Alkali earth co-doping effects on luminescence and scintillation properties of Ce doped Gd3Al2Ga3O12 scintillator
Introduction
Scintillator materials combined with photodetectors are used to detect high energy photons and accelerated particles in medical imaging techniques, high energy and nuclear physics detectors, high-tech industrial applications and most recently also in the advanced homeland security related techniques.[1] In the last two decades, great R&D effort brought several new material systems, namely the Ce-doped orthosilicates as Gd2SiO5 (GSO), Lu2SiO5 (LSO), (Lu1−xYx)2SiO5 (LYSO), pyrosilicates based on RE2Si2O7 (RE = Lu, Y, Gd) and most recently LaX3 (X = Cl, Br) single crystal hosts [1], [2], [3], [4], [5], [6], [7], [8], [9], [10], [11]. Oxide materials based on garnet structure single crystals are promising candidates for scintillator applications because of well mastered technology developed for laser hosts and other applications, optical transparency and easy doping by rare-earth elements. After a decade of R&D of the Lu3Al5O12 (LuAG)-based single crystal scintillators (see review in [12]), new material concept was defined, based on multicomponent (Gd, RE)3(Ga, Al)5O12 host, Re = Lu, Y. Doped by Ce3+, the Gd- and Ga rich host compositions showed amazingly high light yield up to almost 50,000 phot/MeV [13], [14], [15], [16] which is the value exceeding by 30–40% the best Ce:LYSO materials ever seen. Recently, our group reported about Ce:Gd3Al2Ga3O12 (GAGG) single crystal and scintillation response of about ∼90 ns at emission around 520 nm, excellent light yield of about 56,000 photon/MeV, and density of 6.63 g/cm3[15], [16]. In the silicate, perovskite and garnet scintillators the slow tunneling-driven radiative recombination between Ce emission centers and nearby lying electron traps can deteriorate scintillation performance [12], [17]. Ce:LSO and Ce:LYSO single crystals co-doped with Ca2+ have been recently investigated and improvement in their scintillation characteristics, namely afterglow suppression and scintillation decay acceleration, were claimed[18], [19] which is based on the suppression of such slow delayed recombination processes. Positive role of stable Ce4+ centers has been proposed in [19] to explain the improved scintillation performance. Very recently, such an approach has been used in Mg-codoped Ce:LuAG scintillation ceramics the light yield of which was enormously enhanced and the presence of Ce4+ was clearly identified by its characteristic charge transfer (CT) absorption in the near UV range below 350 nm [20]. On the contrary, strong degradation of light yield due to Ca2+ co-doping in Ce:GAGG has been recently reported [21].
The aim of this work is to investigate and compare the alkali earth (AE, AE2+ = Mg2+, Ca2+) co-doping effects on luminescence and scintillation properties of Ce:GAGG scintillator. In this report, AE co-doped Ce:GAGG single crystal were grown by the micro-pulling down (μ-PD) method and characterized as for the chemical composition. Luminescence and scintillation characteristics were also measured.
Section snippets
Crystal growth
A stoichiometric mixture of 4 N MgCO3, CaCO3, CeO2, α-Al2O3, Ga2O3 and Gd2O3, powders (High Purity Chemicals Co.) was used as starting material. Nominally, starting powders were prepared according to the formula of (AEx, Cey, Gd1−y)3Al2Ga3O12(CO3)x. Single crystals of AE (=Mg, Ca) co-doped Ce:GAGG were grown by the μ-PD method with an RF heating system. The y was 0.005 and x were 0, 0.0001, 0.0002 0.0005 and 0.001. These samples will be noted as Mg or Ca-0, 100, 200, 500 and 1000. A schematic of
Crystal growth
Mg and Ca co-doped Ce0.5%:GAGG crystals were grown by the μ-PD method. Example photos are shown in Fig. 1. The grown crystals were transparent with yellow color and 2–3 mm in diameter, 15–30 mm in length. Some of them look slightly cloudy because of the rough surface coming from the gallium oxide evaporation and thermal etching. However, the inner part of all the crystals is perfectly transparent.
Chemical composition distribution along growth direction of Ca 1000 ppm co-doped Ce0.5%:GAGG measured
Conclusion
The Mg and Ca-codoped Ce0.5%:GAGG single crystals were grown by the micro pulling down method and their optical, luminescence and scintillation characteristics were measured. The intensity enhancement of the Ce3+ emission band at 520 nm in radioluminescence spectra was observed between the Mg-0 and Mg-500 samples. The scintillation decays were accelerated by Mg co-doping and dominant decay time decreased down to 39 ns. Comparing to Ca co-doping, the Mg co-doped samples showed better figure of
Acknowledgements
This work is partially supported by (i) the funding program for next generation world-leading researchers, Japan Society for the Promotion of Science (JSPS), (ii) Development of Systems and Technology for Advanced Measurement and Analysis, Japan Science and Technology Agency (JST) (iii) Adaptable & Seamless Technology Transfer Program through Target-driven R&D (A-STEP), JST (iv) JSPS Grant-in-Aid for Exploratory Research (A.Y), (v) JSPS Research Fellowships for Young Scientists (S.Kurosawa),
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