Our work falls within the field of high resolution spectroscopy of gas phase molecules in the far-, mid- and near-infrared ranges. Its guiding line are absorption spectral intensities, dealt with experimentally and theoretically. In particular, we developed in our laboratory the field of intensities measurements of vibration-rotation lines using Fourier transform spectrometers, with a precision of about 0.5 % and an accuracy of 2-4 % for chemically stable species. We study chemically stable (CO2, N2O, C2H6, OCS, C2H2) and unstable (HOCl, HCOOH et HNO3) compounds. We also measure infrared absorption cross section spectra for CFC replacements. Some of our measured intensities, of direct interest for the study of planetary atmospheres, are now incorporated in international spectroscopic databases. Others are used to develop global theoretical models of molecules, in relationship with intra-molecular dynamics./Nos travaux de recherches relèvent de la spectroscopie à haute résolution de molécules en phase gazeuse dans les domaines de l’infrarouge lointain, moyen et proche. Ils ont pour ligne directrice les intensités spectrales d’absorption, abordées expérimentalement et théoriquement. Nous avons en particulier développé dans notre laboratoire le domaine de la mesure d’intensités d’absorption de raies de vibration-rotation à l’aide de spectromètres à transformée de Fourier. Nous réalisons ces mesures avec une précision d’environ 0.5 % et une exactitude d'environ 2-4 % pour les espèces chimiquement stables. Nous étudions des composés chimiquement stables (CO2, N2O, C2H6, OCS, C2H2) et instables (HOCl, HCOOH et HNO3). Nous mesurons également des spectres de sections efficaces d’absorption infrarouge pour des substituts des chlorofluorocarbures (CFC). Certaines de nos mesures d’intensité, d’intérêt direct pour l’étude d’atmosphères planétaires, sont aujourd’hui incorporées dans les bases de données spectroscopiques internationales. D’autres sont utilisées pour développer des modèles théoriques globaux de molécules, en liaison avec la dynamique intramoléculaire. / Agrégation de l'enseignement supérieur, Orientation sciences / info:eu-repo/semantics/nonPublished

The electronic and magnetic structure of the colossal magneto resistance material La1-xSrxMnO3, the high-k and strain tailoring compounds REScO3 (Sm, Gd, Dy) and the multiferroic LuFe2O4 was investigated by means of x-ray spectroscopic techniques. SQUID measurements of La1-xSrxMnO3 (x = 0.125, 0.17, 0.36) were compared with XMCD results. The very good agreement between these two experiments proofs the applicability of the correction factor for the spin magnetic moment and the importance of charge transfer. The magnetic moment measured by SQUID and that determined from XMCD proofs that the magnetic moment is completely localized at the Mn ions for different temperatures and magnetic fields. For x = 0.125 the orbital magnetic moment determined from XMCD corresponds to the structural changes in the phase diagram. Additionally the measured orbital moments correspond to anomalies in magnetization versus temperature curves. The magnetic and electronic structure of the rare earth scandates (SmScO3, GdScO3 and DyScO3) were investigated by means of XPS, XES, XAS, SQUID and neutron powder diffraction. The magnetic measurements reveal antiferromagnetic coupling at low temperatures in agreement with neutron diffraction data. With XAS and XES at the O K-edge in comparison with band structure calculations of the unoccupied oxygen states, the band gaps of REScO3 were determined and it was found that these values are corresponding to the Sc-O mean distances. The electronic and magnetic structure of LuFe2O4 was presented. The valence state of Fe ions was determined to 50% divalent and 50% trivalent by XPS of Fe 2p and 3s levels. The big orbital magnetic moment found by XMCD could explain a discrepancy between the magnetic measurements and the spin configuration, which was confirmed by XMCD.

