Spectroscopic Analysis of Tb 3+ Doped Sol-Gels In recent years, there has been much research in the field of rare-earth (RE) dope sol-gel glasses. These.

Slides:



Advertisements
Similar presentations
Excited Elements.
Advertisements

EMISSION AND ABSORPTION SPECTRA. Spectra A spectrum is the pattern formed when a beam of light (EM – radiation) is broken up into its component frequencies.
The Hydrogen Spectrum Experiment 6 amplitude Wavelength -λ.
Flame Test Lab.
=detail&id=960B953BECE70277F640231B3EB2DF56B0CCF2EA&selectedIndex=18.
Chapter 5 Electrons In Atoms.
Molecular Fluorescence Spectroscopy
Ahmad Aqel Ifseisi Assistant Professor of Analytical Chemistry College of Science, Department of Chemistry King Saud University P.O. Box 2455 Riyadh
Spectroscopy Chapter 7.
Advanced Higher Chemistry Unit 1 Spectroscopy. Spectroscopy  Spectroscopy is used to give information regarding the structure of atoms or molecules.
Understanding infrared spectroscopy
Figure 1 Figure 8 Figure 9Figure 10 Altitude resolved mid-IR transmission of H 2 O, CH 4 and CO 2 at Mauna Loa Anika Guha Atmospheric Chemistry Division,
Light. White light emits light at all wavelengths. Excitation of certain elements or the electrical excitation of certain elements give rise to an atomic.
Earth Science 24.1 The Sun: Study of Light
FLUORESCENCE ENHANCEMENT BY CHELATION OF Eu 3+ AND Tb 3+ IONS IN SOL GELS A. J. Silversmith a A. P. Magyar a, K.S. Brewer a, and D.M. Boye b a Physics.
 How does the wavelength of a light beam and the size of a slit it is going through control the amount of diffraction? DO WORK STOP.
Lab 12 Atomic spectra and atomic structure
What is atomic spectra? In general The light which atoms give off is made up of specific wavelengths, called lines; observed by a spectroscope, the lines.
Emission Spectroscopy Electrons jump from higher levels to lower ones.
CHAPTER 4: Visible Light and Other Electromagnetic Radiation.
Fluorometric determination of riboflavin
Bohr’s Model of the Atom Scientists noticed that the laws of Classical Physics that applied to large objects did not seem to be able to explain.
 The Bohr model was proposed:  1913  by Neils Bohr  After observing the H line emission spectrum.
Infrared Spectroscopy
指導教授:林克默 學 生:陳立偉 Introduction Recently,the interest in up-conversion emission has been increased due to the needs for all-solid compact.
CHAPTER 4: Visible Light and Other Electromagnetic Radiation.
Main Classes of Stars Astrophysics Lesson 10. Homework  None, you have exams next week! Good Luck!
Mechanisms of Radio Wave Emission How different mechanisms create Radio Waves that are detectable by Radio Telescopesdifferent mechanisms.
Nuclear Physics Mr. Jean
日 期: 指導老師:林克默、黃文勇 學 生:陳 立 偉 1. Outline 1.Introduction 2.Experimental 3.Result and Discussion 4.Conclusion 2.
Asa Arjoon U6 Chemistry Presentation on Visible and Ultraviolet Spectroscopy Name : Form : Subject :
Quantum Theory, Part I The Atom Day 4 Prism n White light is made up of all the colors of the visible spectrum. –Passing it through a prism separates.
Homework 4 Unit 21 Problem 17, 18, 19 Unit 23 Problem 9, 10, 13, 15, 17, 18, 19, 20.
Atomic Fluorescence Spectroscopy. Background l First significant research by Wineforder and Vickers in 1964 as an analytical technique l Used for element.
Aim: How to distinguish electrons in the excited state
Topic #9 : Ground State vs. Excited State What is the difference between ground state and excited state electron configurations? How can we identify unknown.
Warm-Up Lithium has an atomic weight of g/mol. When g of lithium is heated, it emits an energy measured at 262,500 joules. What is the energy.
Ground State vs. Excited State
The Effect of Annealing Conditions and Concentration on 5 D 3  7 F J Emission in Terbium-doped Sol-gel Glasses * Colleen Gillespie and Dan Boye, Davidson.
Nanoscale Cr 4+ Doped Olivine Crystallites Used In Optical Amplifiers and Lasers Presentation by: Victor Ortiz Mentor: Dr. Alexei Bykov Mentor: Dr. Alexei.
1 Atomic Emission Spectroscopy Molecular Absorption Spectroscopy Lecture 21.
Infrared Spectroscopy
Types of Spectra.
