摘要
在化学计量的Bi_2O_3(5N)和 GeO_2(6N)的配料里,加入0.01wt%Nd_2O_3,0.01wt%Er_2O_3,0.02wt%Cr_2O_3或0.02wt%Fe_2O_3,用 Bridgman 方法生长 Bi_4Ge_3O_(12)掺杂晶体。给出 eulytite 的结构投影和 BGO 晶体的点阵常数。掺杂稀土 BGO 晶体的室温吸收光谱由稀土离子所特有的几个吸收带所组成。采用3d^3电子的能量久期方程计算 O_h 场下掺 Cr^(3+)BGO 的库仑相互作用参数和内晶体场参数,其吸收光谱是由基态~4A_2到~2E,~4T_2和~4T_1跃迁的三个带组成。以300nm 激发观察到纯锗酸铋强的宽带发光,其峰值位置在498和550nm。这种发射被认为是 Bi^(3+)的~3P_1→~1S_0跃迁。由于存在大的 Stokes 迁移,Bi^(3+)系统猝灭心受到阻止。另外,由于~3P-~1S 能级差别大,使多声子过程中的非辐射衰减亦受到限制。通过接收498nm 发射波长,测量纯 BGO 室温激发光谱,其峰值位置在250、272和285nm,这和 M.J.Weber 测定的吸收收和反射光谱的结果基本一致。按不同波长范围分别采用光电倍增管和 PbS 接收,测量了 BGO 掺 Nd^(3+)的~4F_(3/2)→~4I_(11/2),~4I_(13/2)跃迁;掺 Er^(3+)的~4I_(13/2)→~4I_(15/2)跃迁的荧光光谱。强的荧光发射以及发射带宽界于 YAG和玻璃之间,表明掺杂稀土的 BGO 晶体是一类有希望的激光材料。
Cubic zirconia crystals stabilized by yttria with or without dopants were obtai-ned by skull-melting technique.The different dopant compositions were CeO_2 (0.01,0.3 and 0.5 wt%),Fe_2O_3 0.03 wt%+CeO_2 0.01 wt%,Fe_2O_3 0.03 wt%+CeO_20.03 wt%,CoO (0.1 and 0.3 wt%),Cr_2O_3 1wt% respectively.The optical ab-sorption spectra of these crystals in the range of 300-800 nm were measured with aBeckman modle UV 5270 spectrometer at room temperature.The absorption spectraof the crystals grown in air,or further irradiated by ^(60)Co -ray,were recorded.Theexperimental results show that new absorption spectrum bands will appear for suchcrystals doped with Ce or Co,because of Ce^(4+) changing into Ce^(3+),or Co^(3+) intoCo^(2+) during irradiation.For those crystals doped with Cr,there will not appear anynew absorption spectrum bands after irradiation.The luminescence spectra of the crystals doped with Cr or Er,etc.were alsomeasured and discussed.
出处
《无机材料学报》
SCIE
EI
CAS
CSCD
北大核心
1990年第4期297-306,共10页
Journal of Inorganic Materials
关键词
Bi4Ge3O2
BGO
晶体
稀土元素
光谱
Cubic zirconia doped crystals
Absorption spectra
Luminescence spectra
γ-ray irradiation
Transitional metals
Rare earth