F-theory Axiverse

Fuente: arXiv
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Autori principali: Fallon, Sebastian Vander Ploeg, Halverson, James, McAllister, Liam, Zhu, Yunhao
Natura: Preprint
Pubblicazione: 2025
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author Fallon, Sebastian Vander Ploeg
Halverson, James
McAllister, Liam
Zhu, Yunhao
author_facet Fallon, Sebastian Vander Ploeg
Halverson, James
McAllister, Liam
Zhu, Yunhao
contents We compute the couplings of Ramond-Ramond four-form axions in three ensembles of F-theory compactifications, with up to 181,200 axions. We work in the stretched Kähler cone, where $α'$ corrections are plausibly controlled, and we use couplings to certain non-Abelian sectors as a proxy for couplings to photons. The axion masses, decay constants, and couplings to gauge sectors show striking universality across the ensembles. In particular, the axion-photon couplings grow with $h^{1,1}$, and models in our ensemble with $h^{1,1} \gtrsim$ 10,000 axions are in tension with helioscope constraints. Moreover, under mild assumptions about charged matter beyond the Standard Model, theories with $h^{1,1} \gtrsim$ 5,000 are in tension with Chandra measurements of X-ray spectra. This work is a first step toward understanding the phenomenology of quantum gravity theories with thousands of axions.
format Preprint
id arxiv_https___arxiv_org_abs_2511_20458
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle F-theory Axiverse
Fallon, Sebastian Vander Ploeg
Halverson, James
McAllister, Liam
Zhu, Yunhao
High Energy Physics - Theory
We compute the couplings of Ramond-Ramond four-form axions in three ensembles of F-theory compactifications, with up to 181,200 axions. We work in the stretched Kähler cone, where $α'$ corrections are plausibly controlled, and we use couplings to certain non-Abelian sectors as a proxy for couplings to photons. The axion masses, decay constants, and couplings to gauge sectors show striking universality across the ensembles. In particular, the axion-photon couplings grow with $h^{1,1}$, and models in our ensemble with $h^{1,1} \gtrsim$ 10,000 axions are in tension with helioscope constraints. Moreover, under mild assumptions about charged matter beyond the Standard Model, theories with $h^{1,1} \gtrsim$ 5,000 are in tension with Chandra measurements of X-ray spectra. This work is a first step toward understanding the phenomenology of quantum gravity theories with thousands of axions.
title F-theory Axiverse
topic High Energy Physics - Theory
url https://arxiv.org/abs/2511.20458