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INFLATION WITH VARIABLE OMEGA

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arxiv hep-th/9503097 v3 pith:VH5MTLUN submitted 1995-03-15 hep-th astro-phgr-qchep-ph

classification hep-thastro-phgr-qchep-ph
keywords inflationomegachaoticdivisioninfinitelyleadsmanyopen
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abstract

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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Forward citations

Cited by 2 Pith papers

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

  1. Tunnelling out of Starobinsky inflation: Raising the spectral tilt

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    A first-order phase-transition exit from a displaced Starobinsky branch truncates ~12 e-folds, shifting the spectral tilt from n_s≈0.965 to ≈0.973 at r≈2×10⁻³.

  2. Affine ANEC selects the closed FRW branch for geodesically complete cosmology

    gr-qc 2026-05 unverdicted novelty 6.0 of 10

    Affine ANEC obstructs non-static flat and open FRW from being null geodesically complete while ANEC-satisfying, but allows explicit scalar-field realizations for closed FRW with NEC-respecting matter.

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