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arxiv: hep-th/9402085 · v1 · pith:PLUBJXLInew · submitted 1994-02-15 · ✦ hep-th · gr-qc

Topological Inflation

classification ✦ hep-th gr-qc
keywords inflationtopologicalconditionscoresdefectsfieldfine-tuningforced
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Inflation can occur in the cores of topological defects, where the scalar field is forced to stay near the maximum of its potential. This topological inflation does not require fine-tuning of the initial conditions.

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    astro-ph.CO 2026-05 unverdicted novelty 5.0

    A Hubble-scale domain wall quintessence model produces anisotropic expansion but is tightly constrained by Planck CMB quadrupole limits and supernova data to a negligible contribution, favoring standard LambdaCDM.