# A Chern-Simons Pandemic

**Authors:** Miguel Montero, Angel M. Uranga, Irene Valenzuela

arXiv: 1702.06147 · 2017-09-13

## TL;DR

This paper investigates the fate of global symmetries in quantum gravity, showing that Chern-Simons terms are essential for consistency and that their absence places theories in the Swampland.

## Contribution

It proposes that Chern-Simons terms involving antisymmetric tensor fields are necessary to break global symmetries in string theory, constraining the landscape of consistent quantum gravity theories.

## Key findings

- Global symmetries are obstructed in quantum gravity for certain dimensions.
- Chern-Simons terms can break global symmetries and evade black hole remnants.
- Many known theories are inconsistent without these Chern-Simons terms.

## Abstract

In this paper we study the consistency of generalized global symmetries in theories of quantum gravity, in particular string theory. Such global symmetries arise in theories with $(p+1)$-form gauge fields, and for spacetime dimension $d\leq p+3$ there are obstructions to their breaking even by quantum effects of charged objects. In 4d theories with a 2-form gauge field (or with an axion scalar), these fields endow Schwarzschild black holes with quantum hair, a global charge leading to usual trouble with remnants. We describe precise mechanisms, and examples from string compactifications and holographic pairs, in which these problems are evaded by either gauging or breaking the global symmetry, via (suitable versions of) Stuckelberg or Kaloper-Sorbo couplings. We argue that even in the absence of such couplings, the generic solution in string theory is the breaking of the global symmetries by cubic Chern-Simons terms involving different antisymmetric tensor fields. We conjecture that any theory with (standard or higher-degree antisymmetric tensor) gauge fields is in the Swampland unless its effective action includes such Chern-Simons terms. This conjecture implies that many familiar theories, like QED (even including the charged particles required by the Weak Gravity Conjecture) or $\mathcal{N}=8$ supergravity in four dimensions, are inconsistent in quantum gravity unless they are completed by these Chern-Simons terms.

## Full text

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## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1702.06147/full.md

## References

109 references — full list in the complete paper: https://tomesphere.com/paper/1702.06147/full.md

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Source: https://tomesphere.com/paper/1702.06147