Tm:K2YF5晶体的光谱参量计算

测量了Tm:K2YF5晶体的吸收光谱,根据Judd-Ofelt理论计算了Tm3+在K2YF5中的强度参数:Ω2=5.02×10-20cm2,Ω4=3.40×10-20cm2,Ω6=0.38×10-20cm2,以及Tm3+激发能级的自发辐射跃迁几率A,荧光分支比β,荧光寿命τ和积分发射截面∑等光谱参量.     

Tm:Lu_3Al_5O_(12)晶体的生长与光谱性能研究

采用提拉法生长高质量的纯LuAG晶体和4%(原子分数)Tm:LuAG晶体.对晶体的晶胞参数和光谱性能进行了详细的表征.研究发现:Tm~(3+)的掺入没有改变LuAG基质的晶体结构;吸收光谱中255 nm处的吸收带是由Fe~(3+),Fe~(2+)引起的;晶体在782 nm处的吸收峰,与商用AlGaAs二极管的发射波长匹配良好,吸收截面为5.07×10~(-21) cm~2.Tm:LuAG晶体在2 μm波段的荧光峰对应~3F_4-~3H_6能级之间的跃迁,荧光寿命长达11.9 ms,有利于激光的高能量调Q输出.结果表明,Tm:LuAG晶体是2 μm激光器中很有发展潜力的增益介质,将会替代Tm:YAG晶体应用于激光雷达系统.     

掺Eu3+离子Y2SiO5晶体格位选择光谱研究

分别利用白光灯、４５７－９ ｎｍ 氩离子激光、二倍频ＹＡＧ∶Ｎｄ 激光泵浦的诺丹明６Ｇ 可调谐窄线宽（０－５ ｃｍ －１） 染料激光作为光源， 以单色仪锁相放大器光电倍增管计算机数据采集系统记录光谱， 测量并研究了Ｙ２ＳｉＯ５∶Ｅｕ３ ＋ 晶体的透射光谱、荧光光谱、激发光谱和格位选择荧光光谱。５Ｄ０ →７Ｆ０，１ ，２ ，３，４ 跃迁，３０ 多根谱线（总数为５０ 根） 被观察到。在该晶体中Ｅｕ３＋ 替换Ｙ３＋ 离子， 占据两个较低对称性的光学格位， 这两个格位的５Ｄ０ ７Ｆ０ 能级跃迁谱线相隔大约只有０－２ ｎｍ ， 在室温下有一定的光谱关联。并用Ｘ射线谱对晶体的晶格常数ａ ， ｂ，ｃ 和晶面角度β进行测量， 测量结果显示掺杂后的晶格常数和未掺杂的Ｙ２ＳｉＯ５ 晶格常数基本一致。     

纳米CeO2∶Er荧光粉的光声光谱和荧光光谱研究

采用燃烧法合成了CeO2∶Er纳米荧光粉, 研究了不同粒径大小的CeO2∶Er的晶型和晶貌.TEM结果表明无定形CeO2∶Er包围着纳米晶CeO2∶Er, 可起到表面修饰的作用.光声光谱在保持纳米材料表面状态不改变的前提下, 分析了不同粒径的CeO2∶Er的光谱性质, 解释了随纳米粒径减小CeO2光谱峰吸收峰有蓝移而Er3+没有明显谱峰位移的原因.在荧光光谱中, 发现小粒径的CeO2∶Er有较大的红绿发射比, 并对该现象进行了解释.     

Yb∶YAB晶体的生长及性质

研究了ＹｂｘＹ１－ｘＡｌ３（ＢＯ３）４（Ｙｂ∶ＹＡＢ）晶体的生长及光学性质,结果表明,以Ｋ２Ｍｏ３Ｏ１０作为助熔剂生长Ｙｂ∶ＹＡＢ晶体效果较好,根据测定的Ｙｂ∶ＹＡＢ折射率计算的一类位相匹配角为θｍ（Ⅰ）＝３４°１２′,与实验测定值θｍ（Ⅰ）＝３４°３８′吻合较好。该晶体室温吸收谱在９５６和９７５ｎｍ处存在两个吸收带,适于ＩｎＧａＡｓ泵浦;室温π偏振吸收比σ偏振吸收略强;１０３和１０４μｍ处各存在一荧光峰,１０３μｍ处荧光寿命为１３７９ｍｓ;估算的发射截面数量级为１０－２１ｃｍ２     

Tm3+,Yb3+双掺KLa(WO4)2晶体的生长及光谱特性研究

以Yb3 作为Tm3 的敏化剂,采用泡生法生长了四方晶系的Tm,Yb∶KLW晶体(Tm3 ,Yb3 掺杂浓度分别为1%和8%(原子分数))。测试了晶体的红外光谱和拉曼光谱,并对出现的峰值进行了振动归属。分析了晶体的吸收光谱,计算了相应的光谱参数。从荧光光谱可以看出,在1028 nm附近,Yb3 发射主峰的发射线宽达16 nm,对应的是Yb3 的2F5/2和2F7/2的最低能态之间的跃迁;Tm3 在1768 nm处的荧光发射峰半高宽为40 nm左右。测试了晶体的上转换荧光谱,分别在485 nm,643 nm处得到了上转换蓝光和红光,并分析了相应的上转换机制。     

