Indiana University-Purdue University Indianapolis (IUPUI) / Analysis of explosives (intact and post-blast) is of interest to the forensic science community to qualitatively identify the explosive(s) in an improvised explosive device (IED). This requires high sensitivity, selectivity, and specificity. Forensic science laboratories typically utilize visual/microscopic exams, spectroscopic analysis (e.g., Fourier Transform Infrared Spectroscopy (FTIR)) and gas chromatography/mass spectrometry (GC/MS) for explosive analysis/identification. However, GC/MS has limitations for explosive analysis due to difficulty differentiating between structural isomers (e.g., 2,4-dinitrotoluene, 2,5-dinitrotoluene and 2,6- dinitrotoluene) and thermally labile compounds (e.g., ethylene glycol dinitrate (EGDN), nitroglycerine (NG) and pentaerythritol tetranitrate (PETN)) due to mass spectra with very similar fragmentation patterns. The development of a benchtop vacuum ultraviolet spectrometer coupled to a gas chromatography (GC/VUV) was developed in 2014 with a wavelength region of 120 nm to 430 nm. GC/VUV can overcome limitations in differentiating explosive compounds that produces similar mass spectra. This work encompasses analysis of explosive compounds via GC/VUV to establish the sensitivity, selectivity, and specificity for the potential application for forensic explosive analysis. Nitrate ester and nitramine explosive compounds thermally decompose in the VUV flow cell resulting in higher specificity due to fine structure in the VUV spectra. These fine structures originate as vibronic and Rydberg transitions in the small decomposition compounds (nitric oxide, carbon monoxide, formaldehyde, water, and oxygen) and were analyzed computationally. The thermal decomposition process was further investigated for the determination of decomposition temperatures for the nitrate ester and nitramine compounds which range between 244 oC and 277 oC. Nitrated compounds were extensively investigated to understand the absorption characteristics of the nitro functional group in the VUV region. The nitro absorption maximum appeared over a wide range (170 - 270 nm) with the wavelength and intensity being highly dependent upon the structure of the rest of the molecule. Finally, the GC/VUV system was optimized for post-blast debris analysis. Parameters optimized include the final temperature of a ramped multimode inlet program (200 oC), GC carrier gas flow rate (1.9 mL/min), and VUV make-up gas pressure (0.00 psi). The transfer line/flow cell temperature was determined not to be statistically significant.

The determination of the plasma confinement propertiesdemand data as the electron temperature, the ionic and electrondensity profiles and the radiative emissivity profiles. Thefocus of this thesis is the importance of radial profiles inspectroscopic diagnostics applied to the EXTRAP-T2Rreversed-field pinch. EXTRAP-T2R is a resistive shell reversed-field pinch with amagnetic field shell penetration time much longer than therelaxation cycle time scale. Significant improvements inconfinement properties derived by quantitative plasmaspectroscopy in the vacuum ultraviolet are observed compared tothe previous device EXTRAP-T2. The low level of magneticturbulence and the good magnetic surfaces in the edge regionexplain this observed improvement. A current profile controlexperiment reduces the stochastic transport, which is connectedto the dynamo, and improves the confinement in EXTRAP-T2R evenmore. A comparison of the electron temperature estimated by usinga ratio of line intensities from the same ionization stage ofoxygen and the Thomson scattering system shows that thedifference is explained by the different spatial dependence ofthe excited state populations and the corresponding emissivityof these spectral lines. A collisional radiative model givesestimates for radial profiles of impurities which are notmeasured in EXTRAP-T2R. The estimated profiles can in turn beused to determine the radial profile of the effective ioncharge, the emissivity and finally the radiative power. Asinput, the model uses radial profiles. Neutral hydrogen is predominantly present in the boundaryregion of the plasma. Spectroscopic investigations in this areashow very asymmetric spectral lines of hydrogen due to themovement of atoms. The velocity of the hydrogen atoms dependson the type of plasma-wall interaction and their measurementhelps to identify the different interaction processes. Theexistence of hydrogen molecules in the edge complicates theinterpretation of the line shapes and on the determination ofthe particle confinement time. <b>Keywords:</b>Reversed-field pinch, EXTRAP-T2R, quantitativeplasma spectroscopy, VUV spectroscopy, line-integrated electrontemperature, oxygen, profiles, confinement properties, powerbalance, hydrogen, particle confinement time.

