Open Access NANO EXPRESS

Hydrothermal Synthesis, Microstructure and Photoluminescence of Eu3+-Doped Mixed Rare Earth Nano-Orthophosphates

Bing Yan* and Xiuzhen Xiao

Author Affiliations

Department of Chemistry, Tongji University, 200092, Shanghai, China

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Nanoscale Research Letters 2010, 5:1962-1969  doi:10.1007/s11671-010-9733-8


The electronic version of this article is the complete one and can be found online at:


Received:19 April 2010
Accepted:5 August 2010
Published:18 August 2010

© 2010 The Author(s)

Abstract

Eu3+-doped mixed rare earth orthophosphates (rare earth = La, Y, Gd) have been prepared by hydrothermal technology, whose crystal phase and microstructure both vary with the molar ratio of the mixed rare earth ions. For LaxY1–xPO4: Eu3+, the ion radius distinction between the La3+ and Y3+ is so large that only La0.9Y0.1PO4: Eu3+ shows the pure monoclinic phase. For LaxGd1–xPO4: Eu3+ system, with the increase in the La content, the crystal phase structure of the product changes from the hexagonal phase to the monoclinic phase and the microstructure of them changes from the nanorods to nanowires. Similarly, YxGd1–xPO4: Eu3+, Y0.1Gd0.9PO4: Eu3+ and Y0.5Gd0.5PO4: Eu3+ samples present the pure hexagonal phase and nanorods microstructure, while Y0.9Gd0.1PO4: Eu3+ exhibits the tetragonal phase and nanocubic micromorphology. The photoluminescence behaviors of Eu3+ in these hosts are strongly related to the nature of the host (composition, crystal phase and microstructure).

Keywords:
Mixed rare earth orthophosphate; Nanophosphors; Europium ion; Hydrothermal synthesis; Microstructure; Photoluminescence

Introduction

Nanostructure materials with controlled chemical composition, crystal phase structure, morphology and particle size have been extensively investigated during the past few decades because of their high surface/volume ratio and the special quantum confinement effect [1,2]. Nanomaterials can show remarkable tunable properties and play an important role as active components in the preparation of nanoscale electronic, optical, optoelectronic, electrochemical and electromechanical devices [3-7]. Herein, the fabrication of nanomaterials with well-controlled dimensionality, morphologies, phase purity, chemical composition and desired properties remains one of the most challenging issues [8]. One simple solution to control the particle size and morphology is soft chemistry routes and in particular the hydrothermal process, which is extensively employed in the synthesis of rare earth ions activated inorganic compounds, such as yttrium vanadate, lanthanum fluoride, lanthanum phosphate and yttrium oxide [9-11].

Because of their excellent luminescent properties, rare earth orthophosphates have been extensively applied as phosphors, laser hosts, heat resistant materials and moisture sensors, whose crystal structure and synthesis technology have been studied long time ago [12,13]. For example, LaPO4: Ce, Tb phosphors have been used as green emission component of tri-chromatic luminescent lamp [14,15]. Presently, it is important to synthesize rare earth orthophosphate phosphors with regular morphology, composition and size. Ever since Meyssamy et al. has fabricated LaPO4: Eu and LaPO4: Tb nanocrystals by a simple hydrothermal method, lots of works have been focused on the study of rare earth phosphate nanocrystals [16-27]. The crystal structure of pure LnPO4 compounds can be changed with the decrease in Ln ionic radius: i.e., the orthophosphates structure from Ho to Lu as well as Y only exist in the tetragonal zircon (xenotime) structure, while the lanthanide orthophosphates structure (Ln = La~Dy) exist in the hexagonal structure under hydrothermal treatment [28]. Mixed orthophosphates composed of two rare earth elements have also been investigated, indicating that these phosphates can be used as host lattices for spectroscopic investigations [29-35].

For REPO4 phosphor of light RE3+ with larger ion radius, the monoclinic crystal phase structure is preferred. For REPO4 phosphor of middle RE3+ with intermediate radius, a partly hydrated hexagonal structure is favorable. For REPO4 phosphor of heavy RE3+ with smaller radius, a tetragonal crystal phase is adopted. Therefore, it is very interesting that what will happen when rare earth ions with different radii are introduced into one REPO4 systems with PO43−. In this text, we have investigated the crystal phase structures, microstructure (morphology and particle size) of the mixed orthophosphates REPO4 (RE = La, Gd, Y) prepared by a facile hydrothermal technology. Because of the difference in ion radii between these rare earth ions, the crystal phase and microstructure of the products show obvious differences. At the same time, Eu3+ ions have been doped in the mixed rare earth phosphates in order to examine the influence of the hosts on the luminescence of Eu3+, whose photoluminescent behaviors are studied in detail.

