75 resultados para VUV
Resumo:
采用高温固相反应合成了稀土离子激活的碱土硼磷酸盐MBPO_5:RE(M=Ca, Sr, Ba;RE=Sm, Eu, Tb, Dy), Ba_3BPO_7:RE和Ba_3BP_O_(12):RE、稀土硼磷酸盐Ln_7BP_2P_(17):RE (Ln=La, Gd)、碱土(稀土)磷酸盐M_3(PO_4)_2:RE (M=Sr, Ba),ABLa(PP_4)_2:Ce,Tb (A=K, Na;B=Mg, Zn)、碱土(稀土)硼酸盐SrB_4O_7:RE(Re=Sm, Eu),BaB_8O_(13):Eu,SrB_6O_(10):Sm, M_3Gd_2(BO_3)_4:RE (M=Ca, Sr),B_3O6:Eu(RE=La, Gd)和稀土硼钨酸盐Cd_3BWO_9:Eu。通过XRD、IR光谱和Raman光谱等表征了其结构。测定了上述19个基质的数十个发光体的UV佩VUV光谱和RE-L_3(RE=Sm,Eu, Gd)边的XANES和EXAFS。碱土硼磷酸盐Ba_3BPO_7和Ba_3BP_3O_(12)、稀土硼磷酸盐Ln_7BP_2O_(17) (Ln=La, Gd)和稀土钨硼酸盐Gd3Bwo9等6个基质中稀土离子的UV-VUV光谱和除个别基质(REB_3O_6等)外的VUV光谱均属首次报道。发现土稀土离子激活的这些发光体在VUV范围有丰富的基质吸收带。认为基质中阴离子的结构和基质的晶体结构可能是影响基质的吸收带位置的重要因素。通过XANEs和UV-VUV光谱的联系,结合经验公式首次确证了一些复合氧化物基质中一些RE~(3+)在vuv范围的f-d跃迁位置。根据VUV光谱测定结果推测了一些基质中RE~(3+)的CTB位置。首次应用RE-L_3边的XANES和UV-VUV光谱两种方法分析比较了RE~(3+)(RE=Eu, Sm)离子在空气条件下在碱土硼磷酸盐、硼酸盐和磷酸盐基质中的还原。首次应用高分辨发射光谱和RE-L_3边的EXAFS研究了在一些基质中发光中心的配位数、键长和格位对称性等结构因素。
Resumo:
PDP(等离子平板显示器)是一种最有前途的大屏幕壁挂式彩电,而它需要VUV激发下的高效荧光粉,同时由于VUV荧光粉也是无汞荧光灯的需求,所以研究VUV激发的稀土激活的荧光粉是实际应用的需要.对于光谱分析该工作采用了理论计算与光谱数据分析相结合的方法,对所测光谱各个谱峰进行了详细的指认.得到了以下的结论和成果:1.得到了大量的含氧酸盐中稀土离子的VUV光谱数据.2.首次系统地应用两种方法预测了三价稀土离子的f-d跃迁位置,并首次系统地通过计算预测了三价稀土离子在含氧酸盐中的电荷迁移带的位置.3.首次实验观察到Ce<'3+>的电荷迁移带,观察到了Tb<'3+>的电荷迁移带.4.在所有含Dy<'3+>的样品中都观察到Dy<'3+>的f-d跃迁.5.LaPO<,4>和ABLa(PO<,4>)<,2>(A=K,Na;B=Mg,Zn)基质中,观察到了Ce<'3+>的5个f-d跃迁,指认了Tb<'3+>的5个f-d跃迁,指认了掺杂Ce、Tb的VUV光谱中的所有谱峰.6.对所研究基质中的稀土离子的f-d跃迁和电荷迁移带进行了系统地预测和指认.7.通过总结不同稀土离子在相同基质中的VUV光谱,并参考文献的相关报导,总结了所研究基质的基质吸收位置.8.通过Eu<'3+>的灾光探针作用和ce<'3+>的发射光谱等,确证三价稀土离子在La<,2>CaB<,10>O<,19>基质中同时取代了八配位的Ca<'2+>和十配位的La<'3+>,占据了两种格位.9.合成了一种新型绿色长余辉材料,具有亮度高,余辉时间长,可用日光激发等优点.10.合成了一种UV激发下性能优异的掺Eu<'3+>的红色荧光粉,亮度可以跟商业红粉Y<,2>O<,3>:Eu相比拟,而基质材料与Y<,2>O<,3>相比降低了成本.
