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Effect of inflation on anisotropic cosmologies

descriptionPublicationkeyboard_double_arrow_right Article 15 Aug 1986 English Publisher:American Physical Society (APS)Journal:Physical Review D, volume 34, pages 931-933 (issn: 0556-2821, Copyright policy )
Authors: , Jensen; , Stein-Schabes;

doi: 10.1103/physrevd.34.931

pmid: 9957231

Effect of inflation on anisotropic cosmologies

Abstract

We study the effects of anisotropic cosmologies on inflation. By properly formulating the field equations it is possible to show that any model that undergoes sufficient inflation will become isotropic on scales greater than the horizon today. Furthermore, we shall show that it takes a very long time for anisotropies to become visible in the observable part of the Universe. It is interesting to note that the time scale will be independent of the Bianchi model and of the initial anisotropy.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
70
Top 10%
Top 10%
Top 10%