# Search for excited electrons singly produced in proton-proton collisions   at $\sqrt{s} = 13$ TeV with the ATLAS experiment at the LHC

**Authors:** ATLAS Collaboration

arXiv: 1906.03204 · 2019-10-08

## TL;DR

This paper reports a search for excited electrons in proton-proton collisions at 13 TeV using ATLAS data, setting new limits on their possible mass and the compositeness scale, with no significant signal observed.

## Contribution

It introduces a novel search strategy for excited electrons via contact and gauge interactions, providing the most stringent limits to date on their mass and compositeness scale.

## Key findings

- No significant excess observed over background.
- Excluded excited electron masses below 4.8 TeV for certain model parameters.
- Set lower bounds on the compositeness scale up to 11 TeV.

## Abstract

A search for excited electrons produced in $pp$ collisions at $\sqrt{s} = 13$ TeV via a contact interaction $q\bar{q} \to ee^*$ is presented. The search uses 36.1 fb$^{-1}$ of data collected in 2015 and 2016 by the ATLAS experiment at the Large Hadron Collider. Decays of the excited electron via a contact interaction into an electron and a pair of quarks ($eq\bar{q}$) are targeted in final states with two electrons and two hadronic jets, and decays via a gauge interaction into a neutrino and a $W$ boson ($\nu W$) are probed in final states with an electron, missing transverse momentum, and a large-radius jet consistent with a hadronically decaying $W$ boson. No significant excess is observed over the expected backgrounds. Upper limits are calculated for the $pp \to ee^* \to eeq\bar{q}$ and $pp \to ee^* \to e\nu W$ production cross sections as a function of the excited electron mass $m_{e^*}$ at 95% confidence level. The limits are translated into lower bounds on the compositeness scale parameter $\Lambda$ of the model as a function of $m_{e^*}$. For $m_{e^*} < 0.5$ TeV, the lower bound for $\Lambda$ is 11 TeV. In the special case of $m_{e^*} = \Lambda$, the values of $m_{e^*} < 4.8$ TeV are excluded. The presented limits on $\Lambda$ are more stringent than those obtained in previous searches.

## Full text

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## Figures

19 figures with captions in the complete paper: https://tomesphere.com/paper/1906.03204/full.md

## References

91 references — full list in the complete paper: https://tomesphere.com/paper/1906.03204/full.md

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Source: https://tomesphere.com/paper/1906.03204