Experimental Section

Synthesis of the Mixed Orthophosphates

The starting materials La2O3, Y2O3, Gd2O3 and Eu2O3 are firstly dissolved into concentrated nitric acid, and the appropriate volume of deionized water was added to form the 0.2 mol l−1 RE(NO3)3 (RE = Y, La; La, Gd; Y, Gd) and 0.02 mol l−1 Eu(NO3)3, respectively. Then, the mixed orthophosphates doped with Eu3+ nanophosphors are synthesized by the hydrothermal process, which are described in the following: the different volume of Y(NO3)3, La(NO3)3 (Gd(NO3)3, La(NO3)3; Y(NO3)3, Gd(NO3)3) and Eu(NO3)3 (1:0.05 in molar ratio) solutions are mixed with appropriate amounts of NH4H2PO4 to form the emulsion. The final pH value is adjusted to 3.0 with HNO3 solution (1 M). After being stirred, the milky colloid precursor is obtained, suggesting that the nanoscale particle formation already occurred. In order to make the products to crystallize well, the milky colloid precursor is poured into closed Teflon-lined autoclaves to be treated by hydrothermal process (pressure 2.8 MPaG, 0Cr18Ni9Ti stainless steel outdoor shell, 25 mL, safe temperature 200°C, Peking University Qingniao Company, China) at 160°C for 3 days. The resulting product is filtered, washed with deionized water and absolute alcohol to remove ions possibly remaining in the final products YxLa1–xPO4: 5% Eu3+, LaxGd1-xPO4: 5% Eu3+, YxGd1–xPO4: 5% Eu3+, respectively, (x = 0.1, 0.5, 0.9) and finally dried at 60°C in air for further characterization.

Physical Characterization

The X-rays powder diffraction (XRD) patterns of all samples are performed on a Bruke/D8-Advance with CuKα radiation (λ = 1.540 Å), whose operation voltage and current are maintained at 40 kV and 40 mA, respectively. Transmission electron microscopic (TEM) images are obtained on a JEOL 2010 microscope with an accelerating voltage of 200 kV. The excitation and emission spectra are recorded with RF-5301 spectrophotometer (resolution used in the excitation and emission spectra measurement is 1 nm). All spectra are normalized to a constant intensity at the maximum. Luminescence lifetime measurements are carried out on an Edinburgh FLS920 phosphorimeter using a 450 W xenon lamp as excitation source. A Netzsch thermoanalyzer, STA 409, is used for simultaneous thermal analysis combining the thermogravimetry (TG) and differential scanning calorimetry (DSC) with a heating rate of 10°C min−1.

Results and Discussion

Crystal Phase and Microstructure of Mixed Rare Earth Phosphates

Li et al. have studied the crystal phase structure of the mixed rare earth phosphates, indicating that pure LaPO4 and YPO4 crystallize in monoclinic phase and tetragonal phase, respectively, while the mixed phosphate of La0.5Y0.5PO4 belongs to the hexagonal phase [36]. However, the crystal phase structure of the mixed orthophosphates YxLa1–xPO4 (x = 0.1, 0.5, 0.9) can be changed with different molar ratio of Y3+ to La3+, whose XRD pattern of mixed orthophosphates is shown in Fig. 1a. The change of the XRD pattern for YxLa1–xPO4 (Fig. 1a) depending on the Y:La molar ratio is well known as analyzed as typical solid solution. With the decrease in yttrium ion content, the tetragonal phase cannot be observed and the monoclinic phase appears. With La3+ to Y3+ of 9:1 M ratio, the product shows the pure monoclinic phase, just like the pure LaPO4. The final product La0.1Y0.9PO4: Eu3+ presents the mixture of hexagonal LaPO4 and tetragonal YPO4 for they cannot form the solid solution. As for LaxGd1–xPO4 (x = 0.1, 0.5, 0.9), the mixed rare earth phosphates LaxGd1–xPO4 (x = 0.1, 0.5) have the similar pure hexagonal phase, while La0.9Gd0.1PO4 belongs to the pure monoclinic phase (Fig. 1b). The XRD patterns of the mixed YxGd1–xPO4 (x = 0.1, 0.5, 0.9) are shown in Fig. 1c. The mixed rare earth phosphates YxGd1–xPO4 (x = 0.1 and 0.5) show the hexagonal phase with the different peak intensities. On the base of the literatures, the GdPO4 powders in most cases have been reported to have the pure hexagonal phase. Besides, the ion radii of Y3+ and Gd3+ are 88 pm and 93.8 pm, respectively, so the replacement of Gd3+ by Y3+ cannot have an influence on the final crystal phase structure of the product until the content of Y3+ reaches 0.9 mol. With the 1:9 M ratio of Gd3+ and Y3+, Y0.9Gd0.1PO4 present to the pure tetragonal phase. In one word, because the ion radii of Y3+, Gd3+ and La3+ are 88, 93.8 and 106.1 pm, respectively, the radii difference between rare earth ions strongly affects the crystal phase and microstructure the mixed rare earth phosphates. The difference in radius between Y3+ and La3+ is so large that it is not easy to form the product of the single phase. Additionally, the difference in radius between La3+ and Gd3+ (Gd3+ and Y3+) is smaller than that of Y3+ and La3+, so the product can present the pure phase with the different content ratio of the rare earth ions. Besides, the calculated grain sizes of these samples are in the range of 12–40 nm using Scherrer’s equation, which delegates the dimension in the normal direction of (111) plane.

