DocumentCode
3600400
Title
A new coplanar-grid high-pressure xenon gamma-ray spectrometer
Author
Kiff, Scott D. ; He, Zhong ; Tepper, Gary C.
Author_Institution
Michigan Univ., Ann Arbor, MI, USA
Volume
1
fYear
2004
Firstpage
475
Abstract
High-pressure xenon (HPXe) gas is a desirable radiation detection medium for many reasons, including its large atomic number, high density, low mean ionization energy, and the ability to produce devices with large detection volumes. While past work in HPXe has produced relatively successful detectors with energy resolution at 662 keV as good as approximately 2% FWHM, an expected limitation of these chambers in field operation is resolution degradation due to the vibration of their Frisch grids. Progress on a detector without a Frisch grid is reported in this submission; it is expected that the proposed anode design will provide competitive energy resolution with minimal degradation from mechanical vibration. Simulations accounting for variations due to charge carrier statistics, changes in the charge induced on the anode as a function of interaction location, and electronic noise predict an energy resolution of 2.3% FWHM at 662 keV. Experimental data is compared with these simulations.
Keywords
anodes; gamma-ray detection; gamma-ray spectrometers; noise; Frisch grid vibration; anode design; atomic number; charge carrier statistics; coplanar-grid high-pressure xenon gamma-ray spectrometer; detection volumes; electronic noise; energy resolution; experimental data; induced anode charge; interaction location; mean ionization energy; mechanical vibration; radiation detection medium; resolution degradation; simulations; Anodes; Atomic measurements; Degradation; Energy resolution; Ionization; Predictive models; Radiation detectors; Spectroscopy; Vibrations; Xenon;
fLanguage
English
Publisher
ieee
Conference_Titel
Nuclear Science Symposium Conference Record, 2004 IEEE
ISSN
1082-3654
Print_ISBN
0-7803-8700-7
Electronic_ISBN
1082-3654
Type
conf
DOI
10.1109/NSSMIC.2004.1462237
Filename
1462237
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