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arxiv: hep-th/0408164 · v2 · submitted 2004-08-23 · ✦ hep-th · astro-ph· gr-qc· hep-ph

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Creation of a Compact Topologically Nontrivial Inflationary Universe

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classification ✦ hep-th astro-phgr-qchep-ph
keywords inflationarycompactcreationnontrivialopenuniversedensityflat
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If inflation can occur only at the energy density V much smaller than the Planck density, which is the case for many inflationary models based on string theory, then the probability of quantum creation of a closed or an infinitely large open inflationary universe is exponentially suppressed for all known choices of the wave function of the universe. Meanwhile under certain conditions there is no exponential suppression for creation of topologically nontrivial compact flat or open inflationary universes. This suggests, contrary to the standard textbook lore, that compact flat or open universes with nontrivial topology should be considered a rule rather than an exception.

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  1. Inflation and topology from the no-boundary state

    hep-th 2026-05 unverdicted novelty 7.0

    The no-boundary wavefunction on the 3-torus, summed over SL(3,Z) geometries using GL(3) automorphic forms, favors large inflating universes with N ≳ 250 e-folds and induces torus-moduli corrections to the CMB spectrum.