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Bi3+掺杂Y2O3激发光谱和斯托克斯位移的从头算嵌入簇研究

Ab initio embedded cluster study of the excitation spectrum and Stokes shifts of Bi3+-doped Y2O3.

作者信息

Réal Florent, Vallet Valérie, Flament Jean-Pierre, Schamps Joël

机构信息

Laboratoire PhLAM (CNRS UMR 8523), CERLA (CNRS FR 2416), Université de Sciences et Technologies de Lille 1, F-59655 Villeneuve d'Ascq Cedex, France.

出版信息

J Chem Phys. 2007 Sep 14;127(10):104705. doi: 10.1063/1.2768532.

DOI:10.1063/1.2768532
PMID:17867767
Abstract

The ab initio embedded cluster method coupled with correlated spin-orbit calculations has been used to interpret the excitation spectrum of a Bi(3+)-doped yttria crystal. Our results indicate that the Bi(3+) impurity can absorb light over a wider energy range in the C(2) site than in the S(6) site. Even if the computed absorption energies seem to be about 0.4 eV too high with respect to the experimental peaks for both sites, it is noteworthy that the embedded cluster model renders 93% of the large crystal redshift, about 6 eV. The determination of the geometry relaxation of the first shell of oxygen neighbors upon electronic excitation shows that the Stokes shift is smaller in the S(6) site than in the C(2) site. Combining all these results confirms the assignment of the violet emission to the S(6) site and that of the green emission to the C(2) site, as proposed by Boulon [J. Phys. (Paris) 32, 333 (1971)]. In addition, the nature of the metastable states which lie below the emitting ones and are responsible for the temperature dependence of the fluorescence lifetimes is discussed.

摘要

从头算嵌入簇方法结合相关自旋轨道计算已被用于解释Bi(3+)掺杂氧化钇晶体的激发光谱。我们的结果表明,Bi(3+)杂质在C(2)位点比在S(6)位点能在更宽的能量范围内吸收光。即使计算得到的吸收能量相对于两个位点的实验峰似乎都高约0.4 eV,但值得注意的是,嵌入簇模型给出了约6 eV的大晶体红移的93%。对电子激发时第一壳层氧邻居的几何弛豫的测定表明,S(6)位点的斯托克斯位移比C(2)位点小。综合所有这些结果,证实了如Boulon [《物理学报》(巴黎)32, 333 (1971)]所提出的,紫色发射归属于S(6)位点,绿色发射归属于C(2)位点。此外,还讨论了低于发射态且决定荧光寿命温度依赖性的亚稳态的性质。

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