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Main Authors: Marchesano, Fernando, Prieto, David, Wiesner, Max
Format: Preprint
Published: 2021
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Online Access:https://arxiv.org/abs/2105.09326
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author Marchesano, Fernando
Prieto, David
Wiesner, Max
author_facet Marchesano, Fernando
Prieto, David
Wiesner, Max
contents We compute the flux-induced F-term potential in 4d F-theory compactifications at large complex structure. In this regime, each complex structure field splits as an axionic field plus its saxionic partner, and the classical F-term potential takes the form $V = Z^{AB} ρ_Aρ_B$ up to exponentially-suppressed terms, with $ρ$ depending on the fluxes and axions and $Z$ on the saxions. We provide explicit, general expressions for $Z$ and $ρ$, and from there analyse the set of flux vacua, for an arbitrary number of fields. We identify two families of vacua with all complex structure fields fixed and a flux contribution to the tadpole $N_{\rm flux}$ which is bounded. In the first and most generic one, the saxion vevs are bounded from above by a power of $N_{\rm flux}$. In the second their vevs may be unbounded and $N_{\rm flux}$ is a product of two arbitrary integers, unlike what is claimed by the Tadpole Conjecture. We specialise to type IIB orientifolds, where both families of vacua are present, and link our analysis with several results in the literature. We finally illustrate our findings with several examples.
format Preprint
id arxiv_https___arxiv_org_abs_2105_09326
institution arXiv
publishDate 2021
record_format arxiv
spellingShingle F-theory flux vacua at large complex structure
Marchesano, Fernando
Prieto, David
Wiesner, Max
High Energy Physics - Theory
We compute the flux-induced F-term potential in 4d F-theory compactifications at large complex structure. In this regime, each complex structure field splits as an axionic field plus its saxionic partner, and the classical F-term potential takes the form $V = Z^{AB} ρ_Aρ_B$ up to exponentially-suppressed terms, with $ρ$ depending on the fluxes and axions and $Z$ on the saxions. We provide explicit, general expressions for $Z$ and $ρ$, and from there analyse the set of flux vacua, for an arbitrary number of fields. We identify two families of vacua with all complex structure fields fixed and a flux contribution to the tadpole $N_{\rm flux}$ which is bounded. In the first and most generic one, the saxion vevs are bounded from above by a power of $N_{\rm flux}$. In the second their vevs may be unbounded and $N_{\rm flux}$ is a product of two arbitrary integers, unlike what is claimed by the Tadpole Conjecture. We specialise to type IIB orientifolds, where both families of vacua are present, and link our analysis with several results in the literature. We finally illustrate our findings with several examples.
title F-theory flux vacua at large complex structure
topic High Energy Physics - Theory
url https://arxiv.org/abs/2105.09326