Energy and Timing Response of Six Prototype Scintillators for TOF-PET
The recent development of fast scintillating crystals with high light output (such as LaBr 3 , LYSO, and LSO) has made it possible to incorporate time-of-flight information into whole-body positron emission tomography scanners (TOF-PET). The development of fast scintillators has continued, and scint...
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Published in | IEEE transactions on nuclear science Vol. 55; no. 3; pp. 1404 - 1408 |
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Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
New York
IEEE
01.06.2008
The Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
Subjects | |
Online Access | Get full text |
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Summary: | The recent development of fast scintillating crystals with high light output (such as LaBr 3 , LYSO, and LSO) has made it possible to incorporate time-of-flight information into whole-body positron emission tomography scanners (TOF-PET). The development of fast scintillators has continued, and scintillators such as CeBr 3 and the six crystals we report on here are candidates for future TOF-PET scanners. We have performed preliminary tests on six prototype scintillating crystals composed of YI 3 (2% Ce), (Lu,Gd)I 3 (2% Ce), Lul 3 (10% Ce), Lul 3 (5% Ce), Lul 3 (2% Ce), and Ce(Br,Cl) 3 . The crystals were coupled to a PMT to observe 511 keV photons produced by positron captures in a 22 Na point source. A LaBr 3 coincidence detector was used in order to make timing resolution measurements. The prototype samples had a range of timing resolutions from 160 ps to 250 ps (FWHM). Ce(Br,Cl) 3 was found to have the best timing resolution, with 160 ps, followed by Lul 3 (2% Ce) with 180 ps. These results are competitive with the 160 ps we observed for a pair of LaBr 3 crystals in coincidence with each other. The 2% Ce doped Lul 3 sample was found to have the best overall energy response, with an energy resolution (FWHM) of 6% at 511 keV. Energy resolution and light yield measurements are presented for each of the crystals. |
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Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
ISSN: | 0018-9499 1558-1578 |
DOI: | 10.1109/TNS.2008.921939 |