579.62 nm波长处Y2SiO5:Eu3+晶体永久性光谱烧孔

分别利用氩离子激光，二倍频YAG：Nd激光泵浦的诺明6G可调谐窄线宽（0．5cm^-1）染料激光和899-21可调谐染料激光作为光源，以单色仪-锁相放大器-光电倍增管-计算机数据采集系统记录光谱，对Y2SiO5：Eu^3＋晶体进行了光谱和光谱烧孔研究。在常温和液氮温度下测量了晶体的激发光谱、荧光光谱等。在16K温度下对晶体进行了光谱烧孔研究，得到了孔宽约80MHz并能保存10h的永久性光谱孔。     

bayf5∶Ce3+纳米粒子的制备与光谱性质

bayf5∶ce3+;纳米粒子;荧光光谱     

YAG∶Nd中Pr,Sm,Dy杂质对其光谱的影响

采用溶胶 -凝胶法合成了YAG∶Nd ,Re(Re =Pr,Sm ,Dy)系列化合物 ,研究了它们的光谱性质 .结果表明 :Pr3 + ,Sm3 + ,Dy3 + 对YAG基质中Nd3 + 的发光具有猝灭作用 ,属于有害杂质 ,在激光晶体原料中必须除去     

YAG∶Nd中Pr,Sm,Dy杂质对其光谱的影响

采用溶胶 -凝胶法合成了YAG∶Nd ,Re(Re =Pr,Sm ,Dy)系列化合物 ,研究了它们的光谱性质 .结果表明 :Pr3 + ,Sm3 + ,Dy3 + 对YAG基质中Nd3 + 的发光具有猝灭作用 ,属于有害杂质 ,在激光晶体原料中必须除去     

KZnF3：Eu^3＋单晶生长及光谱特性

利用Ｂｒｉｄｇｍａｎ－Ｓｔｏｃｋｂａｒｇｅｒ方法在氩气气氛下生长出ＫＺｎＦ３：Ｅｕ＾３＋单晶，测定了晶体的激发光谱、荧光发射光谱和ＥＳＲ谱，讨论了Ｅｕ离子的取代格位。     

Crystal Structures of Tris-dipivaloylmetanates of Tm~(3+) and Yb~(3+)

A series of Ln(Ⅲ) dipivaloylmethanates Ln(dpm)3 has been obtained. The crystal structures of Tm(dpm)3(1) and Yb(dpm)3(2) were determined by X-ray analysis at 200(2) K(Pmn21, Z = 2; a = 17.7509(8), b = 10.5805(4), с = 9.8380(4) ?, V = 1847.7(1) ?3 for(1) and a = 17.7272(6), b = 10.5882(3), с = 9.8440(3) ?, V = 1847.7(1) ?3 for(2)). These data complete the structural evaluation of lanthanoid tris-dipivaloylmethanates. Compounds 1 and 2 are isostructural to the complexes Ln(dpm)3(Ln = Er and Lu). It is demonstrated that the volatility of trisdipivaloylmethanates of rare earth elements increases from the complex of Lu to that of La.     

Spectroscopy and Energy Transfer in Yb3＋ and Tm3＋ Co-doped Gd3Ga5O12 Crystal

Yb3+/Tm3+ co-doped Gd3Ga5O12 single crystal with a dimension of Φ30mm×20mm was grown successfully by Czochralski method.The absorption spectrum was recorded at room temperature and used to calculate the absorption cross-section.Based on the Judd-Ofelt(J-O) theory,we obtained the three intensity parameters and spectral parameters of this crystal,such as the line strengths,oscillator strengths,radiative probabilities and radiative lifetimes as well as the fluorescent branching ratios.Room temperature fluorescence spectra and luminescence decay curves were recorded.The energy transfer between Yb3+-Tm3+ was observed and the mechanism was discussed.The stimulated emission cross-section of the 3F4→3H6 transition was calculated by the Füchtbauer-Ladenburg(F-L) equation.The potential laser gains for this transition were also investigated.This crystal is promising as a tunable infrared laser crystal at 2.0 μm.     