thumbnailFigure 1. The XRD patterns of YxLa1−xPO4: 5 mol% Eu3+ (a), LaxGd1−xPO4: 5 mol% Eu3+ (b) and YxGd1−xPO4: 5 mol% Eu3+ (c) (x = 0.1, 0.5, 0.9)

As for the selected TG curves of the hexagonal mixed rare earth orthophosphates (Fig. 2), there exists the weight loss, which occurs in the range of 150–250°C. This indicates a rapid loss of water molecules from the crystal lattice. Thus, it further proves that the mixed rare earth orthophosphates are hexagonal phase with the hydrated powders. Besides, only a significant weight loss of 6.4 wt% occurred at 165°C and finished at 225°C, approximately corresponding to around 1 mol of H2O, whose weight loss phenomenon is similar to the report in ref. [35]. Certainly, the existence of water molecule is necessary to stabilize the hexagonal phase [25].

thumbnailFigure 2. Selected TG and DSC curves of Y0.5Gd0.5PO4: 5 mol% Eu3+

Furthermore, we also have examined the microstructure (particle size and morphology) of the mixed rare earth orthophosphates with the different molar ratio. As shown in Fig. 3, La0.1Y0.9PO4 product (Fig. 3c) is composed with the mixed morphologies of the nanoparticles and nanorods (conglomeration of nanowires), which is consistent with the coexistence of the mixed hexagonal and tetragonal phases. Rare earth orthophosphate with hexagonal phase shows a highly anisotropic structure and is favorable for the crystal growth along a certain direction and form the nanorods or nanowires, while it is contrary to the rare earth phosphate with tetragonal structure to form nanoparticles [37,38]. The actual particle size of these nanophosphors can be estimated to be around 20–80 nm from the measurement of TEM. On the other hand, YxLa1–xPO4 samples with hexagonal phase and monoclinic phase are composed of nanowires. Figure 4 shows the TEM images of the mixed orthophosphates LaxGd1–xPO4 (x = 0.1, 0.5, 0.9), which presents nanowires or nanorods. With the increase in the La3+ content, the ratio of the length to width for the particle is changed. When the molar ratio of Gd3+ is higher than 0.5, nanorods is dominated. On the contrary, the nanowires are preferred. However, it needs to be referred that the products present more uniform morphology of nanorods at the molar ratio of Gd3+: La3+ of 1:1 than at other molar ratios. The actual particle size of these nanophosphors can be estimated to be around 20–50 nm from the measurement of TEM. Figure 5 shows the microstructure of the mixed orthophosphates YxGd1–xPO4 (x = 0.1, 0.5, 0.9). Both Y0.1Gd0.9PO4 and Y0.5Gd0.5PO4 show nanorod morphology. The actual particle size of them can be estimated to be around 50–200 nm from the measurement of TEM. Generally, only tetragonal nanocube can be obtained for YPO4 under such identical conditions, which cannot be observed in the TEM images of Y0.1Gd0.9PO4 and Y0.5Gd0.5PO4 products. This is the evidence that we have synthesized YxGd1–xPO4 instead of the mixture of YPO4 and GdPO4. Besides this, tetragonal Y0.9Gd0.1PO4 presents pure nanocube particle. These phenomena are strongly related to the different ratio of the rare earth ions that have the different ion radii.

