Development of Micromegas-based Time Projection Chamber for Nuclear Astrophysics Studies

TL;DR

This paper presents the development and testing of a Micromegas-based Time Projection Chamber (SAT-TPC) for nuclear astrophysics, demonstrating accurate track reconstruction and simulation validation.

Contribution

The paper introduces a novel Micromegas-based active-target detector for nuclear astrophysics with optimized operation and validated simulation models.

Findings

Successful characterization of Micromegas detector in test chamber.

Accurate reconstruction of alpha-particle tracks.

Good agreement between experimental data and simulations.

Abstract

A Micromegas-based active-target detector named SAT-TPC (Saha Active Target TPC) has been designed and fabricated at the Saha Institute of Nuclear Physics. The SAT-TPC was tested with Ar-CO2 (90:10) and Ar-iC4H10 (95:5) at atmospheric pressure. The Micromegas detector was first characterized in a small test chamber to optimize the ratio between the drift and amplification fields to maximise electron transparency. After establishing the optimal operating parameters, the same Micromegas detector was employed as the readout plane of the SAT-TPC prototype. The energy resolution for 55Fe and 241Am was estimated. A straightforward analysis of {\alpha}-particle tracks has been carried out, demonstrating the pad plane's capability to accurately reconstruct the direction and length of trajectories. A hydrodynamic model based on Geant4, Garfield++ and COMSOL was used to emulate the reconstructed {\alpha}-tracks in the active gas volume. The results show good agreement with simulations, confirming the accuracy of the models employed for {\alpha}-particles in Ar-CO2 (90:10) and Ar-iC4H10(95:5) gas.