Anisotropy in the chaotic inflationary universe

Details Anisotropy in the chaotic inflationary universe Anisotropy in the chaotic inflationary universe

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phlb..178..159m&link_type=abstract

Physics Letters B, Volume 178, Issue 2-3, p. 159-162.

Physics

64

Scientific paper

The effect of anisotropies on the chaotic inflationary model is investigated for a general class of Bianchi cosmologies. It is shown that for suitable initial conditions of a scalar field any initial anisotropy always disappers before the onset of inflation. Using numerical calculations it is also shown for Bianchi I models that the class initial conditions of the scalar field which leads to inflation is very large.

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