4.5 Article Proceedings Paper

Effects of Ca2+ co-doping on the scintillation properties of LSO : Ce

Journal

IEEE TRANSACTIONS ON NUCLEAR SCIENCE
Volume 55, Issue 3, Pages 1178-1182

Publisher

IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
DOI: 10.1109/TNS.2007.913486

Keywords

Lu2SiO5; crystal growth; decay time; light output; scintillators

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In addition to desirable physical properties including a density of 7.4 g/cm(3), an effective atomic number of 66, and no hygroscopicity, Lu2SiO5:Ce has well-known scintillation properties of similar to 30 900 photons/MeV, an emission peak near 420 nm, and a decay time of similar to 43 ns. These scintillation properties are achieved with Ce doping concentrations roughly in the range of 0.05 to 0.5 atomic percent relative to Lu. These properties make Lu2SiO5:Ce a widely used scintillator in positron emission tomography, in particular. We have found that both the light output and decay time may be improved by a combination of optimized crystal growth atmosphere and co-doping with divalent cations such as Ca. Scintillation light output of similar to 38 800 photons/MeV has been achieved as well as scintillation decay time as short as 31 ns with no long components. The relationship between growth conditions, dopant concentration, decay time, and light output is well defined, thus allowing one to reliably tune the crystal to the desired combination of light output and decay time. Possible explanations of the underlying mechanism are being explored and include compensation of oxygen vacancies, alteration of the relative occupancies of the cerium lattice sites, and suppression of trapping centers. In addition to higher count-rate capability and better coincidence timing, the improved decay time is expected to be particularly advantageous for time-of-flight positron emission tomography. Also, phoswich detectors comprising standard LSO (similar to 43 ns decay time) and fast LSO (similar to 31 ns decay time) become an attractive alternative to typical phoswich designs that often suffer from problems of mismatched light outputs and indices of refraction or the absorption of one scintillator's light by the other.

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