Sign-flipping axion potentials via Kapitza-type modulation by heavy axions

A bstract We show that the potential of a light axion can flip sign, or even nearly vanish, as a result of coherent oscillations of a heavier axion with which it mixes. This phenomenon is analogous to the Kapitza pendulum, where a high-frequency external force stabilizes an otherwise unstable configuration, but here it arises naturally from the inherent mass hierarchy and mixing among axions in the axiverse, without the need for any externally imposed modulation. We further show that a late-time sign flip of the potential can significantly enhance the abundance of the light axion, which has important cosmological and observational consequences. Such dynamics may also be realized in multi-natural inflation, or inside oscillons and boson stars formed by a heavy axion.

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Publication Details

Journal
Journal of High Energy Physics
Published
2026-07-17
DOI
https://doi.org/10.1007/jhep07(2026)171
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
0.00

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article

Sign-flipping axion potentials via Kapitza-type modulation by heavy axions

Kai Murai, Fuminobu Takahashi, Kosei Tomiyama
Journal of High Energy Physics
Dark Matter and Cosmic Phenomena
article

Sign-flipping axion potentials via Kapitza-type modulation by heavy axions

Kai Murai, Fuminobu Takahashi, Kosei Tomiyama
article en

Abstract

A bstract We show that the potential of a light axion can flip sign, or even nearly vanish, as a result of coherent oscillations of a heavier axion with which it mixes. This phenomenon is analogous to the Kapitza pendulum, where a high-frequency external force stabilizes an otherwise unstable configuration, but here it arises naturally from the inherent mass hierarchy and mixing among axions in the axiverse, without the need for any externally imposed modulation. We further show that a late-time sign flip of the potential can significantly enhance the abundance of the light axion, which has important cosmological and observational consequences. Such dynamics may also be realized in multi-natural inflation, or inside oscillons and boson stars formed by a heavy axion.

Journal of High Energy PhysicsVol. 2026(7)
Tohoku University (JP), The University of Tokyo (JP)
Japan Society for the Promotion of Science
Openalex Percentile: Top 98%
Dark Matter and Cosmic Phenomena
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