À ses débuts, la conquête spatiale a pu bénéficier des rivalités politiques de la Guerre Froide pour se développer rapidement sans réellement se soucier des efforts économiques à fournir. Aujourd’hui, de nombreux pays subissent le revers de la médaille de cette course effrénée : pour maintenir une flotte de lanceurs viable économiquement, les différentes agences spatiales doivent faire face à un dilemme opposant la minimisation des coûts de lancement à la maximisation de leur fiabilité. Dans cette logique d’optimisation, les industriels présents dans ce processus de réflexion se tournent vers la simulation numérique pour tenter d’améliorer leurs connaissances des technologies existantes, en particulier sur les zones d’ombres inaccessibles aux mesures expérimentales. Dans la lignée de plusieurs études théoriques et expérimentales, ces travaux visent à apporter un éclairage nouveau sur les phénomènes se produisant lors de l’allumage d’un moteur fusée cryotechnique. Ces recherches se tournent dans un premier temps vers l’amélioration de la modélisation de la flamme H2/O2. La validation d’une cinétique chimique réduite initialement destinée à la combustion H2/Air permet de justifier son utilisation lors de l’allumage. Puis, le développement d’un modèle de combustion turbulente pour le régime de flamme de diffusion est mené dans le but de palier aux limitations du modèle de flamme épaissie. Enfin, une analyse du cas où les régimes prémélangés et non-prémélangés sont présents tous les deux permet d’étudier un moyen simple de les distinguer même dans le cas où ils sont très proches. Dans un second temps, ces travaux se tournent vers l’étude de l’allumage dans un moteur fusée cryotechnique. Après avoir analysé de manière globale le calcul d’une séquence simplifiée, deux études plus approfondies sont menées pour investiguer, d’une part, les différents régimes de combustion, et d’autre part, les différents modes de propagation de la flamme propres à cette configuration.

A sustainable solution for meeting the energy demands at our planet is by utilizing wind-, solar-, wave-, thermal-, biomass- and hydroelectric power. These renewable and CO2 emission-free energy sources are highly variable in terms of spatial and temporal availability over the Earth, introducing the need for an appropriate method of storing and carrying energy. Hydrogen has gained significant attention as an energy storage- and carrier media because of the high energy density that is exploited within the ‘power-to-gas’ process chain. A robust way of producing sustainable hydrogen is via electrochemical water splitting. In this work the search for new heterogeneous catalyst materials with the aim of increasing energy efficiency in water splitting has involved methods of both electrochemical water splitting and chemical water oxidation. Some 21 compounds including metal- oxides, oxofluorides, oxochlorides, hydroxide and metals have been evaluated as catalysts. Two of these were synthesized directly onto conductive backbones by hydrothermal methods. Dedicated electrochemical cells were constructed for appropriate analysis of reactions, with one cell simulating an upscale unit accounting for realistic large scale applications; in this cell gaseous products are quantified by use of mass spectrometry. Parameters such as real time faradaic efficiency, production of H2 and O2 in relation to power input or overpotentials, Tafel slopes, exchange current density and electrochemical active surface area as well as turnover numbers and turnover frequencies have been evaluated. Solubility, possible side reactions, the role of the oxidation state of catalytically active elements and the nature of the outermost active surface layer of the catalyst are discussed. It was concluded that metal oxides are less efficient than metal based catalysts, both in terms of energy efficiency and in terms of electrode preparation methods intended for long time operation. The most efficient material was Ni-Fe hydroxide electrodeposited onto Ni metal foam as conductive backbone. Among the other catalysts, Co3Sb4O6F6 was of particular interest because the compound incorporate a metalloid (Sb) and redox inert F and yet show pronounced catalytic performance. In addition, performance of materials in water splitting catalysis has been discussed on the basis of results from electron microscopy, solubility experiments and X-ray diffraction data.

