Modeling the light response of an optically readout GEM based TPC for the CYGNO experiment
Fernando Dominques Amaro, Rita Antonietti, Elisabetta Baracchini, Luigi Benussi, Stefano Bianco, Roberto Campagnola, Cesidio Capoccia, Michele Caponero, Gianluca Cavoto, Igor Abritta Costa, Antonio Croce, Emiliano Dan\`e, Melba D'Astolfo, Giorgio Dho, Flaminia Di Giambattista

TL;DR
This paper models the light response of a GEM-based TPC for the CYGNO experiment, demonstrating accurate prediction of gain dependence on charge density, crucial for detecting rare particle interactions with high granularity.
Contribution
It introduces a new model that accurately describes and predicts the gain dependence on charge density in a GEM-based optical readout TPC.
Findings
Model reproduces gain behavior within percent-level accuracy
Gain reduction linked to space-charge effects in GEM channels
Experimental data validates the model's predictive capability
Abstract
The use of gaseous Time Projection Chambers enables the detection and the detailed study of rare events due to particles interactions with the atoms of the gas with energy releases as low as a few keV. Due to this capability, these instruments are being developed for applications in the field of astroparticle physics, such as the study of dark matter and neutrinos. To readout events occurring in the sensitive volume with a high granularity, the CYGNO collaboration is developing a solution where the light generated during the avalanche processes occurring in a multiplication stage based on Gas Electron Multiplier (GEM) is read out by optical sensors with very high sensitivity and spatial resolution. To achieve a high light output, gas gain values of the order of are needed. Experimentally, a dependence of the detector response on the spatial density of the charge…
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Taxonomy
TopicsParticle Detector Development and Performance · Dark Matter and Cosmic Phenomena · Photocathodes and Microchannel Plates
