Computational aspects of the gravitational instability problem for a multicomponent cosmological medium
arXiv:astro-ph/9402019 · doi:10.1007/BF00982331
Abstract
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.
20 pages in LaTeX, McGill University preprint