Dans le cadre de la recherche de nouvelles sources d'énergie propres et durables, nous étudions les mécanismes de formation du dihydrogène (H2) dans les environnements intra-cratoniques. Des émanations naturelles de H2 ont précédemment été décrites à proximité des dorsales médio-océaniques et des ceintures ophiolitiques. Cette production naturelle de gaz, telle que documentée dans la littérature, est étroitement liée au métasomatisme de roches ultrabasiques d'origine mantellique, riches en minéraux ferromagnésiens, à travers les réactions de serpentinisation. Au Kansas (USA), des émanations de H2 intra-cratonique ont été révélées dès les années 80 par l'étude de puits riches en H2. Nos travaux s'appuient sur un nouveau forage, D#2 (Kansas, USA), ainsi que deux forages existants depuis les années 80, Heins#1 et Scott#1 (Kansas, USA). Le puits D#2 permet d'accéder à un aquifère modérément profond (~300 m) chargé en H2. Le gaz est composé également de N2 et de CH4 tout comme le gaz issu des contextes ophiolitiques. Du He est présent en quantité substantielle -comparé aux contextes précédents- dans ces forages. Afin de comprendre les processus engendrant la production de H2 dans ce contexte géologique, de quantifier le gaz ainsi généré, et de déterminer la relation du H2 avec les autres espèces gazeuses une étude multidisciplinaire gaz/eau/roche a été réalisée. Les résultats obtenus lors de l'étude de ces fluides mis en parallèle avec le contexte géologique régional et les lithologies observées ont permis (1) de proposer différents scénarios pour expliquer les associations de gaz observées et (2) de discuter de l'origine et des processus de production du H2, de l'He, et du N2. / As part of the search for new sources of clean and sustainable energy, the mechanisms for the formation of dihydrogen (H2) in intracratonic environments were studied. Natural emissions of H2 have been described in the vicinity of mid-ocean ridges and ophiolite belts. This natural gas production, as documented in the literature, is closely related to the metasomatism of mantle rocks which are rich in mafic minerals, through the serpentinization reaction. In Kansas (USA), intracratonic H2 seepages were revealed in the 80’s by studies of H2-rich wells. Our work is based on a new borehole D#2 (Kansas, USA), and two boreholes previously studied in the 80s, Heins#1 and Scott#1 (Kansas, USA). The D#2 well provides access to a moderately deep aquifer (~ 300 m) loaded with H2. The gas is also composed of N2 and CH4 similarly to the gases issued from ophiolitic contexts. Helium is present in substantial quantities -compared to preceding contexts- in these boreholes. A multidisciplinary gas/water/rock study was carried out to understand the processes generating the production of H2 in this geological setting, to quantify the gas so generated, and to determine the relationship of H2 with other gaseous species. The results of these studies in parallel with the regional geological setting and observed lithology allowed (1) to propose several scenarios to explain the observed associations of gas and (2) to discuss the origin and production process of H2, He and N2.

O objetivo deste trabalho é o estudo das condições de existência e a determinação da concentração da molécula H2 em diferentes condições típicas de nebulosas planetárias, dentro da região ionizada. Para este cálculo, desenvolvemos sub-rotinas computacionais que se acoplam ao código de fotoionização unidimensional Aangaba que, até agora, somente considerava espécies atômicas (H, He, C, N, O, Mg, Ne, Si, S, Ar, Cl e Fe) e seus íons. Inserimos nesse código os equilíbrios químico e de ionização envolvendo a molécula H2 e os demais compostos de hidrogênio, H-, H2+, H3+, além do H, H+ e dos elétrons que o código de fotoionização Aangaba já considerava em sua forma original. A molécula H3 não é considerada por ser instável. Levamos em conta 41 diferentes mecanismos de formação e destruição desses compostos do hidrogênio. Destacamos particularmente o efeito da reação de formação de H2 na superfície de grãos na produção global dessa molécula em nebulosas planetárias, considerada na literatura como a rota mais importante de formação dessa molécula no meio interestelar. Para isso, estudamos a possibilidade da sobrevivência de grãos dentro da região ionizada da nebulosa planetária. Analisamos também a influência das propriedades da estrela central e da densidade do gás, assim como das propriedades dos grãos astrofísicos, na concentração de H2. Demonstramos que quantidades significativas de H2 podem sobreviver dentro da região ionizada de nebulosas planetárias, principalmente na região de recombinação do hidrogênio. A concentração de H2 relativa à densidade total de H alcança valores de até 1E-4 e a razão entre a massa de H2 e a massa total de H da NP chega a valores de 4E-4. Verificamos que a razão entre a massa de H2 e a massa de H total da nebulosa aumenta significativamente com o aumento da temperatura de estrela central. Essa maior quantidade de H2 em nebulosas planetárias com estrela central mais quente pode explicar porque é mais comum encontrar emissão da molécula H2 em nebulosas planetárias com estrutura bipolar (regra de Gatley), já que nebulosas com esse tipo morfológico têm estrela central tipicamente mais quente. Na literatura, o valor 6,9E-5 é obtido para a razão entre a massa de H2 e a massa de H total da nebulosa planetária NGC 6720, a partir de dados observacionais. Usando os mesmos parâmetros deste artigo, calculamos com o código de fotoionização Aangaba o valor de 3,3E-5, que está razoavelmente próximo do valor da literatura. / The goal of this work is the study of the H2 molecule survival and the determination of its abundance in different typical planetary nebulae conditions inside the ionized region. In order to do these calculations, we developed Fortran subroutines for the Aangaba one-dimensional photoionization code that, until this work, only took into account the atomic species (H, He, C, N, O, Mg, Ne, Si, S, Ar, Cl, and Fe) and their ions. Ionization and chemical equilibria of H, H+, H-, H2, H2+, and H3+ are assumed. The H3 molecule is not included because it is unstable. Fortyone different reactions that could form and destroy these species are taken into account. Reaction on grain surfaces, the most important mechanism for the production of H2 molecules in the interstellar medium, is analyzed in detail in the conditions of planetary nebulae ionized regions. We make a careful analysis of the grain survival in these regions. We also study the influence of the central star properties and gas density, as well as the astrophysical grain properties in the obtained H2 concentration. It is shown that a significant concentration of H2 can exist inside the ionized region of planetary nebulae, mostly in the recombination zone. The H2 concentration relative to the total hydrogen concentration reaches values as high as 1E-4 and the H2 mass to total hydrogen mass ratio inside the ionized region reaches values as high as 4E-4. The ratio increases with increasing temperature. This fact can explain why the H2 emission is more often observed in bipolar planetary nebulae (Gatley?s rule), since this kind of object has typically hotter stars. In the literature a H2 mass to total hydrogen mass ratio equal to 6.9E-5 is estimated from observations for the planetary nebula NGC6720. With the same input parameters for the gas density and the stellar spectrum, we calculated a ratio equal to 3.3E-5, close to the observed value.