Les molécules aromatiques protonées jouent un rôle important dans les réactions de substitution électrophile aromatique, et dans différents processus biologiques. Ces molécules sont présentes aussi dans d’autres milieux tels que les flammes de combustion, les plasmas de divers hydrocarbures, les ionosphères planétaires (Titan) et le milieu interstellaire. Les molécules protonées sont très stables car elles ont des couches électroniques complètes mais elles sont en général très sensibles à leur environnement local car elles sont chargées : une étude en phase gazeuse est nécessaire pour déterminer leurs propriétés intrinsèques. Jusqu’à présent, très peu de chose était connu sur les molécules protonées isolées en phase gazeuse, seulement quelques résultats étaient disponibles. Ce manque de données venait de la difficulté de générer des molécules protonées en phase gazeuse et surtout de les produire à basse température (la protonation est une réaction exothermique). Récemment, des progrès ont permis d’étudier les molécules protonées en phase gazeuse à très basse température, en particulier par le développement des sources ioniques couplées avec des techniques d'expansion de jet supersonique. Grâce à cette technique on a enregistré le spectre photo fragmentation de l’état fondamental vers le premier état excité (S1←S0) de différentes molécules aromatiques protonées en phase gazeuse. Les molécules que nous avons étudiées peuvent être regroupées en quatre familles : Les molécules polycycliques aromatiques protonées linéaires (benzène, naphtalène, anthracène, tétracène, pentacène). Les molécules polycycliques aromatiques protonées non linéaires (fluorène, phénanthrène, pyrène). Les molécules protonées contenant un hétéro atome (benzaldéhyde, salicylaldéhyde, 1-naphthol et 2-naphthol, indole, aniline). Les agrégats protonés (dimère de benzène, naphtalène (H2O)n, n=1,2,3. naphtalène (NH3)n, n=1,2,3, benzaldéhyde (Ar , N2)). Dans les spectres enregistrés presque toutes les transitions électroniques S1←S0 sont décalées vers le rouge (basse énergie) par rapport à celui des molécules parentes neutres. Ce décalage est dû au caractère transfert de charge du premier état excité. Certains spectres sont résolus vibrationnellement, alors que pour d'autres molécules le spectre ne présente pas de progression vibrationnelle à cause d’un dynamique très rapide de l’état excité menant par des intersections coniques à l’état fondamental. Les spectres d’absorption des molécules protonées sont plus riches en vibrations par comparaison avec les molécules neutre. Cela reflète le changement relativement important de géométrie de l’état excité dû à son caractère transfert de charge. Les résultats expérimentaux ont été complétés par des calculs ab-initio qui ont permis de localiser la transition électronique, déterminer la structure géométrique et électronique, les modes de vibration et, pour certaines de ces molécules, la dynamique de l’état excité. Les calculs sont en général en très bon accord avec les expériences. / Protonated aromatic molecules play an important role in electrophilic aromatic substitution reactions, fundamental reactions in organic chemistry and in various biological processes. The interstellar medium is another environment which is likely to contain the protonated aromatic molecules, that’s because these molecules are stable chemically since they are close shell electronic structure. These molecules were also identified in others environments such as combustion flames, plasmas of various hydrocarbons and the upper atmosphere of Titan. Protonated molecules are usually very sensitive to their local environment; a gas phase study is required to determine their intrinsic properties. Until now, very little is known about the isolated protonated molecules, only a few results are available in the literature. This lack of data is due to the difficulties of the production and the cooling of these molecules in gas phase. The technical progress we have done has enabled the study of protonated molecules in the gas phase at very low temperatures, using an ion sources, supersonic jet and the laser induced photofragmentation techniques. Using this technique, we have recorded many electronic spectra (S1←S0) of different protonated molecules. We can regroup the studied molecules into four: Linear protonated polycyclic aromatic molecules (benzene, naphthalene, anthracene, tetracene, pentacene). Nonlinear protonated polycyclic aromatic molecules (fluorene, phenanthrene, pyrene). Protonated molecules containing an hetero atom (benzaldehyde, salicylaldehyde, 1-naphthol and 2-naphthol, indole, aniline). Protonated cluster (dimer of benzene, naphthalene (H2O)n, n = 1,2,3. Naphthalene (NH3)n, n = 1,2,3, benzaldehyde (Ar, N2)). Most of those spectra are red-shifted compare to the spectrums of neutral parent molecules. This red-shift is due to charge transfer character of the first excited state. Some spectra are vibrationally resolved, while for other molecules the spectrum do not shows any vibrational progression. This behaviour is explained by the dynamic of the excited state, this dynamic being usually is very fast, sometimes leading to the ground state through a conical intersection. The spectra of protonated molecules are very active vibrationally in comparison with neutral molecules, many vibrational modes forbidden for neutral molecule becomes active for the protonated one (Franck-Condon factor is not zero). This is reflecting the charge transfer character of the excited state. The experimental results were complemented by ab-initio calculations, which have allowed determining the electronic transition, the geometric and electronic structure of the molecule, the vibrational modes, and for some of these molecules the dynamics of excited state. Calculations are generally in very good agreement with experiments.

