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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Abstract
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