English

Automatic Enhancement in 6D Supergravity and F-theory Models

High Energy Physics - Theory 2021-07-28 v1

Abstract

We observe that in many F-theory models, tuning a specific gauge group GG and matter content MM under certain circumstances leads to an automatic enhancement to a larger gauge group GGG' \supset G and matter content MMM' \supset M. We propose that this is true for any theory G,MG, M whenever there exists a containing theory G,MG', M' that cannot be Higgsed down to G,MG, M. We give a number of examples including non-Higgsable gauge factors, nonabelian gauge factors, abelian gauge factors, and exotic matter. In each of these cases, tuning an F-theory model with the desired features produces either an enhancement or an inconsistency, often when the associated anomaly coefficient becomes too large. This principle applies to a variety of models in the apparent 6D supergravity swampland, including some of the simplest cases with U(1) and SU(N) gauge groups and generic matter, as well as infinite families of U(1) models with higher charges presented in the prior literature, potentially ruling out all these apparent swampland theories.

Keywords

Cite

@article{arxiv.2012.01437,
  title  = {Automatic Enhancement in 6D Supergravity and F-theory Models},
  author = {Nikhil Raghuram and Washington Taylor and Andrew P. Turner},
  journal= {arXiv preprint arXiv:2012.01437},
  year   = {2021}
}

Comments

56 pages, LaTeX

R2 v1 2026-06-23T20:40:58.125Z