Reports: B6

43862-B6 Synthesis, Photoluminescence, and Laser Characteristics of Rare Earth Ions Embedded in HEMA, a Polymeric Plastic Host

Dhiraj K. Sardar, University of Texas (San Antonio)

In this project, our specific goal was to synthesize, fabricate, and investigate the spectroscopic and laser properties of various trivalent rare earth-based nanoparticles embedded in polymeric plastic host 2-hydroxyethyl methacrylate (known as HEMA).

Nd3+:Y2O3 nanoparticles embedded in poly-hydroxyethyl methacrylate, often referred to as p-HEMA, was obtained. Aggregation of nanoparticles in the HEMA matrix was prevented through sonication of the HEMA-nanoparticle solution for an adequate amount of time prior to the polymerization process. Polymerization occurs before the nanoparticles have time to fall out of the solution, thereby forming a uniform distribution of nanoparticles in the polymer matrix. The Judd-Ofelt theoretical model was applied to the room temperature absorption intensities of rare earth ions such as Nd3+­(4f 3) in HEMA, to determine the three phenomenological intensity parameters: W2, W4, and W6. Values are used to determine the spectroscopic quality factor for Er3+ in HEMA and are compared to those for Nd3+ ions in crystalline hosts. The intensity parameters are subsequently used to determine the spectroscopic quality factor, radiative decay rates, branching ratios and radiative lifetimes from the upper multiplet manifolds to the corresponding lower-lying multiplet manifolds 2S+1LJ of Er3+­(4f11) in HEMA. Radiative lifetimes of the excited states were calculated and found to be on the same order of magnitude of those obtained for the Nd3+:Y2O3 ceramic. However, measured lifetimes were found to be longer due to re-absorption mechanisms of the Nd3+ ions on the surface of the particles and potential energy transfer processes between the polymer and the nanoparticles. Our results indicate that the system is capable of storing energy which can lead to low power diode and waveguide applications.

In addition, optical absorption and emission intensities are investigated for Ho3+ in nanocrystalline Ho3+:Y2O3. Room temperature absorption intensities of Ho3+(4f10) transitions in synthesized Ho3+:Y2O3 nanocrystals have been analyzed using the Judd-Ofelt (J-O) approach  in order to obtain the phenomenological intensity parameters. The J-O intensity parameters are used to calculate the spontaneous emission probabilities, radiative lifetimes, and branching ratios of the Ho3+­ transitions from the upper multiplet manifolds to the corresponding lower-lying multiplet manifolds 2S+1LJ of Ho3+­(4f10).  The emission cross section of the important intermanifold  5I7 ® 5I8 (2.0 µm) transition has been determined.  The room temperature fluorescence lifetime of this transition in Ho3+:Y2O3 nanocrystals was measured. From the radiative lifetime determined from the J-O model and measured fluorescence lifetime, the quantum efficiency of this material was determined. The comparative study of Ho3+­(4f10) ions suggests that synthesized Ho3+:Y2O3 nanocrystals could be an excellent alternative to single-crystal Ho3+:Y2O3 for certain applications especially in the near infrared region

We have also synthesized and characterized trivalent erbium-doped yttrium-oxide, Er3+:Y23 nanocrystals. These particles were synthesized by the precipitation from a homogeneous solution. The SEM picture shows the particle size is approximately 200 nm. The room temperature optical absorption and emission spectra show that the trivalent erbium ions in Er3+:Y23 nanocrystals possess sharp absorption lines and strong emission in near infrared region that are characteristic of Er3+:Y23 grown as large single crystals. Also, a detailed spectroscopic analysis of the aggregates indicates that the material has optical properties similar to those reported for single crystals grown by a flame fusion method. Photostability is maintained in the nanocrystalline aggregates. The ability of these aggregates to attach to different surfaces by either chemical or physical means renders them useful in numerous technologies.

The support from the Petroleum Research Fund (PRF # 43862-B6) has been acknowledged in all papers and presentations.