thumbnailFigure 3. The TEM pictures of Y0.1La0.9PO4: 5 mol% Eu3+ (a), Y0.5La0.5PO4: 5 mol% Eu3+ (b), and Y0.9La0.1PO4: 5 mol% Eu3+ (c)

thumbnailFigure 4. The TEM pictures of La0.1Gd0.9PO4: 5 mol% Eu3+ (a), La0.5Gd0.5PO4: 5 mol% Eu3+ (b), and La0.9Gd0.1PO4: 5 mol% Eu3+ (c)

thumbnailFigure 5. The TEM pictures of Y0.1Gd0.9PO4: 5 mol% Eu3+ (a), Y0.5Gd0.5PO4: 5 mol% Eu3+ (b), and Y0.9Gd0.1PO4: 5 mol% Eu3+ (c)

Generally speaking, the inherent crystal structure determines the crystal growth habitual behavior and final morphology. The hexagonal phase crystal of YxLa1–xPO4 commonly appears the anisotropic growth, in which exists apparent layer-like structure along C axle while not along other axles. So it prefers to grow along c axle to release more energy and form the more stable system than other two directions [18,37,38]. Finally, YxLa1–xPO4 with hexagonal phase will grow to form nanowire or nanorod along [001] direction. On the other hand, the tetragonal phase of mixed orthophosphate does not possess apparent layer-like structure and cannot show the dominated growth direction, resulting in the irregular nanoparticles. For pure monoclinic La0.1Y0.9PO4: Eu3+, crystal structure consists of isolated PO4 tetrahedron and REO9-PO4 chain parallel with c axle. So the crystal still prefers to grow along the [001] direction to make crystal system more stable in spite of that the existence of the chain is not so apparent as layer-like structure of hexagonal phase [18,37,38].

Photoluminescent Spectra of Mixed Rare Earth Phosphates

The luminescence of rare earth ions mainly originates from the electron transitions within the 4f shell. However, trivalent Y, La and Lu ions have the empty or completely filled 4f shells, which cannot produce the f–f transitions. Similarly, trivalent Gd3+ has a half-filled 4f shell, and the transition energy for f–f transitions of Gd3+ is much higher than for other Ln3+ with partially filled 4f shells, which is not easy to emit the luminescence too [36]. As a result, the phosphates of these ions are used as host lattice for Eu3+. Herein, we have synthesized the Eu3+ activated mixed rare earth phosphates and investigated the luminescence of Eu3+ in these hosts. Both excitation and emission spectra of LaxGd1–xPO4 (x = 0.1, 0.5, 0.9) are shown in Fig. 6. The excitation spectra consist of a broad band in the short wavelength region and several sharp lines in the long wavelength region. The broad band can be ascribed to the oxygen-to-europium charge transfer band (CTB), whereas the sharp lines correspond to direct excitation of the ground state into higher excited states of the 4f electrons for Eu3+. The position of the CTB of Eu3+ in the lattice of hexagonal phosphates shifts slightly toward shorter wavelength compared with that in monoclinic La0.9Gd0.1PO4: Eu3+ ((CTB = 268 nm), being centered at 255 nm for La01Gd0.9PO4: Eu3+ and 263 nm for La0.5Gd0.5PO4: Eu3+. This result can be explained by the differences in the Eu–O bond lengths. In the monoclinic rare earth phosphate, RE3+ ion is nine-coordinated, while in the hexagonal rare earth phosphate, it is eight-coordinated. This indicates that the average RE–O bond lengths in La0.1Gd0.9PO4: Eu3+ and La0.5Gd0.5PO4: Eu3+ are shorter than that in monoclinic La0.9Gd0.1PO4: Eu3+. Furthermore, it is observed a new absorption band for La0.1Gd0.9PO4: Eu3+, which peaks at 273 nm. This band is attributed to the 8S7/26IJ transitions within Gd3+ ions, indicating the occurrence of the energy transfer process from gadolinium ions to europium ones. The emission spectra of LaxGd1−XPO4: Eu3+ (x = 0.1, 0.5, 0.9) under 393 nm excitation are composed of the characteristic emission lines of Eu3+: 5D07F15D07F25D07F3 and 5D07F4, respectively. The transitions are found to be split into components depending upon the host matrix composition. These phosphors exhibit orange-red color due to the emission transitions 5D07F1 (magnetic dipole line) and 5D07F2 (electric dipole line), respectively. Furthermore, the intensity of the transition 5D07F1 is stronger than that of the transition 5D07F2. As is well known, the relative intensities of 5D07F1 and 5D07F2 emission, which are typical magnetic and electronic dipole–dipole transitions, respectively, depend strongly on the local symmetry of the Eu3+[35-37]. In a site with inversion symmetry, the 5D07F1 magnetic dipole transition is dominating, while in a site without inversion symmetry the 5D07F2 electric dipole transition is the strongest. The results already indicate that more Eu3+ occupied the position with the inversion symmetry in host lattices. At the same time, we have found that the intensity of the Eu3+ emissions in La0.5Gd0.5PO4 is stronger than that of the other two samples. This can be attributed to the morphology of the La0.5Gd0.5PO4, which presents more uniformity nanorods among these three samples.

