Abstract

Transparent Ce:lutetium aluminum garnet (Ce:Lu<sub>3</sub>Al<sub>5</sub>O<sub>12</sub>, Ce:LuAG) ceramics have been regarded as potential scintillator materials due to their relatively high density and atomic number (<i>Z</i><sub>eff</sub>). However, the current Ce:LuAG ceramics exhibit a light yield much lower than the expected theoretical value due to the inevitable presence of Lu<sub>Al</sub> antisite defects at high sintering temperatures. This work demonstrates a low-temperature (1100 ℃) synthetic strategy for elaborating transparent LuAG–Al<sub>2</sub>O<sub>3</sub> nanoceramics through the crystallization of 72 mol% Al<sub>2</sub>O<sub>3</sub>–28 mol% Lu<sub>2</sub>O<sub>3</sub> (ALu28) bulk glass. The biphasic nanostructure composed of LuAG and Al<sub>2</sub>O<sub>3</sub> nanocrystals makes up the whole ceramic materials. Most of Al<sub>2</sub>O<sub>3</sub> is distributed among LuAG grains, and the rest is present inside the LuAG grains. Fully dense biphasic LuAG–Al<sub>2</sub>O<sub>3</sub> nanoceramics are highly transparent from the visible region to mid-infrared (MIR) region, and particularly the transmittance reaches 82% at 780 nm. Moreover, Lu<sub>Al</sub> antisite defect-related centers are completely undetectable in X-ray excited luminescence (XEL) spectra of Ce:LuAG–Al<sub>2</sub>O<sub>3</sub> nanoceramics with 0.3–1.0 at% Ce. The light yield of 0.3 at% Ce:LuAG–Al<sub>2</sub>O<sub>3</sub> nanoceramics is estimated to be 20,000 ph/MeV with short 1 μs shaping time, which is far superior to that of commercial Bi<sub>4</sub>Ge<sub>3</sub>O<sub>12</sub> (BGO) single crystals. These results show that a low-temperature glass crystallization route provides an alternative approach for eliminating the antisite defects in LuAG-based ceramics, and is promising to produce garnet-based ceramic materials with excellent properties, thereby meeting the demands of advanced scintillation applications.

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