Abstract

A study of the effect of gas pressure in the position resolution of an interacting X or γ-ray photon in a gas medium is performed. The intrinsic position resolution for pure noble gases (Argon and Xenon) and their mixtures with CO2 and CH4 was calculated for several gas pressures (1–10 bar) and for photon energies between 1 and 60 keV, being possible to establish a linear relation between the intrinsic position resolution and the inverse of the gas pressure in the indicated energy range, as intuitively expected. We show how, at high pressures and low photoelectron energies, this intrinsic 1/P scaling is modified due to the diffusion of the primary ionization in the direction perpendicular to the electric field. In order to evaluate the quality of the method here described, a comparison between the available experimental data and microscopic simulations is presented in this work and discussed. In the majority of cases, a good agreement is observed. The conditions to achieve position resolutions down to 10 μm in a realistic detector are shown and discussed.

Highlights

  • : A study of the effect of gas pressure in the position resolution of an interacting X or γ-ray photon in a gas medium is performed

  • The intrinsic position resolution for pure noble gases (Argon and Xenon) and their mixtures with CO2 and CH4 was calculated for several gas pressures

  • The position resolution was taken as the Full Width at Half Maximum (FWHM) of a Gaussian function fitted to the projected data of the constructed image, following the Line Spread Function (LSF) method used in [13]

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Summary

Introduction

: A study of the effect of gas pressure in the position resolution of an interacting X or γ-ray photon in a gas medium is performed. The intrinsic position resolution for pure noble gases (Argon and Xenon) and their mixtures with CO2 and CH4 was calculated for several gas pressures (1–10 bar) and for photon energies between 1 and 60 keV, being possible to establish a linear relation between the intrinsic position resolution and the inverse of the gas pressure in the indicated energy range, as intuitively expected. JINST 11 P12008 to decouple the position resolution from the detector gain and electrons diffusion during the drift, the intrinsic position resolution of pressurized pure noble gases (Argon and Xenon, in the pressures range 1–10 bar) was calculated. We have extended our previous simulation code to compute the position resolution at high pressure, including the unavoidable effect of diffusion, providing a more realistic ionization cloud

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