/math/9307214
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