Gravitational instability in a multicomponent cosmological medium

Details Gravitational instability in a multicomponent cosmological medium Gravitational instability in a multicomponent cosmological medium

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jmp....29.2069m&link_type=abstract

Journal of Mathematical Physics (ISSN 0022-2488), vol. 29, Sept. 1988, p. 2069-2077.

Statistics

Computation

4

Astronomical Models, Computational Astrophysics, Cosmology, Gravitational Effects, Asymptotic Methods, Differential Equations, Perturbation Theory, Stability

Scientific paper

A systematic approach to exact solutions for the evolution of small density inhomogeneities of a two-component and in special cases for a three-component cosmological medium is presented. In general, there exists just one increasing perturbation mode. Expressing the solutions of the respective differential equations in terms of Meijer's G function (1946), various exact and asymptotic formulas for the perturbation modes are derived.

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