thumbnailFigure 6. The excitation (a) and emission (b) spectra of LaxGd1−xPO4: 5 mol% Eu3+ (x = 0.1, 0.5, 0.9)

For the mixed rare earth phosphate YxGd1–xPO4: Eu3+ (x = 0.1, 0.5, 0.9), both excitation and emission spectra are shown in Fig. 7, which have the similar features to the above. It can be observed the CTB band of O2− to Eu3+ (belonging to PO43−, here “2−” is only the formatted charge of O in PO42−), peaking at 253 nm and a sharp absorption band from 8S7/26IJ transitions for Gd3+, revealing the existence of the energy transfer process between Gd3+ and Eu3+. The characteristic emissions of Gd3+ are situated at the strong excitation band of YxGd1–xPO4, suggesting that there exists the energy transfer of Gd3+→PO43− → Eu3+, at the same time, the energy level difference in 6GJ and 6PJ of Gd3+ is close to that of 7F1 and 5D0 of Eu3+, a Gd3+ in 6GJ state can excite Eu3+ into 5D0 state by resonance energy transfer, which results in the energy transfer of Gd3+ to Eu3+[39]. Besides this, several strong absorption bands have been observed in the long region of 300–500 nm, which originate from the Eu3+ff transitions. Figure 6B shows the emission spectra of the YxGd1–xPO4: Eu3+ with the different content ratio of Y3+ to Gd3+ ions. The characteristic emission can be seen obviously (5D07FJ) originating from low energy transfer of Eu3+. Among these emission lines, 5D07F1 transition is dominant. This indicates that in these hosts, more Eu3+ sites are in inversion symmetry. With the content of Gd increases, the intensity of 5D07F1 emission increases. Obviously, Gd3+ plays an intermediate role in the energy transfer from PO43− to the activator. The energy transfer process in YxGd1–xPO4: Eu3+ may be described as follows [40]: energy is first absorbed by host absorption band, then is trapped by Gd3+ ions and migrated along them until it is trapped by the activator, resulting in the characteristic luminescence. Certainly, Eu3+ also can obtain energy from host band directly. Besides, it can be seen the luminescent intensity of Y0.9Gd0.1PO4: Eu3+ is weaker than those of other composition, suggesting that the tetragonal phase of Y0.9Gd0.1PO4: Eu3+ is not so favorable as the hexagonal phase of Y0.9Gd0.1PO4: Eu3+ and Y0.9Gd0.1PO4: Eu3+ and the influence of crystal phase on the luminescence is higher than that of water molecules. In addition, either hexagonal phase or tetragonal one cannot show apparent difference in the luminescent intensity of magnetic dipolar transition (5D07F1) and electronic dipolar transition (5D07F2).

thumbnailFigure 7. The excitation (a) and emission (b) spectra of YxGd1−xPO4: 5 mol% Eu3+ (x = 0.1, 0.5, 0.9)

