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http://hdl.handle.net/11452/29868
Title: | Pressure effects on the X-ray intrinsic position resolution in noble gases and mixtures |
Authors: | Azevedo, Carlos D. R. Gonzalez -Diaz, Diego Correia, Pedro M. M. Silva, Ana L. M. Carramate, Lara F. N. D. Veloso, Joao F. C. A. Uludağ Üniversitesi/Fen-Edebiyat Fakültesi/Fizik Bölümü. Biagi, Stephen 57193398882 |
Keywords: | Instruments & instrumentation Detector modelling and simulations I (interaction of radiation with matter, interaction Of photons with matter, interaction of hadrons with matter etc) Gaseous detectors Gaseous imaging and tracking detectors Charge transport and multiplication in gas Region Fwhm Argon Carbon dioxide Electric fields Gamma rays Inert gases Inverse problems Ionization of gases Mixtures Photoionization Photons Pressure effects Xenon Gamma-ray photons Microscopic simulation Modelling and simulations Photoelectron energy Position resolution Realistic detectors Tracking detectors Gases |
Issue Date: | 2-Dec-2016 |
Publisher: | IOP Publishing |
Citation: | Azevedo, C. D. R. vd. (2016). "Pressure effects on the X-ray intrinsic position resolution in noble gases and mixtures". Journal of Instrumentation, 11. |
Abstract: | A study of the effect of gas pressure in the position resolution of an interacting X or gamma-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 mu m in a realistic detector are shown and discussed. |
URI: | https://doi.org/10.1088/1748-0221/11/12/P12008 https://iopscience.iop.org/article/10.1088/1748-0221/11/12/P12008 http://hdl.handle.net/11452/29868 |
ISSN: | 1748-0221 |
Appears in Collections: | Scopus Web of Science |
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