An existence theorem for perturbed Newtonian cosmological models.

Details An existence theorem for perturbed Newtonian cosmological models. An existence theorem for perturbed Newtonian cosmological models.

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jmp....33.1224b&link_type=abstract

Journal of Mathematical Physics, Vol. 33, No. 3, p. 1224 - 1233

Mathematics

Mathematical Physics

6

Scientific paper

Given a Newtonian Friedmann-like cosmological model M0, there
exist, locally in time, spatially periodic solutions close to
M0. Such solutions represent inhomogeneous models that are
homogenous and isotropic on a large scale. The Euler-Poisson system is
shown to be linearization stable at M0.

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