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arxiv: hep-th/9503097 · v3 · submitted 1995-03-15 · ✦ hep-th · astro-ph· gr-qc· hep-ph

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INFLATION WITH VARIABLE OMEGA

Andrei Linde
Authors on Pith no claims yet
classification ✦ hep-th astro-phgr-qchep-ph
keywords inflationomegachaoticdivisioninfinitelyleadsmanyopen
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We propose a simple version of chaotic inflation scenario which leads to a division of the universe into infinitely many open universes with all possible values of $\Omega$ from 1 to 0.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Geodesically Complete Curvature-Bounce Inflation

    astro-ph.CO 2026-04 unverdicted novelty 5.0

    A closed k=+1 FRW universe with curvature-driven bounce and canonical scalar inflation remains sub-Planckian, satisfies the null energy condition, and produces ns=0.9617-0.9650 and r=0.0037-0.0045 consistent with data.