<p>The determination of the plasma confinement propertiesdemand data as the electron temperature, the ionic and electrondensity profiles and the radiative emissivity profiles. Thefocus of this thesis is the importance of radial profiles inspectroscopic diagnostics applied to the EXTRAP-T2Rreversed-field pinch.</p><p>EXTRAP-T2R is a resistive shell reversed-field pinch with amagnetic field shell penetration time much longer than therelaxation cycle time scale. Significant improvements inconfinement properties derived by quantitative plasmaspectroscopy in the vacuum ultraviolet are observed compared tothe previous device EXTRAP-T2. The low level of magneticturbulence and the good magnetic surfaces in the edge regionexplain this observed improvement. A current profile controlexperiment reduces the stochastic transport, which is connectedto the dynamo, and improves the confinement in EXTRAP-T2R evenmore.</p><p>A comparison of the electron temperature estimated by usinga ratio of line intensities from the same ionization stage ofoxygen and the Thomson scattering system shows that thedifference is explained by the different spatial dependence ofthe excited state populations and the corresponding emissivityof these spectral lines. A collisional radiative model givesestimates for radial profiles of impurities which are notmeasured in EXTRAP-T2R. The estimated profiles can in turn beused to determine the radial profile of the effective ioncharge, the emissivity and finally the radiative power. Asinput, the model uses radial profiles.</p><p>Neutral hydrogen is predominantly present in the boundaryregion of the plasma. Spectroscopic investigations in this areashow very asymmetric spectral lines of hydrogen due to themovement of atoms. The velocity of the hydrogen atoms dependson the type of plasma-wall interaction and their measurementhelps to identify the different interaction processes. Theexistence of hydrogen molecules in the edge complicates theinterpretation of the line shapes and on the determination ofthe particle confinement time.</p><p><b>Keywords:</b>Reversed-field pinch, EXTRAP-T2R, quantitativeplasma spectroscopy, VUV spectroscopy, line-integrated electrontemperature, oxygen, profiles, confinement properties, powerbalance, hydrogen, particle confinement time.</p>

L'étude de la photochimie dans le système solaire est de toute première importance pour appréhender la chimie organique complexe au sein d'un environnement extraterrestre. Parmi ces environnements, les comètes revêtent un intérêt particulier en exobiologie puisqu'elles ont pu, ainsi que leurs grains, être des vecteurs de matière organique sur la Terre primitive et ainsi contribuer à l'émergence de la vie. Mais dans quelle mesure, la matière organique potentiellement présente au sein des grains survit-elle face aux rayonnements solaires? Ma thèse porte sur l'étude de la dégradation photochimique de trois bases azotées (adénine, guanine et uracile) et d'un acide aminé (glycine) dans les conditions du système solaire, c'est à dire soumis à des rayonnements énergétiques VUV/UV ( <300 nm). Les études conduites lors de ce travail peuvent aussi être appliquées à l'interprétation des mesures du le spectromètre de masse COSIMA présent sur l'orbiteur de la mission cométaire ROSETTA et dont l'objectif est l'analyse de la surface de grains cométaires capturés dans l'environnement de la comète 67P/Churyomov-Gerasimenko. Ce travail présente les spectres de sections efficaces d'absorption mesurés dans les domaines VUV/UV pour des films organiques purs. Ces spectres ont mené à la déduction de constantes de photolyse, ainsi qu'à l'élaboration d'un modèle simulant la cinétique de destruction globale d'un film organique optiquement épais. La confrontation entre ce modèle et les données expérimentales d'irradiation en orbite basse terrestre ainsi qu'en laboratoire a permis d'estimer les temps de vie des molécules considérées à 1 ua puis extrapolés à différentes distances héliocentriques. Les résultats obtenus ont montré que la glycine, l'adénine et la guanine, potentiellement présentes au sein des grains cométaires, seraient totalement détruites entre le moment de l'éjection des grains du noyau cométaire et l'arrivée sur Terre si elles sont en surface. En sous-surface, elles sont au contraire très stables, de part la protection efficace que leur confèrent les minéraux constitutifs du grain contre les rayonnements solaires. Dans le cadre de la mission ROSETTA, les résultats diffèrent. Au plus loin du soleil, à 3,5 ua, l'abondance des molécules ne diminuerait pas de façon significative pendant le temps de parcours des grains entre le noyau et l'orbiteur. Au périhélie, la "survie" des molécules dépendra fortement de la