Shear in a perturbed Friedmann universe

Details Shear in a perturbed Friedmann universe Shear in a perturbed Friedmann universe

Jun 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970gregr...1..103s&link_type=abstract

General Relativity and Gravitation, Volume 1, Issue 2, pp.103-115

Physics

2

Scientific paper

For perturbed Friedmann models of vanishing and positive curvature the
time development of shear is computed by means of a linear perturbation
theory. As for the smallness of the perturbation functions
mathematically exact and physically meaningful conditions are stated.
The shear is computed for different stages of the universe.

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