新型全色发光材料NaCaPO4∶Dy3+制备及发光性能

釆用高温固相法制备了NaCaPO4∶Dy3+系列样品, 并在紫外(UV)及真空紫外(VUV)区域研究了系列样品的发光性能. 紫外激发光谱显示在350 nm处有最强的激发峰, 可以有效地吸收紫外光并将其转化为可见光. 真空紫外激发光谱表明, NaCaPO4∶Dy3+能有效地吸收无汞荧光灯的激发源并将其转化为可见光. 系列样品发光均呈现为白色, 这种材料有潜力作为全色显示材料应用于发光二极管(LED)和无汞荧光灯中.     

高温固相法合成长余辉发光材料Sr0.96Al2O4:Eu2+0.02,Dy3+0.02

以高温固相法合成了Sr0.96Al2O4:Eu2+0.02,Dy3+0.02长余辉发光材料,其激发光谱和发射光谱均为宽带谱,激发光谱为300～480nm,具有从紫外到蓝绿光波段能量的吸收范围.随着稀土元素Eu2+掺杂量的增加,发光强度逐渐增强,当Eu2+掺杂量达到2(mol)%时,材料的发光强度最大.辅助激活剂Dy3+...     

高温固相法合成长余辉发光材料Sr_(0.96)Al_2O_4:Eu_(0.02)~(2+),Dy_(0.02)~(3+)

以高温固相法合成了Sr0.96Al2O4:Eu2+0.02,Dy3+0.02长余辉发光材料,其激发光谱和发射光谱均为宽带谱,激发光谱为300～480nm,具有从紫外到蓝绿光波段能量的吸收范围.随着稀土元素Eu2+掺杂量的增加,发光强度逐渐增强,当Eu2+掺杂量达到2(mol)%时,材料的发光强度最大.辅助激活剂Dy3+的添加能显著改善材料的余辉性能.Sr0.96Al2O4:Eu2+0.02,Dy3+0.02在25W日光灯激发30min后,黑暗环境中余辉长达3h.     

Ce3+离子激活的Sr5( BO3)3F荧光材料VUV-Vis发光性质

利用高温固相法合成了一系列Ce3+掺杂的Sr-2xCexNax(BO3)3F (x=0.01,0.03,0.05,0.10,0.15,0.20,0.25,0.30,0.35)荧光粉.用XRD表征了荧光粉的相纯度.测定了材料在真空紫外-紫外(VUV-UV)范围的激发光谱和VUV-UV光激发下的发射光谱.研究结果显示:Sr5 (BO3)3F的基质吸收峰位置大约在150 ～ 190 nm范围,与Xe基稀有气体混合物等离子体发射波长吻合,适于用作PDP和无汞荧光灯用荧光粉的基质材料.从VUV-UV激发和发射光谱来分析,Ce3+在Sr5( BO3)3F中是占据了Sr(1)和Sr(2)格位,当Ce3+的掺杂浓度较低时,进入Sr(2)格位Ce3+的发光(～390 nm)较强,随着Ce3+的掺杂浓度增加,较低能量Sr(1)格位上Ce3+的发射(～450 nm)增强,因而在同一波长激发下,发射光谱随着掺杂浓度增加发生明显的红移现象,荧光体的发光颜色由蓝紫光(390 nm)向蓝绿光(453 nm)变化.     

Ce3+∶YAG闪烁晶体的真空紫外激发光谱特性

掺铈钇铝石榴石(Ce3+∶YAG)晶体是性能优良的闪烁材料. 以同步辐射光源为激发光源研究了单晶Ce3+∶YAG的真空紫外-紫外(VUV-UV)激发光谱和荧光谱. 同时也测量和分析了该晶体的吸收光谱、紫外-可见(UV-VIS)激发光谱和荧光谱.根据光谱测量的结果讨论了激发能在Ce3+∶YAG晶体中的传输过程和在Ce3+离子5d态的直接激发和YAG价带激发下Ce3+∶YAG单晶发光的差别.     