The photoluminescence spectrum of Eu3+ in monoclinic phase La0.9Y0.1PO4 has also been investigated, which is shown in Fig. 8. There are no apparent excitation bands in long wavelength of 300–400 nm and the effective energy absorption takes place in the shorter wavelength of 200–280 nm, peaking at 270 nm. This broad band is ascribed to the CTB band of O2− (belonging to PO43−, here “2−” is only the formatted charge of O in PO42−) to Eu3+. At the same time, under 270 nm excitation, the emission originates mainly from those crystallographic Eu3+ sites due to the local energy transfer from Eu–O charge transfer state to the adjacent Eu3+ ions. The emission spectra are composed with the characteristic Eu3+ emission lines. Different from the luminescent spectra of YxGd1–xPO4: Eu3+ and LaxGd1–xPO4: Eu3+, the emission intensity of 5D07F2 transition for Eu3+ in La0.9Y0.1PO4 is stronger than that of 5D07F1. This result shows that more Eu3+ in the monoclinic La0.9Y0.1PO4 occupied the site with less inversion symmetry. When the Eu3+ is located at a low-symmetry local site lack of inversion center, the emission at transition is dominated in the emission spectra [41-43]. The resulting lifetime data of the selected Eu-activated rare earth orthophosphates (LaxGd1–xPO4, YxGd1–xPO4) are given in Table 1. It can be observed that the composition of hosts with different molar ratio of rare earth ions have great influence on the luminescent lifetimes of excited state of europium ions. Besides, there exists different order between LaxGd1–xPO4: Eu3+ and YxGd1–xPO4: Eu3+. For LaxGd1–xPO4: Eu3+, the luminescent lifetime reaches the longest (3.43 ms) at the x = 0.5, which is much longer than the other two compositions (x = 0.1 or 0.9), suggesting there exist a suitable molar ratio of La3+ to Gd3+ (1:1) for the luminescence of Eu3+. While it is different for YxGd1–xPO4: Eu3+, whose lifetime decreases dramatically with the increase in the molar ratio of Y, revealing the introduction of Y ion is not suitable for the luminescence of Eu3+.

thumbnailFigure 8. The excitation (a) and emission (b) spectra of Y0.1La0.9PO4: 5 mol% Eu3+

Table 1. Photoluminescence lifetimes for LaxGd1–xPO4 Eu3+ and YxGd1–xPO4: Eu3+ Nanophosphors

Conclusions

In summary, the Eu3+ activated rare earth phosphate (YxGd1–xPO4, LaxGd1–xPO4 and YxLa1–xPO4) nanophosphors (x = 0.1, 0.5, 0.9) have been synthesized by hydrothermal technology. The crystal phase and microstructure of the products are strongly depended on the difference in the ion radii of rare earth elements. For Y3+ and La3+ ions, the difference in the radii is so large that YxLa1–xPO4 cannot be favorable for the formation of the pure phase except that Y0.1La0.9PO4 powders present the pure monoclinic phase and nanowires. As for YxGd1–xPO4 and LaxGd1–xPO4, the radii difference between two rare earth ions cannot make a big influence on the crystal structure and the morphology. With the increase in the Y content in YxGd1–xPO4, the structure of the product has been changed from the hexagonal phase to the tetragonal phase and the morphology from nanorods to nanowires. Similarly, LaxGd1–xPO4 (x = 0.1, 0.5) powders have the hexagonal phase and La0.9Gd0.1PO4 belongs to the monoclinic phase. With the increase in the La3+ content, the ratio of the length to width has been changed. Y0.1Gd0.9PO4: Eu3+ and La0.5Gd0.5PO4: Eu3+ nanophosphors present the longest lifetime in the corresponding series. These lanthanide phosphates can be expected to have some potential applications in such fields as fluorescent lamps, plasma display panels and luminescent probes or labels for biomolecule system.

Acknowledgments

The work is supported by the Science Fund of Shanghai University for Excellent Youth Scientists and National Natural Science Foundation of China (20971100).

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References

  1. Hu JT, Odom TW, Lieber CM:

    Acc. Chem. Res.. 1999, 32:435.

    COI number [1:CAS:528:DyaK1MXht1ShurY%3D]

    Publisher Full Text OpenURL

  2. Kovtyukhova NI, Mallouk TE:

    Chem. Eur. J.. 2002, 8:4355. Publisher Full Text OpenURL

  3. Huang Y, Duan XF, Wei QQ, Lieber CM:

    Science. 2001, 291:630.

    COI number [1:CAS:528:DC%2BD3MXntlWlsw%3D%3D]; Bibcode number [2001Sci...291..630H]

    PubMed Abstract | Publisher Full Text OpenURL

  4. Huang MH, Mao S, Feick H, Yan H, Wu Y, Kind H, Weber E, Russo R, Yang PD:

    Science. 2001, 292:1897.

    COI number [1:CAS:528:DC%2BD3MXksVaqsb0%3D]; Bibcode number [2001Sci...292.1897H]

    PubMed Abstract | Publisher Full Text OpenURL

  5. Wang ZL:

    Adv. Mater.. 2000, 12:1295.

    COI number [1:CAS:528:DC%2BD3cXnt1Wksr8%3D]

    Publisher Full Text OpenURL

  6. Dekker C:

    Phys. Today. 1999, 52:22.

    COI number [1:CAS:528:DyaK1MXjsVGntL4%3D]; Bibcode number [1999PhT....52E..22D]

    Publisher Full Text OpenURL

  7. Frank S, Poncharal P, Wang ZL, de Heer WA:

    Science. 1998, 280:1744.