三苯基锡(Ⅳ)荒酸盐Ph3SnS2CN(C2H5)2的波谱及结构研究

合成了三苯基锡(Ⅳ)Ⅳ，Ⅳ-二乙基荒酸盐。通过元素分析、红外光谱和核磁共振氢谱对其结构进行了表征。用X-射线单晶衍射测定了该化合物的晶体结构；结果表明，化合物中锡原子呈五配位畸变三角双锥构型。     

Single Crystal Growth and Crystal Structure of Anhydrous Mercury(I) Nitrate,Hg2(NO3)2

Polycrystalline anhydrous Hg₂(NO₃)₂ was prepared by drying Hg₂(NO₃)₂·2H₂O over concentrated sulphuric acid. Evaporation of a concentrated and slightly acidified mercury(I) nitrate solution to which the same volumetric amount of pyridine was added, led to the growth of colourless rod‐like single crystals of Hg₂(NO₃)₂. Besides the title compound, crystals of hydrous Hg₂(NO₃)₂·2H₂O and the basic (Hg₂)₂(OH)(NO₃)₃ were formed as by‐products after a crystallization period of about 2 to 4 days at room temperature. The crystal structure was determined from two single crystal diffractometer data sets collected at —100°C and at room temperature: space group P2₁, Z = 4, —100°C [room temperature]: a = 6.2051(10) [6.2038(7)]Å, b = 8.3444(14) [8.3875(10)]Å, c = 11.7028(1) [11.7620(14)]Å, ß = 93.564(3) [93.415(2)]°, 3018 [3202] structure factors, 182 [182] parameters, R[Fμ² > 2σ(Fμ²)] = 0.0266 [0.0313]. The structure is built up of two crystallographically inequivalent Hg₂²⁺ dumbbells and four NO₃^— groups which form molecular [O₂N‐O‐Hg‐Hg‐O‐NO₂] units with short Hg‐O bonds. Via long Hg‐O bonds to adjacent nitrate groups the crystal packing is achieved. The Hg‐Hg distances with an average of d(Hg‐Hg) = 2.5072Å are in the typical range for mercurous oxo compounds. The oxygen coordination around the mercury dumbbells is asymmetric with four and six oxygen atoms as ligands for the two mercury atoms of each dumbbell. The nitrate groups deviate slightly from the geometry of an equilateral triangle with an average distance of d(N‐O) = 1.255Å.     

Synthesis and Single Crystal Structure of RbEr_2Cu_3Se_5

1 INTRODUCTION Halide fluxes are excellent media for growing single crystals of chalcogenides[1~3]. It is well known that during the single crystal growth via flux methods, occasional inclusion of the flux elements in the structure leads to the formation of new phases[4~9]. Several rare earth chalcogenides have been prepared through such reactive halid flux methods[4~9]. Thus we used RbCl as reactive flux to explore a new quaternary selenide by the reaction of ErCuSe precursor with Rb…     

Growth and Spectroscopic Properties of Nd3＋：Sr3Gd2（BO3）4 Crystal

<正>This paper reports the growth,X-ray diffraction and spectroscopy of Nd~(3+):Sr_3Gd_2(BO_3)_4 crystal.A Nd~(3+):Sr_3Gd_2(BO_3)_4 crystal with dimensions ofφ20×45 mm~3 has been grown by the Czochralski method.Nd~(3+):Sr_3Gd_2(BO_3)_4 crystal belongs to the orthorhombic system,space group Pnma(D_(2h))with a=0.7401,b=1.604 and c=0.8755 nm.The absorption and emission spectra of Nd~(3+):Sr_3Gd_2(BO_3)_4 were investigated.The absorption cross sectionσ_a is 3.11×10~(-20)cm~2 at 808 nm. The absorption transition at 808 nm has an FWHM of 14 nm.The luminescence lifetimeτ_f is 51.7 us.The emission cross sectionσ_e at 1064 nm wavelength is 1.09×10~(-19)cm~2.     

Growth and Spectral Properties of Nd^3＋ Doped KLa（MoO4）2 Crystal

1 INTRODUCTION There has been an increasing interest in the re- search of diode-pumped solid-state lasers in recent years because of the rapid development of high power diode lasers. The absorption peak of Nd3 ions at about 800 nm corresponding to 4I9/2→ 2H9/2 tran- sition is suitable for commercial laser diode GaAlAs pumping[1]. KLa(MoO4)2 is a kind of disordered crystalline host for lasing rare-earth ions[2], and it belongs to Scheelite (CaWO4) structure[3]. The disorder derives…     

Er3+:KLa(WO4)2晶体的生长与光谱性质

采用提拉法生长出尺寸为φ25mm×40mm的透明Er^3＋：KLa（WO4）2（简称Er：KLW）晶体，并确定了较佳的生长工艺。X射线粉末衍射分析结果表明该晶体为四方晶系白钨矿结构（I41／a空间群），晶格常数为a=b=0．5444（3）nm，c=1．2120（6）nm。测量了Er：KLW晶体的拉曼谱，发现了380，450和808cm^-1等钨酸根的特征振动峰。测量了晶体的吸收光谱，应用J-O理论计算了晶体中Er^3＋离子的强度参量（Ω2，Ω4，Ω6）；荧光光谱测量结果表明该晶体在1529nm附近有很强的荧光发射峰，利于产生受激辐射。