(Y,Gd)VO_4∶Eu~(3+)的紫外-真空紫外发光特性

用高温固相法合成了Y1-xGdxVO4∶Eu3 (0≤x≤1)系列单相样品并研究了其发光特性。在254nm激发下,观察到最大强度位于619nm的红色发射峰且其强度在Y/Gd=0.4/0.6时达到最大。在147nm激发下的发射峰与紫外下的一致,发射强度也是在Y/Gd=0.4/0.6时达到最大,大约是商用(Y,Gd)BO3∶Eu3 荧光体的65%。619nm监控下的真空紫外激发光谱由峰值位于158nm,204nm,247nm以及300nm的系列激发带组成,归属于钒酸根的基质吸收以及Gd3 、Y3 和Eu3 的电荷迁移带吸收。相对(Y,Gd)BO3∶Eu3 中Eu3 占据中心对称格位,(Y,Gd)VO4∶Eu3 中Eu3 占据非中心对称格位,其真空紫外下光谱色纯度更好。色坐标分别为(0.632,0.355),(0.672,0.328)。     

Sr2SiO4∶Dy3+材料制备及发光特性

采用高温固相法制备了Sr2SiO4∶Dy3+发光材料. 在365 nm紫外光激发下, 测得Sr2SiO4∶Dy3+材料的发射光谱为一个多峰宽谱, 主峰分别为486, 575和665 nm; 监测575 nm的发射峰, 所得材料的激发光谱为一个多峰宽谱, 主峰分别为331, 361, 371, 397, 435, 461和478 nm. 研究了Dy3+掺杂浓度对Sr2SiO4∶Dy3+材料发射光谱强度的影响. 研究结果显示, 随着Dy3+浓度的增大, 黄、蓝发射峰比值(Y/B)也逐渐增大; 随着Dy3+浓度的增大, 575 nm发射峰强度先增大后减小. 加入电荷补偿剂Li+, Na+和K+均提高了Sr2SiO4∶Dy3+材料的发射光谱强度, 其中以Li+的情况最为明显.     

纳米SrAl2O4:Eu2+,Dy3+长余辉发光材料的制备与性能

采用水热-均匀共沉淀法制备了纳米SrAl2O4:Eu2+,Dy3+长余辉发光材料.通过XRD、TEM、荧光光谱、热释光谱对其结构和性能进行分析.XRD结果表明所制备的SrAl2O4:Eu2+Dy3+纳米发光材料为单相,属单斜晶系.TEM测试表明纳米SrAl2O4:Eu2+,Dy3+发光材料为规则的球状粒子,粒径为50～80 nm,且分散性良好.激发和发射光谱测试表明,样品的激发光谱是峰值在356 nm 的连续宽带谱,发射光谱是峰值位于512 nm的宽带谱,与SrAl2O4:Eu2+,Dy3+粗晶材料相比,激发和发射光谱都出现了"蓝移"现象.样品的热释光峰值位于358 K,适合于产生长余辉.     

(Y,Gd)BO_3∶Eu的真空紫外光谱特性

近年来由于等离子体平板显示 (PDP)技术的需要 ,对真空紫外 (VUV)光激发的荧光粉的研究成为发光材料领域中的一个新方向 [1～ 3] .由于技术和实验仪器等方面的原因 [4 ] ,以往人们对稀土发光材料VUV区的研究很少 ,缺乏对其光谱和能级的完整认识 .另外 ,稀土离子 Gd3+在荧光粉的能量传递中具有特殊作用 ,一些含 Gd3+的发光材料在 VUV区发光效率很高 ,例如 ,(Y,Gd) BO3∶ Eu在 VUV区的发光效率比 YBO3∶ Eu提高了 2 0 % ,比 Y2 O3∶ Eu提高了 1 .8倍 ,与其它红粉相比更具有实际应用价值 [4 ,5] .但目前对于 (Y,Gd) BO3∶ Eu的研…     

白色荧光粉KCaY_(1-x)(PO_4)_2:xDy~(3+)的制备及真空紫外发光特性

一种新型具有六方晶系的KCaY_(1-x)(PO_4)_2:xDy~(3+)(0x≤0.10)白色荧光粉采用固相法被成功合成,研究了其在真空紫外激发下的发光特性。结果表明,在147 nm激发下,样品主要呈现472 nm的蓝色和578 nm的黄色发射,在578 nm监控下的激发光谱表明基质和激活离子间存在着一定的能量转移现象,因此通过固相反应制备的单一体系单一激活离子的白色荧光粉KCaY_(1-x)(PO_4)_2:xDy~(3+)(0x≤0.10)将在无汞荧光灯上有潜在的应用价值。     