Resumo:
RE3+-activated alpha- and beta-CaAl2B2O7 (RE = Tb, Ce) were synthesized with the method of high-temperature solid-state reaction. Their VUV excitation and VUV-excited emission spectra are measured and discussed in the present article. The charge transfer band of Tb3+ and Ce3+ is respectively calculated to be at 151 +/- 2 and 159 +/- 3 nm. All the samples show an activator-independent excitation peak at about 175 nm and an emission peak at 350-360 nm ascribed to the host absorption and emission band, respectively.
Resumo:
Phosphors CaYBO4:RE3+ (RE = Eu, Gd, Tb, Ce) were synthesized with the method of solid-state reaction at high temperature, and their vacuum ultraviolet (VUV)-visible luminescent properties in VUV-visible region were studied at 20 K. In CaYBO4, it is confirmed that there are two types of lattice sites that can be substituted by rare-earth ions. The host excitation and emission peaks of undoped CaYBO4 are very weak, which locate at about 175 and 350-360nm, respectively. The existence of Gd3+ can efficiently enhance the utilization of host absorption energy and result in a strong emission line at 314 nm. In CaYBO4, Eu3+ has typical red emission with the strongest peak at 610 nm; Tb3+ shows characteristic green emission, of which the maximum emission peak is located at 542 nm. The charge transfer band of CaYBO4:Eu3+ was observed at 228 nm; the co-doping of Gd3+ and Eu3+ can obviously sensitize the red emission of Eu3+. The fluorescent spectra of CaYBO4:Ce3+ is very weak due to photoionization; the co-addition of Ce3+-Tb3+ can obviously quench the luminescence of Tb3+.
Resumo:
The optical properties of rare earth ions-activated barium orthophosphate phosphors, Ba-3(PO4)(2):RE (RE = Ce3+, Sm3+, Eu3+, Eu2+, and Tb3+), were investigated in vacuum ultraviolet (VLTV)-Vis range. A band-band transition Of PO43- in Ba-3(PO4)(2) is observed in the region of 150-170 nm. The partial reduction of Eu3+ to Eu2+ was observed and confirmed by luminescent spectra under the VUV-UV excitation. It is proposed that the electronegative defects that formed by aliovalent substitution of Eu3+ on the Ba2+ site in the host are responsible for the reduction process.
Resumo:
The VUV-UV spectra of rare earth ions activated calcium borophosphate, CaBPO5:RE (RE = Ce3+, sm(3+), Eu2+, Eu3+, Tb3+ and Dy3+) were determined. The bands at about 155 nm in the VUV excitation spectra are attributed to the host lattice absorptions. The bands at 166 and 190 nm for the sample CaBPO5:Sm have been considered as related to the f-d transition and the charge transfer band (CTB) of Sm3+ ions, and the band at 169 nm for the sample CaBPO5:Dy is assumed to be connected with the f-d transition of the Dy3+ ions in CaBPO5. The partial reduction of Eu3+ CaBPO5:Eu prepared by high temperature solid state reaction in air is confirmed by the VUV-UV spectra.
Resumo:
The high-resolution luminescent spectrum of divalent samarium excited by 355 nm UV light at 77 K, the VUV excitation spectra, the VUV excited emission spectra and EXAFS at Sm-L-3 edge were reported for samarium doped strontium borophosphate, SrBPO5:Sm prepared by solid state reaction in air at high temperature. The high-resolution luminescent spectrum showed that the divalent samarium ions occupied the C-2upsilon lattice sites. The VUV excitation spectra indicated that the sample exhibited absorption bands with the maxima at 129 and 148 nm, respectively. The performance of EXAFS at Sm-L3 absorption edge suggested that the samarium ions were nine-coordinated and the mean distances of bond Sm-O were 2.38 Angstrom.
Resumo:
The measurements of VUV-UV photoluminescence emission (PL) and photoluminescence excitation (PLE) spectra of rare earth ions activated strontium orthophosphate [Sr-3(PO4)(2):RE, RE = Ce, Sm, Eu, Tb] are performed. Whenever the samples are excited by VUV or UV light, the typical emission of Ce-3+,Ce- Sm3+, Eu3+, Eu2+ and Tb3+ ions can be observed in PL spectra, respectively. The charge transfer bands (CTBs) of Sm3+ and Eu3+ are found, respectively, peaking at 206 and 230nm. The absorption bands peaking in the region of 150-160 nm are assigned to the host lattice sensitization bands, i.e., the band-to-band transitions of PO43- grouping in Sr-3(PO4)(2). It is speculated that the first f-d transitions of Sm3+ (Eu3+), and the CTB of Tb3+ are, respectively, located around 165 (14 3) and 167 urn by means of VUV-UV PLE spectra and relational empirical formula, these f-d transitions or CT bands are included in the bands with the maxima at 150-160 nm, respectively. The valence change of europium from trivalent to divalent in strontium orthophosphate prepared in air is observe by VUV-UV PL and PLE spectra.
