# Stability tests performed on the triple GEM detector built using   commercially manufactured GEM foils in India

**Authors:** Mohit Gola, Shivali Malhotra, Ashok Kumar, Md. Naimuddin

arXiv: 1907.09322 · 2019-08-09

## TL;DR

This study evaluates the stability and gain performance of triple GEM detectors built with commercially manufactured GEM foils from India, focusing on effects of high flux and long-term operation.

## Contribution

It provides new insights into the stability and gain behavior of GEM detectors using Indian-manufactured foils under high flux conditions.

## Key findings

- Gain stability affected by X-ray induced polarisation.
- Small-scale structures mitigate space charge effects.
- Stable gain achieved at fluxes of MHz/mm^2.

## Abstract

The Gas Electron Multiplier (GEM) technology is based on thin polymer foils cladded with copper on both the sides with a regular matrix of holes. Due to the limited manufacturing capacity of CERN, these GEM foils are now commercially manufactured also by Micropack Pvt. Ltd., a company based in India. In order to gain an insight on the behaviour of detectors built using the foils from Micropack, it is important to study various long and short term effects on these foils due to the applied voltage as well as the flux of the incident particles. In this paper, we report the effect on gain stability of triple GEM detectors due to the polarising field induced by X-rays on the polyimide foils. Also, reducing the size of the amplifying structure to the microscopic scale results in a quick mitigation of the space charge effects which in turn helps in attaining a stable gain at very high incident flux. We report on the measurements of variations in the effective gain at very high particle flux of the order of $ \rm MHz/mm^2$

## Full text

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## Figures

18 figures with captions in the complete paper: https://tomesphere.com/paper/1907.09322/full.md

## References

24 references — full list in the complete paper: https://tomesphere.com/paper/1907.09322/full.md

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Source: https://tomesphere.com/paper/1907.09322