Effects of charge compensation on red emission in CaYAl3OT7：Eu3＋ phosphor

Monovalent ions Li＋, Na＋, and K＋, as charge compensators, are introduced into CaYA1307： M （M = Eu3＋, Ce~＋） in this letter. Their crystal phases and photoluminescence properties of different alkali metal ions doped in CaYA1307 are investigated. In addition, the influence of charge compensation ion Li＋ which has a more obvious role in improving luminescence intensity on CaYA1307： Eu3＋ phosphor is intentionally discussed in detail and a possible mechanism of charge compensation is given. The enhancement of red emission centered at 618 nm belonging to Eu3＋ is achieved by adding alkali metal ion Li＋ under 393-nm excitation.     

Preparation and characterization of nanosized GdxBi0.95-xVO4：0.05Eu3＋ solid solution as red phosphor

A complete solid solutions with monophasic zircon-type structure of vanadates of formula GdxBio.95-xVO4：0.05Eu3＋ （x = 04）.95） are synthesized by combined method of co-precipitation and hydrothermal synthesis. Their microstructures and morphologies are characterized by X-ray powder diffraction and transmission electronic microscope, and the results show that each of all the samples has a monophasic zircon-type structure. The absorption spectrum of the prepared phosphor shows a blue-shift of the fundamental absorption band edge with increasing the gadolinium content. Under UV-light and visible-light excitation, all the prepared phosphors show the typical luminescence properties of Eu3＋ in the zircon-type structure. The emission intensity of GdxBi0.95-xVO4：0.05Eu3＋ （x = 0.55） is strongest in all samples under UV-light and visible-light excitations. Finally, the mechanisms of luminescence of Eu3＋ in the GdxBi0.95-xVO4：0.05Eu3＋ （x = 0-0.95） solid solutions are analyzed and discussed.     

Energy transfer relation of a novel Ce~(3+)/Pr~(3+)/Eu~(3+) co-doped Sr_(2.975-x)La_xAlO_(4+x)F_(1-x) solid solution phosphor

The photoluminescence properties and energy transfer of a new Ce3+/ Pr3+/ Eu3+co-doped solid-solution composition of Sr2.975-xLaxAlO4+xF1-x(LSAF) phosphor are investigated. Upon doping Pr3+into lattices of LSAF:Ce host,a shoulder emission peak is observed at about 620 nm, owing to the transition of1D2→3H4. Addition of Eu3+to LSAF:Ce3+, Pr3+phosphor results in a sharp emission peaked at 675 nm for the5D0→7F3transition and an increase of the intensity of red emission for Pr3+with increasing Eu3+concentration. The pathways of energy transfer among Ce3+, Pr3+, and Eu3+are proposed to be responsible for color addition of a red component to the primary yellow emission,enabling a potential adjustable color for blue excitable warm white.     

微波场作用下CaS:Eu~(2+)的快速合成及其荧光光谱特性

在微波场作用下快速合成了CaS :Eu2 +红色荧光体 ,用X射线粉末衍射 (XRD)分析证实它们是立方晶相 ,用扫描电镜 (SEM )观察了Eu2 +各种掺杂浓度下CaS :Eu2 +微晶的形貌及其粒径 ,测定了它们的荧光光谱和荧光衰减曲线。系统地探讨了Eu2 +离子浓度对晶体形貌和粒径以及荧光光谱性质之间的影响关系     

Electronic structure and photoluminescence property of a novel white emission phosphor Na_3MgZr(PO_4)_3:Dy~(3+) for warm white light emitting diodes

To explore suitable single-phase white emission phosphors for warm white light emitting diodes, a series of novel phosphors Na_3MgZr(PO_4)_3:xDy~(3+)(0 ≤ x ≤ 0.03) is prepared, and their phase purities as well as photoluminescence properties are discussed in depth via x-ray diffraction structure refinement and photoluminescence spectrum measurement.The electronic structure properties of the Na_3MgZr(PO_4)_3host are calculated. The results reveal that Na_3MgZr(PO_4)_3 possesses a direct band gap with a band gap value of 4.917 e V. The obtained Na_3MgZr(PO_4)_3:Dy~(3+) phosphors are all well crystallized in trigonal structure with space group Rc, which has strong absorption around 365 nm and can generate warm white light emissions peaking at 487, 576, and 673 nm upon ultraviolet excitation, which are attributed to the transitions from ~4F_(9/2) to ~6H_(15/2),~6H_(13/2), and ~6H_(11/2) of Dy~(3+) ions, respectively. The optimal doping content, critical distance, decay time, and Commission International de L'Eclairage(CIE) chromaticity coordinates are investigated in Dy~(3+) ion-doped Na_3MgZr(PO_4)_3. The thermal quenching analysis shows that Na_3MgZr(PO_4)_3:Dy~(3+) has a good thermal stability, and the thermal activation energy is calculated. The performances of Na_3MgZr(PO_4)_3:Dy~(3+) make it a potential single-phase white emission phosphor for warm white light emitting diode.     

Ultrabroadband mid-infrared emission from Cr~(2+):ZnSe-doped chalcogenide glasses prepared via hot uniaxial pressing and melt-quenching

We reported an ultrabroadband mid-infrared(MIR) emission in the range of 1800 nm–3100 nm at room temperature(RT) from a Cr~(2+):Zn Se-doped chalcogenide glasses(Ch Gs) and studied the emission-dependent properties on the doping methods. A series of Cr~(2+):Zn Se/As40 S57 Se3(in unit wt.%) glass-ceramics were prepared by hot uniaxial pressing(HUP)and melt-quenching methods, respectively. The glass-ceramics with MIR emission bands greater than 1000 nm were successfully prepared by both methods. The effects of matrix glass composition and grain doping concentration on the optical properties of the samples were studied. The occurrence state, morphology of the grains, and the microscopic elemental distributions were characterized using x-ray diffraction(XRD), scanning electron microscope(SEM), and energy dispersive spectrometer(EDS) analyses.     

