# On Monopole Bubbling Contributions to 't Hooft Loops

**Authors:** Benjamin Assel, Antonio Sciarappa

arXiv: 1903.00376 · 2019-06-26

## TL;DR

This paper introduces an algorithmic approach to compute monopole bubbling contributions to 't Hooft loops in 4d $
=2$ theories, overcoming previous computational challenges by analyzing brane configurations and residues in flavor fugacities.

## Contribution

It presents a novel method to calculate bubbling contributions using enlarged SQMs and residues, applicable to 4d and 5d-4d coupled systems, advancing the understanding of 't Hooft loop operators.

## Key findings

- Successfully computed bubbling contributions in $
=2$ SQCD theories.
- Linked bubbling terms to residues of instanton sectors in 5d line operators.
- Provided a brane-based framework for analyzing monopole bubbling effects.

## Abstract

Monopole bubbling contributions to supersymmetric 't Hooft loops in 4d $\mathcal{N}=2$ theories are computed by SQM indices. As recently argued, those indices are hard to compute due to the presence of Coulomb vacua that are not captured by standard localization techniques. We propose an algorithmic method to compute the full bubbling contributions that circumvent this issue, by considering SQM with more matter fields and isolating the bubbling terms as residues in flavor fugacities. The enlarged SQMs are read from brane configurations realizing the bubbling sector of a given 't Hooft loop. We apply our technique to loop operators in $\mathcal{N}=2$ conformal SQCD theories. In addition we embed this discussion in the larger setup of a 5d-4d system interacting along a line, associated to the brane systems previously discussed. The bubbling terms arise from residues of specific instanton sectors of 5d line operators in this context.

## Full text

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## Figures

18 figures with captions in the complete paper: https://tomesphere.com/paper/1903.00376/full.md

## References

27 references — full list in the complete paper: https://tomesphere.com/paper/1903.00376/full.md

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Source: https://tomesphere.com/paper/1903.00376