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Light up-conversion in rare earth doped thin films : synthesis, characterization, luminescence and prospects for solar cell application / Etude de la up-conversion de la lumière dans les couches minces dopées terres rares : synthèse, caractérisation, luminescence et perspectives pour l'application aux cellules solairesPayrer, Elisabeth L. 12 February 2014 (has links)
Le phénomène d’up-conversion de photon (UpC) permet de générer de la lumière à longueurs d’onde plus courtes que la longueur d’onde d’excitation. Dans cette recherche, la synthese de couches minces dopées avec des ions de terres rares (RE3+) optiquement actifs, leurs caractérisations structurales, ainsi que leurs propriétés optiques et de photoluminescentes ont été étudiées. Les couches ont été élaborées par deux voies de dépôt de couche sur du silicium et des substrats transparents: tout d’abord, un dépôt chimique organométallique en phase vapeur (LI-MOCVD, AA-MOCVD) est utilisé pour le dépôt des couches minces de YF3 et Y2O3 co-dopées Er/Yb. Il est démontré que l’émission d’UpC de Er3+ avec une excitation à 972 nm est influencée par le réseau hôte. Par ailleurs, le traitement sol-gel, une technique chimique par voie humide, est utilisé pour la fabrication de couches minces Y2O3, SiO2 et TiO2 co-dopées Er/Yb par spin-coating. Une optimisation de l’´emission de lumière par UpC a été atteinte grâce à l’ajustement de la concentration de RE et de la température de traitement thermique. De plus, une approche différente a été étudiée pour atteindre une émission UpC renforcée : l’utilisation de microcavités diélectriques de Fabry-Pérot obtenues par sol-gel, constitués d’un empilement de couches de silice et d’oxyde de titane, avec Er/Yb:Y2O3 comme couche de cavité. Le but de ce travail est de répondre aux questions suivantes: comment la nature du réseau hôte et le niveau de dopage influencent l’émission radiative de l’Er3+? Quelles sont les conditions pour un bon matériau d’UpC et ses limites? Nous incluons également une discussion sur les perspectives d’une application possible d’une couche d’UpC dans un dispositif de cellule solaire, qui pourrait améliorer la réponse dans l’infrarouge. / Photon up-conversion (UpC) allows the generation of light of shorter wavelengths compared to the excitation wavelength. In this work the synthesis of thin films doped with optically active rare earth (RE3+) ions, their structural characterization, as well the optical and photoluminescence properties are highlighted. The emphasis lies on two different routes of film deposition on silicon and transparent substrates: first, metalorganic chemical vapor deposition (LI-MOCVD, AA-MOCVD) is introduced for the deposition of Er/Yb-doped YF3 and Y2O3 films and it is demonstrated, how the UpC emission of Er3+ upon 972 nm excitation is influenced by the host lattice. Secondly, sol-gel processing, a wet-chemical technique, is used for the fabrication of Er/Yb-doped Y2O3, SiO2 and TiO2 thin films by spin-coating. Optimization of the up-converted light emission was achieved through adjusting the RE concentration and the processing temperature. Moreover, in a different approach for achieving an enhanced UpC emission, sol-gel derived Fabry-Pérot dielectric microcavities, consisting of a multilayer stack of silica and titania layers and Er/Yb: Y2O3 as the cavity layer, are investigated. The aim of this work is to address the questions, how does the nature of the host lattice and doping level influence the radiative emission in Er3+, what are the requirements for a good upconverter material and what are the limitations? We also include a discussion of the application of an upconverter to a solar cell device, which may debatably enhance the response in the infrared.
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A Radio Frequency Quadrupole Instrument for use with Accelerator Mass Spectrometry: Application to Low Kinetic Energy Reactive Isobar Suppression and Gas–phase Anion Reaction StudiesEliades, John Alexander 21 August 2012 (has links)
A radio frequency (rf) quadrupole instrument, currently known as an Isobar Separator for Anions (ISA), has been integrated into an Accelerator Mass Spectrometry (AMS) system to facilitate anion–gas reactions before the tandem accelerator. An AMS Cs+ sputter source provided > 15 keV ions that were decelerated in the prototype ISA to < 20 eV for reaction in a single collision cell and re-accelerated for AMS analysis. Reaction based isobar suppression capabilities were assessed for smaller AMS systems and a new technique for gas–phase reaction studies was developed.
