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Topology and the cosmic microwave background

Levin, Janna·2002·Physics Reports
DOI 10.1016/s0370-1573(02)00018-2
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  • In the open universe case, the effective energy associated with curvature decreases as a^-2, becomes dominant soon after expansion, making the relative role of normal matter and its density perturbations insignificant; this is an additional reason density perturbations in a compact hyperbolic universe will rapidly decrease.

    “Moreover, the effective energy associated with the curvature of 3D space in the open universe case decreases as a -2 , i.e. much more slowly than the energy of ordinary matter.Soon after the beginning of expansion, the curvature energy density becomes dominant, and the relative role of normal matter and of its density perturbations become insignificant.This is an additional reason to expect that”

    From Creation of a compact topologically nontrivial inflationary universe (2004) · cites this paper as [22]

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Metadata

Authors
Levin, J.
Venue
Physics Reports
Publisher
Elsevier BV
Published
2002-08
Volume
365
Issue
4
Pages
251-333
ISSN
0370-1573
DOI
10.1016/s0370-1573(02)00018-2
Cited by
149
References
5
Language
en
Licence
www.elsevier.com/tdm/userlicense/1.0/ (tdm)

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