# Neutron activation and prompt gamma intensity in Ar/CO$_{2}$-filled   neutron detectors at the European Spallation Source

**Authors:** E. Dian (1, 2, 3), K. Kanaki (2), R. J. Hall-Wilton (2, 4), P., Zagyvai (1, 3), Sz. Czifrus (3) ((1) Hungarian Academy of Sciences, Centre, for Energy Research, Budapest, Hungary, (2) European Spallation Source ESS, ERIC, Lund, Sweden, (3) Budapest University of Technology, Economics,, Institute of Nuclear Techniques, Budapest, Hungary, (4) Mid-Sweden, University, Sundsvall, Sweden)

arXiv: 1701.08117 · 2017-06-19

## TL;DR

This study uses Monte Carlo simulations to analyze neutron activation effects in Ar/CO₂ neutron detectors at the European Spallation Source, finding that only argon-40 activation significantly impacts the detector environment.

## Contribution

The paper presents a validated MCNP6.1 model to quantify neutron activation effects in Ar/CO₂ detectors, highlighting the limited impact of gamma emissions and argon-41 activity.

## Key findings

- $^{40}$Ar activation is the primary concern among neutron activation effects.
- Prompt gamma emissions from $^{40}$Ar neutron capture do not significantly affect background levels.
- $^{41}$Ar activity does not impact gamma dose rates around the detector.

## Abstract

Monte Carlo simulations using MCNP6.1 were performed to study the effect of neutron activation in Ar/CO$_{2}$ neutron detector counting gas. A general MCNP model was built and validated with simple analytical calculations. Simulations and calculations agree that only the $^{40}$Ar activation can have a considerable effect. It was shown that neither the prompt gamma intensity from the $^{40}$Ar neutron capture nor the produced $^{41}$Ar activity have an impact in terms of gamma dose rate around the detector and background level.

## Full text

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## Figures

12 figures with captions in the complete paper: https://tomesphere.com/paper/1701.08117/full.md

## References

45 references — full list in the complete paper: https://tomesphere.com/paper/1701.08117/full.md

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Source: https://tomesphere.com/paper/1701.08117