Isobar suppression of 36S– and 12C3– for 36Cl analysis, and YF3– and ZrF3– for 90Sr analysis were studied in NO2 with deceleration to < 12 eV. Observed attenuation cross sections, σ [x 10^–15 cm^2], were σ(S– + NO2) = 6.6, σ(C3– + NO2) = 4.2, σ(YF3– + NO2) = 7.6, σ(ZrF3– + NO2) = 19. With 8 mTorr NO2, relative attenuations of S–/Cl– ~ 10^–6, C3–/Cl– ~ 10^–7, YF3–/SrF3– ~ 5 x 10^–5 and ZrF3–/SrF3– ~ 4 x 10^–6 were observed with Cl– ~ 30% and SrF3– > 90% transmission. Current isobar attenuation limits with < 1.75 MV accelerator terminal voltage and ppm impurity levels were calculated to be 36S–/Cl– ~ 4 x 10^–16, 12C3–/Cl– ~ 1.2 x 10^–16, 90YF3–/SrF3– ~ 10^–15 and 90ZrF3–/SrF3– ~ 10^–16.
Using 1.75 MV, four 36Cl reference standards in the range 4 x 10^–13 < 36Cl/Cl < 4 x 10^–11 were analyzed with 8 mTorr NO2. The measured 36Cl/Cl ratios plotted very well against the accepted values. A sample impurity content S/Cl < 6 x 10^–5 was measured and a background level of 36S–/Cl < 9 x 10^–15 was determined.
Useful currents of a wide variety of anions are produced in AMS sputter sources and molecules can be identified relatively unambiguously by stripping fragments from tandem accelerators. Reactions involving YF3–, ZrF3–, S– and SO– + NO2 in the ISA analyzed by AMS are described, and some interesting reactants are identified.
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A Radio Frequency Quadrupole Instrument for use with Accelerator Mass Spectrometry: Application to Low Kinetic Energy Reactive Isobar Suppression and Gas–phase Anion Reaction StudiesEliades, John Alexander 21 August 2012 (has links)
A radio frequency (rf) quadrupole instrument, currently known as an Isobar Separator for Anions (ISA), has been integrated into an Accelerator Mass Spectrometry (AMS) system to facilitate anion–gas reactions before the tandem accelerator. An AMS Cs+ sputter source provided > 15 keV ions that were decelerated in the prototype ISA to < 20 eV for reaction in a single collision cell and re-accelerated for AMS analysis. Reaction based isobar suppression capabilities were assessed for smaller AMS systems and a new technique for gas–phase reaction studies was developed.
Isobar suppression of 36S– and 12C3– for 36Cl analysis, and YF3– and ZrF3– for 90Sr analysis were studied in NO2 with deceleration to < 12 eV. Observed attenuation cross sections, σ [x 10^–15 cm^2], were σ(S– + NO2) = 6.6, σ(C3– + NO2) = 4.2, σ(YF3– + NO2) = 7.6, σ(ZrF3– + NO2) = 19. With 8 mTorr NO2, relative attenuations of S–/Cl– ~ 10^–6, C3–/Cl– ~ 10^–7, YF3–/SrF3– ~ 5 x 10^–5 and ZrF3–/SrF3– ~ 4 x 10^–6 were observed with Cl– ~ 30% and SrF3– > 90% transmission. Current isobar attenuation limits with < 1.75 MV accelerator terminal voltage and ppm impurity levels were calculated to be 36S–/Cl– ~ 4 x 10^–16, 12C3–/Cl– ~ 1.2 x 10^–16, 90YF3–/SrF3– ~ 10^–15 and 90ZrF3–/SrF3– ~ 10^–16.
Using 1.75 MV, four 36Cl reference standards in the range 4 x 10^–13 < 36Cl/Cl < 4 x 10^–11 were analyzed with 8 mTorr NO2. The measured 36Cl/Cl ratios plotted very well against the accepted values. A sample impurity content S/Cl < 6 x 10^–5 was measured and a background level of 36S–/Cl < 9 x 10^–15 was determined.
Useful currents of a wide variety of anions are produced in AMS sputter sources and molecules can be identified relatively unambiguously by stripping fragments from tandem accelerators. Reactions involving YF3–, ZrF3–, S– and SO– + NO2 in the ISA analyzed by AMS are described, and some interesting reactants are identified.
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