    COI number [1:CAS:528:DyaK1cXjslOhu7g%3D]; Bibcode number [1998Sci...280.1744F]

    PubMed Abstract | Publisher Full Text OpenURL

  8. Xia YN, Yang PD:

    Adv. Mater.. 2003, 15:351.

    COI number [1:CAS:528:DC%2BD3sXisFemtr0%3D]

    Publisher Full Text OpenURL

  9. Huignard A, Gacoin T, Boilot JP:

    Chem. Mater.. 2000, 12:1090.

    COI number [1:CAS:528:DC%2BD3cXhvFymsrw%3D]

    Publisher Full Text OpenURL

  10. Huignard A, Buissette V, Franville AC, Gacoin T, Boilot JP:

    J. Phys. Chem. B. 2003, 107:6754.

    COI number [1:CAS:528:DC%2BD3sXks1SqsLc%3D]

    Publisher Full Text OpenURL

  11. Riwotzki K, Haase M:

    J. Phys. Chem. B. 1998, 102:10129.

    COI number [1:CAS:528:DyaK1cXnt12itL0%3D]

    Publisher Full Text OpenURL

  12. Mooney RCL:

    J. Chem. Phys.. 1948, 16:1003.

    COI number [1:CAS:528:DyaH1MXhtV0%3D]; Bibcode number [1948JChPh..16.1003M]

    Publisher Full Text OpenURL

  13. Mooney RCL:

    Acta Crystallogr.. 1950, 3:337.

    COI number [1:CAS:528:DyaG3cXlsV2mug%3D%3D]

    Publisher Full Text OpenURL

  14. Dexpert – Ghys J, Mauricot R, Faucher MD:

    J. Lumin.. 1996, 69:203. Publisher Full Text OpenURL

  15. Aia MA:

    J. Electrochem. Soc.. 1967, 114:367.

    COI number [1:CAS:528:DyaF2sXpvF2msw%3D%3D]

    Publisher Full Text OpenURL

  16. Meyssamy H, Riwotzki K, Kornowski A, Naused S, Haase M:

    Adv. Mater.. 1999, 11:840.

    COI number [1:CAS:528:DyaK1MXkvFOisbo%3D]

    Publisher Full Text OpenURL

  17. Shi HT, Qi LM, Ma JM, Cheng HM:

    Chem. Commun. 2002., 1704 OpenURL

  18. Fang YP, Xu AW, Song RQ, Zhang HX, You LP, Yu J, Liu HQ:

    J. Am. Chem. Soc.. 2003, 125:16025.

    COI number [1:CAS:528:DC%2BD3sXptlOgtbc%3D]

    PubMed Abstract | Publisher Full Text OpenURL

  19. Bu WB, Hua ZL, Chen HR, Zhang LX, Shi JL:

    Chem. Lett.. 2004, 33:612.

    COI number [1:CAS:528:DC%2BD2cXktFelt7o%3D]

    Publisher Full Text OpenURL

  20. Yan ZG, Zhang YW, You LP, Si R, Yan CH:

    J. Cryst. Growth. 2004, 262:408.

    COI number [1:CAS:528:DC%2BD2cXhtVKmtLg%3D]; Bibcode number [2004JCrGr.262..408Y]

    Publisher Full Text OpenURL

  21. Tang CC, Bando Y, Golberg D, Ma RZ:

    Angew. Chem. Int. Ed.. 2005, 52:576.

    COI number [1:CAS:528:DC%2BD2MXosFCgsw%3D%3D]

    Publisher Full Text OpenURL

  22. Cao MH, Hu CW, Wu QY, Guo CX, Qi YJ, Wang EB:

    Nanotechnology. 2005, 16:282.

    COI number [1:CAS:528:DC%2BD2MXislClu7Y%3D]; Bibcode number [2005Nanot..16..282C]

    Publisher Full Text OpenURL

  23. Ito H, Fujishiro Y, Sato T, Okuwaki A:

    Ber. Ceram. Trans.. 1995, 94:146.

    COI number [1:CAS:528:DyaK2MXptVOjurY%3D]

    OpenURL

  24. Kijkowska R, LeGeros RZ:

    Key Eng. Mater.. 2005, 284–286:79. Publisher Full Text OpenURL

  25. Zollfrank C, Scheel H, Brungs S, Greil PJ:

    Cryst. Growth Des.. 2008, 8:766.

