Development of High-Resolution Muon Tracking Systems Based on Micropattern Detectors

TL;DR

This paper reports on the development and testing of high-resolution muon tracking detectors using Micromegas and GEM technologies, demonstrating sub-100 micron spatial resolution and high efficiency for high-energy muon detection in CERN environments.

Contribution

It introduces new high-precision muon detectors with detailed signal analysis and background sensitivity studies, advancing detector performance in high-rate environments.

Findings

Achieved 80um spatial resolution with Micromegas detectors.

Demonstrated >99% detection efficiency for 140GeV muons.

Analyzed detector response and background sensitivity in CERN-like conditions.

Abstract

A muon tracking system consisting of four 9cm x 10cm sized bulk Micromegas detectors with 128um amplification-gap and two 10cm x 10cm triple GEM detectors is foreseen for high-precision tracking of 140GeV muons at the H8 beamline at CERN with a rate of up to 10kHz and an overall resolution below 40um. Larger detectors with an active area of 0.5m^2 and more are under development for detector studies in high neutron or gamma ray background environments at the Gamma Irradiation Facility at CERN and the Munich tandem accelerator. Signal studies of both detector types have been performed by recording cosmic muon and 5.9keV X-ray signals with a single charge-sensitive preamplifier using several gas-mixtures of Ar:CO_2. The signals were digitized using 1GHz VME based flashADCs with 2520 sampling points. The analysis of the complete signal-cycles allows for the determination of rise times, pulse heights, timing fluctuations and discrimination of background, resulting in a FWHM energy resolution of about 20% and detection efficiencies of 99% and more. Models for signal formation in both detector types will be presented. The single detector spatial resolution of 80um was measured using a fast Gassiplex based strip readout with readout strips of 150um width and a pitch of 250um. The Gassiplex readout, formerly used at the HERMES experiment, had to be substantially adapted. No more crosstalk or non-linearities were observed after reconfiguration of the multiplexing amplifier on the frontend boards. The observed spatial resolution is limited by multiple scattering of the cosmic muons used in the laboratory. We also report on the sensitivity to gamma- and neutron background and on the behaviour of spatial resolution as a function of background rates.