Stability of homogeneous universes

Details Stability of homogeneous universes Stability of homogeneous universes

Dec 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972cmaph..26..259b&link_type=abstract

Communications in Mathematical Physics, Volume 26, Issue 4, pp.259-270

Mathematics

Mathematical Physics

5

Scientific paper

The stability of a class of homogeneous cosmological models is
investigated. It is shown that the perturbation problem for six such
universes can be reduced to a system of ordinary differential equations.
The time development of the perturbations is such that they remain
finite at all times for which the unperturbed metric is non-singular.

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