GdVO_4∶Eu~(3 )的真空紫外激发光谱研究

报道了GdVO4∶Eu3 的光致发光光谱和真空紫外 紫外激发光谱。GdVO4∶Eu3 是高效率的真空紫外 紫外激发荧光材料。GdVO4∶Eu3 在6 0～ 35 0nm真空紫外 紫外波段的激发可能主要来源于基质的吸收 ,有明显的Eu3 及Gd3 的 4fn - 1 5d吸收。在GdVO4∶Eu3 中 ,存在如下能量传递过程 :VO3 - 4 →Eu3 ,Gd3 →Eu3 ,Gd3 →VO3 - 4 →Eu3 ;通过后两个过程 ,Gd3 Eu3 可实现量子剪裁。     

The dependence of DNA luminescence on excitation wavelength in the UV/VUV region

Luminescence emission and excitation spectra have been obtained for DNA films at 77 K under vacuum ultraviolet excitation (150–280 nm). The emission spectra, which cover the wavelength range 310 to 490 nm, consists of two components, a short-lived component around 350 nm which is attributed to fluorescence and a longer-lived component around 410 nm believed to be phosphorescence. The excitation spectra, as functions of emission wavelength, are similar in profile with a fairly broad peak around 9240–260 nm) with a shoulder around 200 nm followed by a gradual but constant decrease into the vacuum ultraviolet region of the spectrum. No evidence of autoionization was seen in the region investigated.     

NaGdF_4:Eu~(3 )的结构和VUV荧光性质

利用水热方法合成了纯度较高的六方结构的 NaGdF4,在氧气存在条件下 950℃加热处理可以使其转变为 CaF2型立方结构。在真空紫外光激发下,六方结构的 NaGdF4∶ Eu3＋中的 Gd3＋离子吸收一个光子,并将能量分两步传递给 Eu3＋离子,发生双光子发射。立方结构的 NaGdF4∶ Eu3＋中存在有一定量的氧离子取代缺陷,使 Gd3＋离子 4f-5d跃迁移到 177nm附近,这与惰性气体放电产生的真空紫外光波长一致。     

High-resolution Absorption Spectra of Acetylene in 142.8-152.3 nm

The absorption spectra of acetylene molecules was measured under jet-cooled conditions in the wavelength range of 142.8-152.3 nm,with a tunable and highly resolved vacuum ultraviolet (VUV) laser generated by two-photon resonant four wave difference frequency mixing processes. Due to the sufficient vibrational and rotational cooling effect of the molecular beam and the higher resolution VUV laser, the observed absorption spectra exhibit more distinct spectral features than the previous works measured at room temperature. The major three vibrational bands are assigned as a CC symmetry stretching vibrational progress (v2=0-2) of the C1Ⅱu state of acetylene.The observed shoulder peak at 148.2 nm is assigned to the first overtone band of the trans-bending mode v4 of the C1Ⅱu state of acetylene. Additionally,the two components, 420 (μ1Ⅱu) and 420(к1Ⅱu),are suggested to exhibit in the present absorption spectra,due to their Renner-Teller effect and transition selection rule.All band origins and bandwidths are obtained subsequently,and it is foundthat bandwidths are broadened and lifetimes decrease gradually with the excitation of vibration.     

Subsurface investigation of the surface modification of polydimethylsiloxane by 172‐nm vacuum ultraviolet irradiation using ToF‐SIMS and VUV spectrometry

We investigate the mechanism of polydimethylsiloxane (PDMS) surface modification by 172‐nm vacuum ultraviolet (VUV) light. Time‐of‐flight secondary ion mass spectrometry and optical spectrometry are used to measure the chemical composition and VUV transmittance of the PDMS before and after surface modification, respectively. For modified samples of bulk PDMS, the VUV transmittance and the depth of the modified region increased with increasing VUV dose. This can be explained by the following self‐reinforcing cycle of (1) modification of PDMS by VUV light to a more silica‐like composition, (2) improvement of the VUV light transparency, and (3) deeper modification. For thin‐film samples of PDMS formed on sapphire substrates, the transmittance at 172 nm also increased with increasing VUV dose and exceeded that of sapphire in the region from 172 to 300 nm. Finally, thin‐film samples of PDMS formed on silicon substrates, which function as a VUV reflector, were also investigated. For these samples, the secondary ion depth profiles for several chemical species in the PDMS were oscillatory, probably due to the interference of the incident and reflected VUV light. These results strongly suggest that the photon energy of the VUV light plays an important role in modifying PDMS.     

