Gravitational instability - The quasi-linear approximation

Details Gravitational instability - The quasi-linear approximation Gravitational instability - The quasi-linear approximation

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64...26r&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Jan.-Feb. 1987, p. 26-30. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Gravitational Fields, Perturbation Theory, Cosmic Dust, Energy Distribution, Nonlinear Equations, Tetrad Theory, Universe

Scientific paper

Consideration is given to the second approximation of the problem of the evolution of small gravitational perturbations in Friedmann's standard model of the universe filled with dust. The tetrad representation of the field equations is used. It is shown that the interaction of perturbations can accelerate the evolution of perturbations and can lead to the redistribution of energy between gravitational perturbations of different spatial scales.

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