Well-defined silica supported bimetallic catalysts Pt100-x Pdx (where x is the molar ratio of Pd) are prepared by Surface Organometallic Chemistry (SOMC) via controlled decomposition of Pd2(allyl)2Cl2 on Pt/SiO2. For comparison purposes, Pt100-x Pdx bimetallic catalysts is also prepared by ion-exchange (IE). According to the results of STEM, XAS and H2 chemisorption, all bimetallic nanoparticles, prepared using neither SOMC nor IE, produce discrete formation of monometallic species (either Pt or Pd). Most catalysts exhibit a narrow particle size distribution with an average diameter ranging from 1 to 3 nm for samples prepared by IE and from 2 to 5 nm for the ones synthesized by SOMC. For all catalysts investigated in the present work, iso-butane reaction with hydrogen under differential conditions (conversions below 5%) leads to the formation of methane and propane (hydrogenolysis), n-butane (isomerization), and traces of iso-butylene (dehydrogenation). The total rate of reaction decreases with increasing the Pd loading for both catalysts series as a result of decreasing turnover rate (expressed as moles converted per total surface metal per second) of both isomerization and hydrogenolysis. In the case of Pt100-x Pdx(SOMC) catalysts, the results suggest a selective coverage of Pt (100) surface by a Pd layer, followed by a buildup of Pd overcoat onto a Pd layer assuming that each metal keeps its intrinsic catalytic properties. There is no mutual electronic charge transfer between the two metals (DFT). For the PtPd catalysts prepared by IE, the catalytic behavior cannot simply be explained by a surface coverage of highly active Pt metal by less active Pd (not observed), suggesting there is formation of a surface alloy between Pt and Pd collaborated by EXAFS and DFT. The catalytic results are explained by a simple structure activity relationship based on the previously proposed mechanism of C-H bond and C-C Bond activation and cleavage for iso-butane hydrogenolysis, isomerization, cracking and dehydrogenation.