distance noyau-orbiteur. Les pertes significatives des 3 molécules par photochimie n'auraient lieu que si l'orbiteur se situe au moins à quelques centaines de kilomètres du noyau / The study of photochemistry in the solar system is of prime importance to assess complex organic chemistry in an extraterrestrial environment. Among those environments, comets are subject to a particular interest in the context of exobiology, along with their grains, as they could have bring organic matter on the primitive earth, and hence contribute to the emergence of life. But to what extent does the organic matter potentially with in grains survive face to solar radiation? My thesis deals with the study of photochemical degradation of three nitrogenous bases (adenine, guanine and uracil) and one amino acid ( glycine) in the conditions of the solar system, which means subject to VUV/UV energetically radiations ( <300 nm). Studies performed during this work can also be applied to the interpretation of COSIMA mass spectrometer, present on the cometary mission ROSETTA, which aims to analyze the surface of cometary grains captured in the environment of the 67P/Churyomov-Gerasimenko comet. This work present absorption cross section spectrum measured in the VUV/UV range, for pure organic films. These spectrum led to the deduction of photolysis rate constants, and to the elaboration of a model simulating the global kinetic of destruction of a optically thick organic film. The comparison between this model and experimental data of low earth orbit irradiation as well as laboratory data allowed to estimates lifetimes for the considered molecules at 1 AU, and then extrapolated at different heliocentrically distances. Results show that glycine, adenine and guanine, potentially existing inside the cometary grains, would be entirely destroyed between the ejection of the grains and the arrival on earth if they exist at the surface. Below the surface, they are at the contrary very stable, thanks the effective protection of the mineral constitutive of the grain against solar radiations. In the frame of ROSETTA mission, results differ. At the farther of the sun, at 3.5 AU, the abundance of the molecule would not significantly decrease during the time of travel of grains between the core and the orbiter. At the perihelia, the survival of molecule strongly depends of the core-orbiter distance. Significant loss of the 3 molecules by photochemistry would only occurred if the orbiter is at more than hundred of kilometers from the core

Depuis le début de la microélectronique, l’industrie a développé sans arrêt des nouvelles technologies de gravure plasma pour diminuer la taille des dispositifs tout en réduisant le cout de fabrication et en augmentent les performances des circuits intégrés. Aujourd’hui, les transistors tel que le FDSOI 22nm ou FinFET 10 nm doivent être gravé avec une précision sub-nanométrique et sans endommager la sous-couche sur plus d’une couche atomique. Pour arriver à faire cela, de nouvelles technologie se développent, dont le Smart Etch. Cette technologie en deux étapes consiste à modifier la surface du matériau sous l’action d’un plasma, puis à retirer ce matériau modifié sélectivement par rapport au matériau non modifié. Le but de cette thèse est d’étudier la faisabilité de remplacer les plasmas de He et H2 utilisé dans le Smart Etch par des plasmas d’O2. L’intérêt est l’oxydation du matériau est une réelle modification chimique, permettant l’élimination sélective de ce dernier en RPS. Par ailleurs, contrairement aux plasma de He/H2, le plasma de O2 ne grave pas les parois du réacteur et rejette beaucoup moins d’impuretés dans le plasma. Dans un premier temps, nous avons étudié les mélanges gazeux NF3/H2 et NF3/NH3 utilisés dans l’étape de retrait RPS. Ces études ont été fait grâce à la spectroscopie d’absorption VUV et d’émission UV. Nous avons mis en évidence la création de HF dans les deux mélanges et nous avons mis en avant de manière indirecte la création de NH4F (cette espèce jouant un rôle clé dans la formation des sels) à partir de NH3 et HF. De plus nous avons observé la présence de F et H qui sont responsable de la gravure de SiO2 et SiN lorsque H2<NF3 et NH3<NF3. Dans un second temps, nous avons étudié par XPS angulaire et ellipsométrie l’implantation des ions oxygène dans du SiN avec différent flux et énergie ionique. Cela a bien montré que le SiN initial est transformé en une couche SiOxNy avec une contribution SiO2 importante, sous réserve que l’état stationnaire soit atteint (il faut une dose d’ions significative pour cela). Le flux, l’énergie des ions et le temps de traitement sont donc les paramètres clés pour le contrôle de la couche modifié. Enfin, des tests préliminaires