Axions in the dark dimension

A bstract The dark dimension scenario, which is motivated from Swampland principles and predicts a single micron scale extra dimension, suggests a consistent framework for the dark sector of the universe. We consider the implications of this scenario for the QCD axion. We find that in the scenario in which the axion is localized on the standard model brane (which we will argue is natural), a combination of theoretical (being bounded by the 5D Planck mass) and observational constraints forces it to have decay constant in a narrow range f ~ 10 9 – 10 10 GeV. This corresponds to a mass for the QCD axion of m a ~ (1 – 10) meV. The axion mass surprisingly coincides with the mass scale for the dark energy, the dark matter tower, and the neutrinos. In this scenario axions are not expected to form a large fraction of the dark matter but nevertheless this range of axion parameters is accessible to observations in near future experiments.

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Publication Details

Journal
Journal of High Energy Physics
Published
2024-12-17
DOI
https://doi.org/10.1007/jhep12(2024)127
Citations
8
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
5.28

Funders

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article

Axions in the dark dimension

Naomi Gendler, Cumrun Vafa
8 citations
Journal of High Energy Physics
Dark Matter and Cosmic Phenomena
5.28
article

Axions in the dark dimension

Naomi Gendler, Cumrun Vafa
article en
8 citations

Abstract

A bstract The dark dimension scenario, which is motivated from Swampland principles and predicts a single micron scale extra dimension, suggests a consistent framework for the dark sector of the universe. We consider the implications of this scenario for the QCD axion. We find that in the scenario in which the axion is localized on the standard model brane (which we will argue is natural), a combination of theoretical (being bounded by the 5D Planck mass) and observational constraints forces it to have decay constant in a narrow range f ~ 10 9 – 10 10 GeV. This corresponds to a mass for the QCD axion of m a ~ (1 – 10) meV. The axion mass surprisingly coincides with the mass scale for the dark energy, the dark matter tower, and the neutrinos. In this scenario axions are not expected to form a large fraction of the dark matter but nevertheless this range of axion parameters is accessible to observations in near future experiments.

Journal of High Energy PhysicsVol. 2024(12)
Harvard University Press (US)
National Science Foundation
Openalex Percentile: Top 3%
Dark Matter and Cosmic Phenomena
5.28
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