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

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

1994-02-08

arxiv.org/abs/astro-ph/9402019v1

Astrophys.Space Sci. 214 (1994) 139-149

Astronomy and Astrophysics

Astrophysics

20 pages in LaTeX, McGill University preprint

Scientific paper

10.1007/BF00982331

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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