# Search for heavy charged long-lived particles in the ATLAS detector in   36.1 fb$^{-1}$ of proton-proton collision data at $\sqrt{s} = 13$ TeV

**Authors:** ATLAS Collaboration

arXiv: 1902.01636 · 2019-06-05

## TL;DR

This paper reports a search for heavy charged long-lived particles in proton-proton collisions at 13 TeV using the ATLAS detector, setting new mass limits and cross-section constraints for various supersymmetric particles.

## Contribution

It introduces model-independent search strategies for long-lived particles and provides the first limits on their production cross sections and masses at 13 TeV.

## Key findings

- No significant excess over Standard Model background observed.
- Set lower mass limits on long-lived gluino, sbottom, stop, staus, and charginos.
- Provided upper limits on production cross sections at 95% confidence level.

## Abstract

A search for heavy charged long-lived particles is performed using a data sample of 36.1 fb$^{-1}$ of proton-proton collisions at $\sqrt{s} = 13$ TeV collected by the ATLAS experiment at the Large Hadron Collider. The search is based on observables related to ionization energy loss and time of flight, which are sensitive to the velocity of heavy charged particles traveling significantly slower than the speed of light. Multiple search strategies for a wide range of lifetimes, corresponding to path lengths of a few meters, are defined as model-independently as possible, by referencing several representative physics cases that yield long-lived particles within supersymmetric models, such as gluinos/squarks ($R$-hadrons), charginos and staus. No significant deviations from the expected Standard Model background are observed. Upper limits at 95% confidence level are provided on the production cross sections of long-lived $R$-hadrons as well as directly pair-produced staus and charginos. These results translate into lower limits on the masses of long-lived gluino, sbottom and stop $R$-hadrons, as well as staus and charginos of 2000 GeV, 1250 GeV, 1340 GeV, 430 GeV and 1090 GeV, respectively.

## Full text

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## Figures

31 figures with captions in the complete paper: https://tomesphere.com/paper/1902.01636/full.md

## References

69 references — full list in the complete paper: https://tomesphere.com/paper/1902.01636/full.md

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Source: https://tomesphere.com/paper/1902.01636