Spectroscopy and Atoms
Fluorometric determination of riboflavin
Figure 1 Figure 8 Figure 9Figure 10 Altitude resolved mid-IR transmission of H 2 O, CH 4 and CO 2 at Mauna Loa Anika Guha Atmospheric Chemistry Division,
THE ORIGIN OF LIGHT. The example on this slide looks at a Hydrogen atom that begins in the energy state of n=3 (Don't worry, it is just a system used.
IB NOTES: Modern Analytical Chemistry. Definitions: Qualitative Analysis: The detection of the __________________ but not the __________ of a substance.
Light!. a form of radiation emitted by stars and other celestial bodies consists of changing electric and magnetic fields can travel through empty space.
Fluorescent Art Studio Glazes
Atomic Emission Spectra and Flame Test Lab
Atomic Emission Spectra
HOMEWORK # 6 Spectral Lines WS.
Bohr’s Model of the Atom
Ch 10: Modern Atomic Theory
Spectroscopy Chapter 7.
Aim: How to distinguish electrons in the excited state
Lecture 20 Light and Quantized Energy Ozgur Unal
BELLWORK 10/18/2016 SOLVE THE FOLLOWING NUCLEAR DECAY PROBLEMS:
Drying Control Additive: DMF
UNRAVELLING THE MYSTERIES OF THE ATOM AND THE UNIVERSE
YOYO: What element is this? How do you know?
Quantum Physics Atomic spectra and atomic energy states.
Flame Test Lab.
Rare Earth Calixarene Complexes in a Sol-Gel Matrix: Synthesis and Luminescence Karen S. Brewer, Department of Chemistry, Hamilton College, Clinton, NY.
IYNT 2017 NANJING Team BULGARIA
Light!.
Neils Bohr Tried to use the emission spectrum of hydrogen to further explain the atom Proposed that electrons orbit the nucleus in circular paths of fixed.
Atomic emission spectrum
Chemistry/Physical Setting
Presentation transcript:

Spectroscopic Analysis of Tb 3+ Doped Sol-Gels In recent years, there has been much research in the field of rare-earth (RE) dope sol-gel glasses. These glasses are formed by mixing water, hydrochloric acid, and either TMOS (tetramethylorthosilicate) or TEOS (tetraethylorthosilicate), and gradually heating over the span of a few days. This allows the mixture to gel, and then by letting it cool, a solid piece of glass is formed. During the formation of the gels, we can add ions of rare-earth metals from the lanthanide series of the periodic table. These elements frequently have very strong fluorescence in the visible spectrum. By exciting the ion’s electrons with ultraviolet light, the electrons will jump to a higher energy level, and subsequently drop down to a lower level, in the process emitting a photon. These photons are what cause the gels to glow. Figure A shows a Dieke diagram depicting energy levels for all the RE elements: Brendan W. Sullivan ‘07, Ann J. Silversmith, Karen S. Brewer Departments of Chemistry and Physics, Hamilton College Another factor that affects 5 D 3 emission is the concentration of Tb 3+ ions. We hypothesize that higher concentrations of RE ions result in more clustering and thus more quenching of fluorescence, and that lower concentrations will tend to show stronger peaks in the 5 D 3 range. This can be seen in Figure F. However, we have noticed that the differences between subsequent concentration changes become smaller for very low concentrations. The 5 D 3 to 5 D 4 peak ratios (see Figure I below) are very similar for 0.01% Tb and 0.02% Tb, and both are typically much better than any other concentration, so it’s possible that we have found the lower limit of RE concentration, meaning that the ions are dispersed through the matrix well enough such that any further reductions in concentration will not reduce clustering effects. Typically our sol-gels are annealed by gradually heating them to 750°C for 24 hours. As an experiment, we tried reheating sol-gel samples to higher temperatures for 6 hours. For instance, we tried reheating to 900°C, 950°C, and 1000°C for 6 hours. In terms of qualitative data, heating to 950°C and 1000°C yielded sol-gels that were slightly more cloudy, and less transparent. Heating to 900°C, though, seemed like a perfect temperature, as it yielded optically clear samples, and also showed strong 5 D 3 emission when tested. Figure G shows a comparison between annealing at 750°C and reheating to 900°C. One phenomenon that we examined and found to be consistent with current literature is the effect of Aluminum co-doping on the fluorescence of rare-earth ions in sol- gels. It is believed that the addition of Al 3+ ions to the matrix will increase the inter-ion separation between RE ions and thus reduce the effects of clustering. Our experimentation confirmed this idea, as show in the two graphs on the left. Figure D is an emission spectra of a sol-gel pellet containing 0.02% Tb and 0% Al (all percentages are by molar ratio relative to TMOS). Figure E is an emission spectra where the pellet also contains 2% Al. The 5 D 3 emission of the sol-gel containing 2% Al is clearly much stronger, thus showing that co- doping with Al 3+ ions helps reduce quenching effects on 5 D 3 emission. The most interesting phenomenon we noticed was the decay of 5 D 3 emission over time after reheating. Heating to 900°C yielded great results with strong 5 D 3 peaks, but unfortunately, when tested the next day, there was significantly less fluorescence in that region. Figure H shows how a sample containing 0.02% Tb and 2% Al decayed over time after being heated to 900°C for 6 hours. We also experimented with other co-dopants in the sol-gel recipe. One paper mentioned their results when co-doping with both Al 3+ and Na + ions, saying that “when both Al 3+ and Na + ions are co-doped at the same time, the composition dependent PL spectra…revealed that one of them compensates the spectral change due to the other.” 