# Commissioning the SoLid Detector Using Cosmic Ray Muons

**Authors:** Giel Vandierendonck

arXiv: 1903.11842 · 2019-04-09

## TL;DR

The paper describes the commissioning process of the SoLid neutrino detector using cosmic ray muons, focusing on stability, calibration, and environmental monitoring to ensure optimal performance.

## Contribution

It demonstrates how cosmic muons can be effectively used for detector calibration, stability monitoring, and environmental correlation during the commissioning phase.

## Key findings

- Muon-based calibration and timing synchronization achieved
- Detector stability monitored via cosmic muons over time
- Secondary particles from muons used to verify detector properties

## Abstract

The SoLid detector was constructed during 2017 and started to take data in December 2017. Commissioning a new detector implies defining and understanding a whole set of new variables. On the one hand the environmental conditions are followed, and on the other hand quantities related to the stability of the detector are monitored. Cosmic muons are ideal for studying the stability of SoLid, because of their abundance due to the small overburden. Muons can be used to study the timing synchronisation and energy calibration of the detector on a daily timescale. They can be used to monitor the detector stability and to correlate it with the environmental conditions. Muons also create secondary particles along their trajectory that can be detected and used for commissioning. For instance, spallation neutrons that are thermalized and captured in the detector can be used to verify the thermalisation properties of the detector. Stopping muon decays allow for a check of the muon decay time.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1903.11842/full.md

## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1903.11842/full.md

## References

5 references — full list in the complete paper: https://tomesphere.com/paper/1903.11842/full.md

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Source: https://tomesphere.com/paper/1903.11842