Solar energy is the most abundant efficient and important source of renewable energy. The objective of this study is to develop highly efficient visible light responsive photocatalysts for overall water splitting. This is done by using silver or copper containing materials. Phosphate compounds have caught much attention due to their rigid structure, thermal stability and resistance to chemical attacks. Solid phosphates can be prepared by direct solid-state reaction between metal cations and phosphate anions at high temperatures. Double metal phosphates of the Nasion-type structure had shown further technological importance. It has been reported that well-crystallized double metal phosphate particles have excellent ordering and cationic conduction channels in the Nasicon framework. In this study, several Nasion-type structured materials have been synthesized by solid-state method (e.g. CuTi2(PO4)3 and AgTi2(PO4)3) heated up under different temperatures (400–1100C) in N2 or air atmosphere. These materials were characterized by XRD, SEM, DR-UV-Vis spectroscopy and tested for photocatalytic applications. A new method for direct synthesis of photoelectrode on Ti Plate had been demonstrated. Further investigations on controlling the size and morphology for better performance of single and double metal phosphates will be done.

NR 20140805

京都大学 / 新制・課程博士 / 博士(理学) / 甲第23598号 / 理博第4760号 / 新制||理||1682(附属図書館) / 京都大学大学院理学研究科化学専攻 / (主査)教授 寺西 利治, 教授 若宮 淳志, 教授 倉田 博基 / 学位規則第4条第1項該当 / Doctor of Science / Kyoto University / DGAM

Presentation of antigenic peptides on MHC-II molecules is essential for induction of tolerance to self and for effective immunity against foreign pathogens. The non- classical MHC-II molecule DO (HLA-DO in humans, H2-O in mice) functions in selection of MHC-II epitopes by competitively inhibiting the peptide exchange factor DM. Previous studies have suggested a role for DO in development of autoimmunity and in the immune response to retroviral infection, presumably via modulation of the MHC-II peptidome, but the precise effect of DO has been difficult to discern. Through characterization of the full spectrum of peptides from DO-sufficient and DO-deficient cells, we demonstrate that DO functions to broaden the diversity of peptide species presented on MHC-II. DO is regulated differently from other components of the MHC-II processing machinery, with expression limited to B cell and dendritic cell subsets, as well as thymic epithelial cells, suggesting a role for DO in mediating central tolerance. In a mouse model lacking DO, we show that selection of T regulatory cells (Tregs) is increased and that DO- deficient Tregs are more activated and exert greater suppressive capacity. Despite augmented Treg function, mice lacking DO display enhanced susceptibility to autoimmunity, with altered germinal center (GC) Tregs and B cells indicative of an aberrant GC reaction. These data suggest that DO expression serves to fine-tune the immunopeptidome in order to promote self-tolerance to a wide spectrum of epitopes and to select a Treg population with appropriate specificity for self- antigens.

The fact that hydrogen is a clean and versatile fuel offers an attractive carbon-free source of energy and leverages the U.S. economy toward long-term sustainable economic growth. At an industrial scale, hydrogen production is mostly relying on methane steam reforming producing stoichiometric amounts of carbon oxides (CO and CO2), which imposes economic and environmental concerns. To mitigate the issue, we propose NH3 assisted anaerobic reforming of natural gas liquids (ethane and propane) as an alternative approach to produce COx free hydrogen. Here, in the first chapter, through comprehensive performance evaluation, characterization, and transient kinetic studies, it is shown that the atomically dispersed Re-oxo grafted into framework Al of the HZSM-5 zeolite are highly active and stable for the ammonia reforming of ethane and propane at temperatures comparable to steam reforming ≤ 650 °C. In the second chapter, an alternative non- noble Ni/Ga intermetallic compound (IMC) with various Ni to Ga ratios is synthesized through the solvothermal synthesis by forming the oxalate MOF precursor. The result indicates that while Ni-rich samples form pure Ni3Ga IMC with promising catalytic performance, the Ga rich catalyst consists of segregated phases of Ni/Ga IMC and Ga2O3 with ill-defined structure showing lower stability despite the high activity. In chapter 3, a bifunctional Ni/Ga supported ZSM-5 is successfully developed in ethane aromatization. Influence of metal function in early-stage and steady-state activity and stability as well as structure reactivity relation was investigated applying comprehensive characterization, performance test, deactivation modeling, and transient studies. The results suggest that a tandem reaction mechanism between Ni3Ga intermetallic compound, Ga cation, and Bronsted acid sites of zeolite is responsible for the superior performance of bimetallic catalysts compared to their monometallic counterpart. In the last chapter, applying transient kinetic technique, the mechanism of ethane aromatization over Pt and Zn supported ZSM-5 model catalysts was precisely explored. The results reveal that despite mechanistic differences between these catalysts, ethane amortization on both catalysts follows a hydrocarbon pool mechanism.