TY - JOUR
T1 - Luminescence properties of Gd2Si2O7:Ce and Gd2Si2O7:La, Ce under vacuum ultraviolet irradiation
AU - Koshimizu, M.
AU - Yanagida, T.
AU - Fujimoto, Y.
AU - Asai, K.
N1 - Funding Information:
Acknowledgements: Part of this work was carried out at the UVSOR facility and it was supported by the Joint Studies Program (2014, No. 26–546) of the Institute for Molecular Science. This work was partially supported by the SPRITS program, Kyoto University and the Cooperative Research Project of Research Institute of Electronics, Shizuoka University.
Publisher Copyright:
© 2016 The Chinese Society of Rare Earths
PY - 2016/8/1
Y1 - 2016/8/1
N2 - The luminescence properties of Ce- or Ce and La-doped gadolinium pyrosilicate (Gd2Si2O7, GPS) were characterized using vacuum ultraviolet (VUV) excitation light. A prominent emission band was observed in the luminescence spectra with excitation at 60 nm and ascribed to 5d-4f transition of Ce3+. Because the excitation wavelength of 60 nm corresponded to the excitation in the host matrix, this result indicated that the excitation energy transfer occurred from the host matrix to Ce3+ ions. On the basis of the rise in the luminescence time profiles with excitation at 60 nm, the energy transfer occurred within 2 ns, which was much shorter than that of Ce-doped Gd2SiO5. For Ce-doped GPS, the decay rate was slower for the host excitation than that for direct excitation of Ce3+. In contrast, for Ce and La-doped GPS, no significant difference was observed for the host excitation and direct excitation of Ce3+. This result indicated that the energy transfer from the host to Ce3+ ions led to a different radiative decay process, and that La doping had an effect on the energy transfer and decay process.
AB - The luminescence properties of Ce- or Ce and La-doped gadolinium pyrosilicate (Gd2Si2O7, GPS) were characterized using vacuum ultraviolet (VUV) excitation light. A prominent emission band was observed in the luminescence spectra with excitation at 60 nm and ascribed to 5d-4f transition of Ce3+. Because the excitation wavelength of 60 nm corresponded to the excitation in the host matrix, this result indicated that the excitation energy transfer occurred from the host matrix to Ce3+ ions. On the basis of the rise in the luminescence time profiles with excitation at 60 nm, the energy transfer occurred within 2 ns, which was much shorter than that of Ce-doped Gd2SiO5. For Ce-doped GPS, the decay rate was slower for the host excitation than that for direct excitation of Ce3+. In contrast, for Ce and La-doped GPS, no significant difference was observed for the host excitation and direct excitation of Ce3+. This result indicated that the energy transfer from the host to Ce3+ ions led to a different radiative decay process, and that La doping had an effect on the energy transfer and decay process.
KW - energy transfer
KW - rare earths
KW - scintillation
KW - vacuum ultraviolet
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U2 - 10.1016/S1002-0721(16)60094-7
DO - 10.1016/S1002-0721(16)60094-7
M3 - Article
AN - SCOPUS:84991672401
SN - 1002-0721
VL - 34
SP - 782
EP - 785
JO - Journal of Rare Earths
JF - Journal of Rare Earths
IS - 8
ER -