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Topological Inflation
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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.
Forward citations
Cited by 4 Pith papers
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A Dynamical Solution to the Axion Domain Wall Problem
Adding a spectator PQ field with a large early-universe value and a high-dimensional S^mP mixing term can solve the axion domain wall problem and suppress isocurvature, allowing non-trivial domain wall numbers with HI...
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Eternal Inflation in Swampy Landscapes
Eternal inflation persists in landscapes where de Sitter vacua are rare or absent, via flyover transitions between isolated dS vacua or inflating bubble walls nucleated around saddle points.
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Domain-wall Quintessence
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.
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Cross-Modal Prototype Augmentation and Dual-Grained Prompt Learning for Social Media Popularity Prediction
The abstract claims SOTA multimodal popularity prediction, but the attached full text is a different paper on inflationary reheating, so the claimed result is unverifiable as submitted.
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