A bulk inflaton from large volume extra dimensions
Brian Greene, Daniel Kabat, Janna Levin, and Dylan Thurston

TL;DR
This paper explores how large volume extra dimensions can naturally produce a weakly coupled inflaton field, enabling viable inflationary models and offering insights into dark matter and brane-less scenarios.
Contribution
It demonstrates that bulk scalar fields in large volume extra dimensions can generate suitable inflation potentials with minimal tuning, expanding the understanding of extra-dimensional cosmology.
Findings
Bulk scalar fields produce weakly coupled inflaton potentials.
Models achieve inflation with tunings at the per mil level.
Potential implications for dark matter and brane-less models.
Abstract
The universe may have extra spatial dimensions with large volume that we cannot perceive because the energy required to excite modes in the extra directions is too high. Many examples are known of such manifolds with a large volume and a large mass gap. These compactifications can help explain the weakness of four-dimensional gravity and, as we show here, they also have the capacity to produce reasonable potentials for an inflaton field. Modeling the inflaton as a bulk scalar field, it becomes very weakly coupled in four dimensions, and this enables us to build phenomenologically acceptable inflationary models with tunings at the few per mil level. We speculate on dark matter candidates and the possibility of braneless models in this setting.
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