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    Luminescence and Energy Transfer between Ce<sup>3+</sup> and Pr<sup>3+</sup> in BaY<sub>2</sub>Si<sub>3</sub>O<sub>10</sub> under VUV–vis and X‑ray Excitation

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    A detailed investigation on photoluminescence properties and energy transfer (ET) dynamics of Ce<sup>3+</sup>, Pr<sup>3+</sup>-doped BaY<sub>2</sub>Si<sub>3</sub>O<sub>10</sub> is provided along with the potential X-ray excited luminescence application. The luminescence properties of Pr<sup>3+</sup> are studied in VUV–UV–vis spectral range at low temperature, and the spectral profiles of Pr<sup>3+</sup> <sup>3</sup>P<sub>0</sub> and <sup>1</sup>D<sub>2</sub> emission lines are determined using time-resolved emission spectra. Upon 230 nm excitation, the electron population from Pr<sup>3+</sup> 4f5d state to its 4f<sup>2</sup> excited state is discussed in detail. As Pr<sup>3+</sup> concentration rises, Pr<sup>3+</sup> <sup>3</sup>P<sub>0</sub> and <sup>1</sup>D<sub>2</sub> luminescence possess different concentration-related properties. The incorporation of Ce<sup>3+</sup> in the codoped sample produces the strong Ce<sup>3+</sup> luminescence under 230 nm excitation, which is the combined result of Pr<sup>3+</sup> 4f5d → Ce<sup>3+</sup> 5d ET and Ce<sup>3+</sup> intrinsic excitation. On the other hand, the increasingly strong ET of Ce<sup>3+</sup> 5d → Pr<sup>3+</sup> 4f<sup>2</sup> results in the decrease of Ce<sup>3+</sup> emission intensity and the gradual deviation of Ce<sup>3+</sup> luminescence decay from the single exponential in the system. By employing the Inokuti–Hirayama model, the dipole–dipole interaction is confirmed as the predominant multipolar effect in controlling this ET process, and the value of <i>C</i><sub><i>DA</i></sub> is determined to be 9.97 × 10<sup>–47</sup> m<sup>6</sup>·s<sup>–1</sup>. Finally, the relatively low scintillation light yield of Ce<sup>3+</sup>-doped BaY<sub>2</sub>Si<sub>3</sub>O<sub>10</sub> material impedes its application potential in the scintillator field, and the cosubstitution of Pr<sup>3+</sup> results in the observable decline of scintillation performance
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