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A solution to the anisotropy problem in bouncing cosmologies · Around

2009

A solution to the anisotropy problem in bouncing cosmologies

Bozza, V., Bruni, M.

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Bouncing cosmologies are often proposed as alternatives to standard inflation for the explanation of the homogeneity and flatness of the universe.

In such scenarios, the present cosmological expansion is preceded by a contraction phase.
However, during the contraction, in general the anisotropy of the universe grows and eventually leads to a chaotic mixmaster behavior.
This would either be hard to reconcile with observations or even lead to a singularity instead of the bounce.

Built on

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Then

See e.g. the articles of Rendall and Nicolai in 100 Years of Relativity. Space-Time Structure: Einstein and Beyond
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Original
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