    COI number [1:CAS:528:DC%2BD1cXhtFOnu7k%3D]

    Publisher Full Text OpenURL

  26. Peng ZA, Peng XG:

    J. Am. Chem. Soc.. 2001, 123:1389.

    COI number [1:CAS:528:DC%2BD3MXmslSgtA%3D%3D]

    Publisher Full Text OpenURL

  27. Peng ZA, Peng XG:

    J. Am. Chem. Soc.. 2002, 124:3343.

    COI number [1:CAS:528:DC%2BD38Xhslegtro%3D]

    PubMed Abstract | Publisher Full Text OpenURL

  28. Zhang YW, Yan ZG, You LP, Si R, Yan CH:

    Eur. J. Inorg. Chem. 2003., 4099 OpenURL

  29. Riwotzki K, Meyssamy H, Schnablegger H, Kornowski A, Haase M:

    Angew. Chem. Int. Ed.. 2001, 40:573.

    COI number [1:CAS:528:DC%2BD3MXhsVSqsrg%3D]

    Publisher Full Text OpenURL

  30. Riwotzki K, Meyssamy H, Kornowski A, Haase M:

    J. Phys. Chem. B. 2000, 104:2824.

    COI number [1:CAS:528:DC%2BD3cXhsFyhtLY%3D]

    Publisher Full Text OpenURL

  31. Nishihama S, Hirai T, Komasawa I:

    J. Mater. Chem.. 2002, 12:1053.

    COI number [1:CAS:528:DC%2BD38Xit1Kntbw%3D]

    Publisher Full Text OpenURL

  32. Schuetz P, Caruso F:

    Chem. Mater.. 2002, 14:4509.

    COI number [1:CAS:528:DC%2BD38XoslSisrY%3D]

    Publisher Full Text OpenURL

  33. Mullica DF, Sappenfield EL, Boatner LA:

    Inorg. Chim. Acta. 1996, 244:247.

    COI number [1:CAS:528:DyaK28XitFChsLo%3D]

    Publisher Full Text OpenURL

  34. Ito H, Fujishiro Y, Sato T, Okuwaki A:

    Br. Ceram. Trans.. 1995, 94:146.

    COI number [1:CAS:528:DyaK2MXptVOjurY%3D]

    OpenURL

  35. Yan RX, Sun XM, Wang X, Peng Q, Li YD:

    Chem. Eur. J.. 2005, 11:2183.

    COI number [1:CAS:528:DC%2BD2MXislOgurs%3D]

    Publisher Full Text OpenURL

  36. Wickleder MS:

    Chem. Rev.. 2002, 102:2011.

    COI number [1:CAS:528:DC%2BD38Xktl2gs70%3D]

    PubMed Abstract | Publisher Full Text OpenURL

  37. Milligan WO, Mullika DF, Beall GW, Boatner LA:

    Acta Crystallogr.. 1983, C39:23.

    COI number [1:CAS:528:DyaL3sXotFygsA%3D%3D]

    OpenURL

  38. Milligan WO, Mullica DF, Beall GW, Boatner LA:

    Inorg. Chim. Acta. 1982, 60:39.

    COI number [1:CAS:528:DyaL38XksVOlu70%3D]

    Publisher Full Text OpenURL

  39. Rambabu U, Buddhudu S:

    Opt. Mater.. 2001, 17:401.

    COI number [1:CAS:528:DC%2BD3MXkvVGhsLo%3D]; Bibcode number [2001OptMa..17..401R]

    Publisher Full Text OpenURL

  40. Wu XY, You HP, Cui HT, Zeng XQ, Hong GY, Kim CH, Pyun CH, Yu BY, Park CH:

    Mater. Res. Bull.. 2002, 37:1531.

    COI number [1:CAS:528:DC%2BD38Xls1Wiurs%3D]

    Publisher Full Text OpenURL

  41. Wang ZL, Liang HB, Gong ML, Su Q:

    Opt. Mater.. 2007, 29:896.

    COI number [1:CAS:528:DC%2BD2sXntV2ntA%3D%3D]; Bibcode number [2007OptMa..29..896W]

    Publisher Full Text OpenURL

  42. Wang JG, Jing XP, Yan CH, Lin JH, Liao FH:

    J. Lumin.. 2006, 121:57.

    COI number [1:CAS:528:DC%2BD28XkvVartr4%3D]

    Publisher Full Text OpenURL

  43. Yu M, Lin J, Wang Z, Fu J, Wang S, Zhang HJ, Han YC:

    Chem. Mater.. 2002, 14:2228. OpenURL