具有D4h对称性构型的C42+分子的Jahn-Teller效应与能级分裂

依据量子理论与配位场理论,利用群论和对称性分析的方法探讨了C42+分子在具有D4h对称性构型时,E(b1g+b2g)系统的Jahn-Teller效应中的相关问题.研究了C42+分子的电子态与声子态的对称性及其活跃声子态,讨论了系统声子间的耦合与CG系数,构建了E(b1g+b2g)系统的电声耦合哈密顿量,利用幺正平移变换将系统变换到了无声子激发的空间中,由此计算出了系统无声子激发的基态与激发态及其能级,结果表明由于系统的电声耦合作用缘故,在系统的势能面上形成了四个对称性势阱.无论系统处在哪一个势阱中,在Jahn-Teller畸变之后,系统的二重简并的能级都将发生分裂,分裂后系统电子态的简并性完全被消除.文中利用群论又进一步探讨了系统的Jahn-Teller畸变方向及其基态对称性,发现系统将沿着D4h→D2h方向发生畸变.畸变后C24+分子的基态具有D2h群下的B1u对称性.     

Effect of H_3BO_3 on the phase stability and long persistence properties of Sr_(3.96)Al_(14)O_(25):Eu_(0.01)~(2+), Dy_(0.02)~(3+) phosphor

Sr3.96Al14O25:Eu2+ ,Dy3+ long persistent materials with different weights of H3BO3 prepared by the high temperature solid-state reaction method were characterized by X-ray powder diffraction (XRD), scanning electronic microscopy (SEM), photoluminescence spectra (PL), and thermoluminescence (TL). The results of XRD indicate that the 3% addition of H3BO3 favorable for the formation of pure phase Sr4Al14O25 , and SrAl12O19 was generated when there is a low content or high content of H3BO3 . The average grain sizes of samples grow bigger with an increase of H3BO3 . PL spectra show that the emission peak does not shift evidently and the emission intensity changes little, indicating that the different amount of H3BO3 has little influence on the crystal field. The decay characteristics and TL measurement show that H3BO3 affects the afterglow properties of Sr3.96Al14O25 :Eu2+ ,Dy3+ , because the increasing H3BO3 leads to more defects in the Sr4Al14O25 matrix.     

Nd:Ca4ReO(BO3)3(Re=Gd,Y)晶体最佳激光、最佳倍频及最佳自倍频方向的确定

介绍了Nd:Ca4ReO(BO3)3(Re=Gd,Y)晶体最佳激光方向、最佳倍频方向的确定.综合考虑激光受激发射截面、抽运光吸收系数、有效非线性系数的各向异性,分析了自倍频性质的空间分布,并就此确定出最佳自倍频方向 关键词： Nd:Ca4ReO(BO3)3(Re=Gd Y)晶体 激光发射 倍频 自倍频     

Model, software and database for line-mixing effects in the ν3 and ν4 bands of CH4 and tests using laboratory and planetary measurements—II: H2 (and He) broadening and the atmospheres of Jupiter and Saturn

The absorption shapes of the ν₂, ν₃ and ν₄ infrared bands of CH₄ perturbed by H₂ in large ranges of pressure and temperature have been measured in the laboratory. In order to model these spectra, the theoretical approach accounting for line-mixing effects proposed for CH₄-N₂ and CH₄-air and successfully tested in the companion paper (I), is used. As before, state-to-state rotational rates are used together with some empirical parameters that are deduced from a fit of a single room temperature spectrum of the ν₃ band at about 50 atm. The comparisons between measured and calculated spectra in the ν₃ and ν₄ regions under a vast variety of conditions (9-300 atm, 80-300 K) then demonstrate the quality and consistency of the proposed model. In the case of the ν₂ band, which is of E symmetry, specific parameters, different from those adapted to the ν₃ and ν₄ transitions of F₂ symmetry, are used for proper modeling of the spectral shape. Furthermore, as shown previously, a broad absorption feature grows underneath the ν₂ band with increasing H₂ density. The latter, for which an empirical model is proposed, is attributed to a collision-induced absorption (CIA) process in methane. From the developed models, a database and associated software are built for the updating of planetary atmospheres radiative transfer codes. The quality of these tools is then further demonstrated using emission measurements of the Jovian and Saturnian atmospheres in the ν₄ region (7-10 μm) recorded by the Short Wave Spectrometer of the Infrared Space Observatory and the Composite Infrared Spectrometer on-board Cassini. Comparisons between measured radiances and predictions confirm the failure of the purely Lorentzian approach and the quality of the proposed line-mixing model. Furthermore, it is shown that the methane CIA contribution has a significant influence on the planetary emission beyond 1400 cm⁻¹.     

The B3Π(0+) → X1Σ+ emission spectrum of 79BrF and 81BrF in the range 6250–8700 Å: Rotational analysis of bands in the v′ = 0, 1, 2, 3, 4 progressions,and merged molecular constants for the X1Σ+ and B3Π(0+) states

Sixteen emission bands of the B³Π(0⁺) → X¹Σ⁺ systems of ⁷⁹BrF and ⁸¹BrF have been analyzed rotationally. Measured line frequencies are fitted by least-squares to determine the rotational constants and origin for each band. The least-squares results for 0 ≤ v′ ≤ 4 and 4 ≤ v″ ≤ 12 are merged with constants from previously reported B ← X absorption and X-state microwave data. RKR potentials for the two states and Franck-Condon factors and r-centroids for the BrF (B-X) system are reported.