Spectroscopy of Dibenzorubicene: Experimental Data for a Search in Interstellar Spectra

We report on the characterization of dibenzo[cde,opq]rubicene (C₃₀H₁₄). The molecule was studied in solution at room temperature with absorption spectroscopy in the visible (vis) and ultraviolet (UV) wavelength ranges, and with emission spectroscopy. The infrared (IR), visible, ultraviolet, and vacuum ultraviolet (VUV) absorption spectra of a thin film were measured also at room temperature. In addition, the UV/vis absorption spectrum was measured at cryogenic temperatures using the matrix isolation spectroscopy technique. The interpretation of spectra was supported by theoretical calculations based on semiempirical and ab initio models, as well as on density functional theory. Finally, the results of the laboratory study were compared with interstellar spectra.     

Photophysical properties of praseodymium complexes with aromatic carboxylic acids: double light conversion both in ultraviolet and visible region

A series of luminescent praseodymium complexes with different aromatic carboxylic acids have been synthesized and characterized. The photophysical properties of these complexes have been studied with ultraviolet spectra, phosphorescence spectra and fluorescence spectra. Ultraviolet absorption spectra show that the praseodymium complexes systems with aromatic carboxylate form the more extensive conjugated systems to be suitable for the distribution of electron in the whole coordination environment, resulting in the energy decrease and red-shifts of ultraviolet spectral bands. Phosphorescence spectra suggest that excited triplet state of aromatic carboxylic acids, which can indicate the energy match and intermolecular energy transfer process between the excited triplet state of ligands and the resonant emissive energy level of Pr ions. The emission spectra of all praseodymium complexes show two emission peaks under the excitation band of 245 nm at about 395 and 595 nm, respectively, while one peak at about 595 nm under 415 nm excitation, which attributed to be 1S0-->1I6 (395 nm) transition and the characteristic emission 1D2-->3H4 (595 nm) transition of Pr3+ ion. The 1S0-->1I6 transition can be speculated to belong to the transition of charge transfer state, and the 1D2-->3H4 can be further proved that there exists an antenna effect in the luminescence of praseodymium with aromatic carboxylic acids. In conclusion, the praseodymium complexes systems can realize the double proton light conversion both in the ultraviolet and visible region, which can be further studied to have potential application.     

Regulation of pattern dimension as a function of vacuum pressure: alkyl monolayer lithography

Photopatterning of a hexadecyl (HD) monolayer has been demonstrated using vacuum ultraviolet (VUV; lambda = 172 nm) light under controlled vacuum pressure with the objective of minimizing the pattern dimension. X-ray photoelectron spectroscopy (XPS) and lateral force microscopy (LFM) studies reveal that photodegradation of the HD monolayer not only is limited to the regions exposed to VUV but also spreads under the masked regions. The strong oxidants generated by VUV irradiation to atmospheric oxygen and water vapor diffuse toward the masked regions through the nanoscopic channels and photodissociate the monolayer under the masked area, near the photomask apertures, resulting in broadening of the photopattern. Such broadening decreases with decreased vacuum pressure inside the VUV chamber, associated with a decrease of oxidant concentration and reduction of their diffusion. Gold nanoparticles (AuNPs) were immobilized on the VUV patterned features to probe the dimension of the chemically active pattern. Field emission electron microscopy reveals the construction of 565 nm wide pattern features at a vacuum pressure of 10 Pa. This pattern widens to 1,030 nm at 10 (4) Pa using the same size apertures (500 nm) as printed on the photomask. This study provides insight for fabricating submicron patterns with high reproducibility and its exploitation for different applications, which includes the patterning of nanoparticles, biopolymers, and other nano-objects at submicron dimensions.     

Synchrotron radiation circular dichroism spectroscopy of ribose and deoxyribose sugars, adenosine, AMP and dAMP nucleotides.

Synchrotron radiation circular dichroism (SRCD) spectra of ribose and deoxyribose sugars, adenosine, AMP and dAMP nucleotides and cyclic derivatives were measured in the vacuum ultraviolet region (down to 168 nm for sugars and 175 nm for adenine derivatives) and at different pH values (3, 6-7, 9-10) and temperatures (between 5 and 45 degrees C). The information content in the VUV region is important since the CD bands strongly depend on the chemical structure of the sugar, the presence and orientation of a phosphate group and the protonation state of adenine. On the other hand, single or double deprotonation of the phosphoric acid group has no influence on the spectra. We assign the vacuum ultraviolet (VUV) CD bands of the nucleoside and nucleotides to be due mainly to n-->pi* transitions in the adenine nucleobase based on a comparison with the absorption spectra. The CD bands of the sugars are due to n(O -->sigma*) transitions and are much smaller than the CD signal from the nucleotides in the VUV region. Bands are assigned to both pyranose and open-chain forms.