Resumo:
VUV-UV and Eu-L-3 edge XANES spectra were measured for europium-doped strontium tetraborate prepared by solid state reaction at high temperature in air. The VUV-UV spectra show that the host absorption band of (SrBO7)-O-4 appears below 170 nm. The charge transfer band of Eu3+ doped in SrB4O7 is peaked at 272 nm. The 4f-5d transitions of Eu2+ consist of a band peaked at 310 nm with a shoulder at 280 nm and also include the bands peaked at 238 (weak) and 203 (strong) nm. The result of XANES spectrum at Eu-L3 edge of the synthesized sample indicates that Eu3+ and Eu2+ coexist in SrB4O7:Eu prepared in air, which is consistent with the results of the VUV-UV spectra.
Resumo:
The local structure and the valences of europium in SrBPO5:Eu prepared in air were checked by means of XAFS at Eu-L-3 edge. From the EXAFS results, it was discovered that the doped europium atoms were nine-coordinated by oxygen atoms and the distances of bond Eu-O were 2.42 Angstrom in the host. From the XANES data, it was found that the divalent and trivalent europium coexisted in the matrix. The emission spectra excited by VUV or UV exhibited a prominent broad band due to the 4f(6)5d-4f(7) transition of Eu2+ ions, which indicated that the trivalent europium ions were reduced in air in the matrix at high temperature by the defects [V-Sr]" formed by aliovalent substitution between Sr2+ and Eu3+ ions. The VUV excitation spectra in 100-200 nm range showed that the matrix had absorption bands with the maxima at about 130 and 150 nm, respectively.
Resumo:
XAFS (EXAFS and XANES) at Eu-L-3 edge were used to determine the local structure and the valences of europium in CaBPO5:Eu prepared in air. The results of EXAFS showed that the doped europium atoms were nine-coordinated by oxygen atoms and the distances of bond Eu-O were 2.39 Angstrom in the host lattice. XANES at Eu-L-3 edge exhibited that Eu2+ and Eu3+ coexisted in the matrix. The luminescent spectrum of the material excited by VUV at 147 nm presented a similar spectrum with that excited by f-f transition of Eu2+ at 396 nm and f-d transition of Eu2+ at 312 nm. The broad emission band due to both 4f(6)5d - 4f(7) transition of EU2+ and f - f transition of Eu3+ could be observed in emission spectra, which indicated that the trivalent europium ions were reduced in air in the matrix at high temperature by the defects [V-Cn]" formed by aliovalent substitution between Ca2+ and Eu3+ ions. The UV excitation spectrum showed the typical f-f transition of Eu3+ and f-d transition of Eu2+. The bands with the maxima at about 113 and 158 nm in VUV excitation spectrum were assigned to originate from the absorption of the host lattice.
Resumo:
研究了La2CaB10O19∶Eu3+红色发光材料的高分辨发射光谱和UV VUV激发光谱。根据发射光谱和荧光寿命,认为进入晶格的Eu3+占据了两种格位,一种Eu3+占据了与O2-离子十配位的La3+的格位,另一种Eu3+则占据了与O2-离子八配位的Ca2+的格位。又从激发光谱的分析中,得到Eu3+的电荷迁移带(CTB)是峰值位于244nm的宽带,而位于130~170nm之间的成份复杂的宽带包括硼酸盐基质的吸收带和Eu3+的f d跃迁的结论。
Resumo:
The (Y, Gd) BO3 : Eu phosphor was synthesized by solid-state reaction, The UV spectra showed that in a certain range of Gd3+ concentration, more Gd3+ absorbed energy and transferred it to Eu3+ with its increasing concentration. From the spectra in VUV region, it was observed that both the doping and the concentrations of Gd3+, Eu3+ greatly affected the absorption of the host lattice. The absorbances at 147 nm and 170 nm increased when the Gd3+ was doped which can be explained as that Gd3+ transferred energy to BO4. The optical properties of (Y, Gd)BO3 : Eu were the best when the concentration of Eu3+ was about 0.04.
Resumo:
Vacuum ultraviolet excitation spectra of LnAl(3)B(4)O(12):Re (Ln = Y, Gd; Re = Eu, To), along with X-ray photoelectron spectra, were measured. The spectra are tentatively interpreted in terms of the optical properties of the rare earth ions and the band structure. It was found that there is an energy transfer from the hosts to the rare earth ions. It was also found that the top of the valence band in the Gd compound is mainly formed by the 2p levels of O2- and the 4f levels of Gd3+, and in the Y compound mainly by the 2p levels of O2-. (C) 2000 Elsevier Science Ltd. All rights reserved.