Relativistic theory of spherically symmetric perturbation in dust universe.

Details Relativistic theory of spherically symmetric perturbation in dust universe. Relativistic theory of spherically symmetric perturbation in dust universe.

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jmp....31.2462l&link_type=abstract

Journal of Mathematical Physics, Vol. 31, No. 10, p. 2462 - 2465

Mathematics

Logic

3

Cosmological Models: Relativity Theory

Scientific paper

Starting from the initial value formulation of dust solution given in paper 161.308 a relativistic perturbation equation and its general solutions in spherically symmetric universes are derived. It is found that these solutions are in analogy with the Bonnor-Weinberg results of the Newtonian theory and contain three modes: a growing mode, a decaying mode, and a constant mode.

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