Please use this identifier to cite or link to this item: 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

Files in This Item:
File Description SizeFormat 
Biagi_vd_2016.pdf222.88 kBAdobe PDFThumbnail
View/Open


This item is licensed under a Creative Commons License Creative Commons