de gravure cyclique de SiN pleine plaque en mode « ALE » (c’est dire monocouche atomique par monocouche atomique) ainsi qu’en mode standard (retrait de quelques nanomètres / cycle) montrent que le principe de gravure est réaliste. Ce travail ouvre donc la voie au développement de ce nouveau type de procédé. / Since the beginning of microelectronics, the industry has continuously developed new plasma etching technologies to reduce the size of devices while reducing the cost of manufacturing and increase the performance of integrated circuits. Today, transistors such as 22nm FDSOI or 10nm FinFET must be engraved with sub-nanometric precision and without damaging the underlayment on more than one atomic layer. To achieve this, new technologies are developing, including the Smart Etch. This two-step technology involves modifying the surface of the material under the action of a plasma and then removing selectively the modified material from the unmodified material. The aim of this thesis is to study the feasibility of replacing the He and H2 plasmas used in the Smart Etch by O2 plasmas. The interest is the oxidation of the material, that it is a real chemical modification, allowing latter the selective elimination by RPS. Moreover, unlike He / H2 plasma, the O2 plasma does not damage the reactor walls and releases much less impurities into the plasma. Firstly, we studied the gaseous mixtures NF3 / H2 and NF3 / NH3 used in the step of RPS remove. Thouse studies were done through VUV absorption spectroscopy and UV emission. We have demonstrated the creation of HF in both mixtures and we have indirectly highlighted the creation of NH4F (this species plays a key role in the formation of salts) from NH3 and HF. In addition we observed the presence of F and H which are responsible for the etching of SiO2 and SiN when H2 <NF3 and NH3 <NF3. Secondly, we studied angular XPS and ellipsometry by implanting oxygen ions in SiN with different flux and ionic energy. This has shown that the initial SiN is transformed into a SiOxNy layer with a significant SiO2 contribution, provided that the stationary state is reached (a significant dose of ions is required for this). Flux, ion energy and processing time are therefore the key parameters for controlling the modified layer.Finally, preliminary tests of full-plate SiN cyclic etching in "ALE" mode (ie atomic monolayer by atomic monolayer) as well as in standard mode (removing a few nanometers / cycle) show that the etching principle is realistic. This work opens the way to the development of this new type of process.

Les composés perfluorés possèdent des propriétés à la fois hydrophobes et lipophobes et sont commercialisés depuis les années 1950. Ils ont été depuis largement utilisés dans de nombreuses applications industrielles. Cependant, il s’agit de composés persistants, bioaccumulatifs, avec de grandes durées de vie atmosphérique. Ces espèces sont considérées comme de puissants gaz à effet de serre, et seraient principalement dégradées par photolyse, dans la haute atmosphère. Un travail de caractérisation physicochimique de deux composés perfluorés, le PFOA et le PFOS, produits de dégradation ultime des composés perfluorés les plus utilisés, a été réalisé. Des expériences de spectroscopie VUV et spectrométrie de masse ont permis d’identifier les voies de relaxation de ces composés après photoactivation. Une méthodologie par couplage rayonnement synchrotron/spectrométrie de masse permettant la mesure de sections efficaces absolues a été développée puis appliquée aux composés d’intérêt. Ces mesures ont ensuite été reliées à leur taux de photolyse et durées de vie atmosphérique selon l’altitude. / Perfluorocarbons compounds have both hydrophobic and lipophobic properties. They have been manufactured since the 1950s, and widely used in many industrial applications. However, they are persistent, bioaccumulative compounds with long atmospheric lifetimes. They are considered to be potent greenhouse gases, and are supposed to be mainly degraded by photolysis in the upper atmosphere. A work of physicochemical characterization of two perfluorinated compounds was realized on the PFOA and PFOS. They have been found to be the final compounds of degradation of the majority of perfluororinated compounds. VUV spectroscopy and mass spectrometry experiences have been undertaken to identify their relaxation pathways after photoactivation. A methodology based on the coupling of synchrotron radiation and mass spectrometry was developed to perform absolute cross section measurements and was apply to the compounds of interest. These measurements have been used to determine their photolysis rates and atmospheric lifetimes according to the altitude.