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A New X-Ray Spectroscopy Concept-Room Temperature Mercuric Iodide with Peltier-Cooled Preamplification(1)

Published online by Cambridge University Press:  06 March 2019

G.C. Huth
Affiliation:
University of Southern California, School of Medicine, Medical Imaging Science Group, 4676 Admiralty Way, Marina del Rey, California 90291
A.J. Dabrowski
Affiliation:
University of Southern California, School of Medicine, Medical Imaging Science Group, 4676 Admiralty Way, Marina del Rey, California 90291
M. Singh
Affiliation:
University of Southern California, School of Medicine, Medical Imaging Science Group, 4676 Admiralty Way, Marina del Rey, California 90291
T.E. Economou
Affiliation:
University of Southern California, School of Medicine, Medical Imaging Science Group, 4676 Admiralty Way, Marina del Rey, California 90291
A. L. Turkevich
Affiliation:
University of Southern California, School of Medicine, Medical Imaging Science Group, 4676 Admiralty Way, Marina del Rey, California 90291
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Extract

Mercuric iodide (HgI2) with high atomic numbers of 80 and 53 for the components, and wide bandgap (2.1 eV) has been considered a potentially useful material for gamma ray spectroscopy for the last number of years. Considerable effort by numerous groups has been directed toward purification and growth of large single crystals of this material. Even with continuing improvement, however, the material is still characterized by good electron transport properties and only modest to poor hole transport behavior. Interesting results nevertheless have been reported in mid-range gamma ray spectroscopy using “up to millimeter thick sections of HgI2. One question always asked is: has the fundamental of lattice scattering etc. been reached in increasing hole transport behavior in this material? There is interesting speculation at this time that this may not be so.

Type
Research Article
Copyright
Copyright © International Centre for Diffraction Data 1978

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Footnotes

(2)

On leave from Institute of Nuclear Research, Swierk, Poland.

*

Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637

(1)

Research supported by Department of Energy Funding under Contract EY-76-S-03-0113 and Planetology Program, Office of Space Science, NASA, under Contract NGR-14-Q01-135.

References

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