1 We attempted to obtain similar results by co-doping such that the total concentration of Al 3+ and Na + ions summed to 2%. When annealed at 750°C for 24 hours, the samples showed very little activity. However, when reheated to 900°C for 6 hours, they showed significantly stronger 5 D 3 emission (see Figure J). The 2% Na and 1.5% Na samples, though, still showed little activity. The best co-dopant amount that we tried appears to be 0.5% Na and 1.5% Al. Perhaps in the future other combinations of Al 3+ /Na + can be tested. References: 1. K. Itoh, N. Kamata, T. Shimazu, C. Satoh, K. Tonooka, K. Yamada. Journal of Luminescence (2000) T. Ishizaka, R. Nozaki, Y. Kurokawa. Journal of Physics and Chemistry of Solids 63 (2002) R. Reisfeld, T. Saraidarov, E. Ziganski, M. Gaft, S. Lis, M. Pietraskiewicz. Journal of Luminescence (2003) Thanks to: Profs. Silversmith and Brewer, Greg Armstrong, Helena Grabo, Kate Schirmer, Peter Burke Conclusions: Our project has examined many characteristics of Tb 3+ sol-gels. We have confirmed the idea that Al 3+ co-doping reduces clustering effects and improves 5 D 3 emission. Concentration effects, as well, have been confirmed, and in fact we believe we have found the lower limit of Tb 3+ concentration. Annealing temperature dependence, and the effects of decay over time after reheating, however, can be explored much further. Our experiments have shown that after reheating to 900°C for 6 hours, 5 D 3 emission gradually decreases (see Figure K), but we are unsure as to why exactly this happens. Perhaps future experiments will be able to examine the mechanism for this process and discover ways to prevent it. Finally, the effects of Al/Na co-doping can also be explored further by trying other combinations of the two ions. These are the problems we sought to examine with this project, in hopes of finding Tb to be a good probe for learning about rare-earth clustering and sol-gels in general. Along the way, we discovered other interesting phenomena as well Energy (1000cm -1 ) 7F67F F07F D45D4 5D35D3 414nm 436nm 460nm 490nm 545nm 590nm 620nm Fig. A: Dieke diagram Fig. B: cross-relaxation Fig. C: Tb 3+ energy levels This individual project was intended to examine the quenching processes in Terbium (Tb) doped sol-gel glasses. Neighboring Tb 3+ ions in the sol-gel matrix can undergo a process called cross-relaxation, where one ion’s electron drops down in energy and donates this energy to the other ion’s electron (Figure B). This is a problem because that drop in energy of the first electron yields a photon with a wavelength outside of the visible spectrum, whereas other energy level changes result in visible fluorescence that can be examined easily (Figure C). Another problem has to do with residual hydroxyl (OH - ) groups that remain even after the annealing process in sol-gel synthesis. These ion groups can affect the fluorescence of the Tb 3+ ions by releasing and absorbing energy into phonons, or tiny vibrational energies, as opposed to light. Fig. D Fig. E Fig. F: concentration dependence Fig. G: annealing temperature dependence Fig. H: 5 D 3 emission time decay Fig. I: 5 D 3 to 5 D 4 ratios To compare the 5 D 3 emission of different samples, we created a 5 D 3 to 5 D 4 ratio. We calculated the heights of each 5 D 3 peak and one 5 D 4 peak, and then found their ratio. Figure I shows the ratios for 5 sets of samples that we tested. It is clear that 2% Al shows more activity than 0% Al, and 900°C/6hrs shows more activity than 750°C/24hrs. Also, the samples that had aged 3 days since reheating to 900°C show very little activity. Finally, we tried reheating a set of samples to 900°C for 6 hours and then immediately placing them in a secure environment. To do this we used Schlenkware and a vacuum to create an airtight environment and to keep the samples unaffected by the atmosphere for 2 days. Then we removed them and tested their fluorescence. The results showed that they behaved almost as well as completely fresh samples, and clearly much better than other aged samples. (all spectroscopic data obtained on Fluoromax) Fig. K: 5 D 3 to 5 D 4 ratios over time Fig. J: Al 3+ /Na + co-doping Energy (1000cm -1 ) F07F D45D4 5D35D3 6