Chapter 1.<br />1-Ethynyl-2-phenyltetramethyldisilanes HCºCSiMe2SiMe2C6H4-p-X [X = NMe2(1.1), Me (1.2), H (1.3), Br (1.4), CF3 (1.5)] are accessible from ClSiMe2SiMe2Cl, BrMgC6H4X and HCºCMgBr in a two step Grignard reaction. The crystal structure of 1.1 as determined by single crystal X-ray crystallography exhibits a nearly planar PhNMe2 moiety and an unusual gauche array of the phenyl and the acetylene group with respect to rotation around the Si-Si-bond. Full geometry optimization (B3LYP/6- 31+G**) of the gas phase structures of 1.1 and 1.3 affords minima for the gauche and the trans rotational isomers, both being very close in energy with a rotational barrier of only 3 – 5 kJ/mol. Experimental and calculated (time-dependent DFT B3LYP/TZVP) UV absorption data of 1.1 – 1.5 show pronounced electronic interactions of the HCºC- and the C6H4X p-systems with the central Si-Si bond.<br /><br />Chapter 2.<br />A family of [( 5-Cp*)Ru( 6-arene)]+ (Cp* = C5Me5) sandwich complexes of 1- and 1,4-substituted phenyl and naphthyl systems are described along with the regioselectivities of the reactions under various conditions. Finally, the (h 5-Cp*) Ru+ arenophile was found to act as a gate to the flow of electrons between para-substituted termini. When it is complexed onto the phenyl or A naphthyl ring, the gate is closed. On the contrary, when it is complexed onto the B naphthyl ring, the gate is open.<br /><br />Chapter 3.<br />Regioselective complexation reactions of the organoiron acetylide derivatives (h 2- dppe)(h 5-Cp*)Fe-C C-Ar (Ar = phenyl, 1-naphthyl; dppe = 1,2- bis(diphenylphosphino)ethane) with [(h 5-Cp*Ru(CH3CN)3][PF6] to afford heterobimetallic complexes formulated as [(h 2-dppe)(h 5-Cp*)Fe-C C-{(h 6-Ar)Ru(h 5- Cp*)}][PF6], were achieved. In the case of the FeII-RuII 1-naphthyl derivative, the (h 5-Cp*)Ru+ arenophile was complexed both onto the substituted ring and free rings of the acetylide 1-naphthyl linker. The first redox-driven h 6-h 6 inter-ring haptotropic migration of the (h 5-Cp*)Ru+ moeity was shown to occur. Crystal structures of all of the seven new iron acetylenes were resolved, including both haptotropomers of the naphthyl compound.<br /><br />Chapter 4.<br />The diorganoiron [{(h2-dpppe)(h5-Cp*)Fe-CC-}2(1,4-naphthyl)] (4.12) was synthesized in good yield in two steps via the vinylidene, and oxidation led to the mixed valence (MV) and iron(III)-iron(III) species in good to excellent yields. This exhaustive empirical study on the family of complexes 4.12[PF6]n (n = 0,1,2) includes a crystal structure for the case in which n = 2. This work clearly establishes good electronic and magnetic communication between the iron centers across the bis(ethynyl)naphthalene bridge. All empirical measurements of these naphthyl compounds reveal that their properties fall between those of known phenyl and anthracenyl derivatives. In some cases, the naphthyl derivative behaves as an average of the phenyl and anthracenyl complexes. For example, the comproportionation constant of the naphthyl species falls at the midpoint between those for the phenyl and anthracenyl compounds. The same is true for the UV absorption maxima in all three oxidation states (Fe[II]- Fe[II], MV, and Fe[III]- Fe[III]). The large electronic (2043 cm-1) and magnetic (-526 cm-1) coupling constants were determined via NIR spectroscopy and SQUID magnetometry, respectively. As for the heterotrinuclear species, the iron(II) acetylene, 4.14B[PF6] [{Cp*(dppe)Fe-C C}2-(h 6 – [1,4-napthyl])RuCp*](PF6), [Cp* = h 5 - C5Me5; Fe = FeII] was prepared in high yields with an adapted, regioselective synthesis via the trinuclear vinylidene. Complete characterization, including a crystal structure, of this sandwich complex reveals that the arenophile perturbs the organoiron ligand more in the bis(iron) than in the previously reported mono(iron) case.

No description available.

The role of clusters in planetary atmospheres and the interstellar medium is potentially important. Investigating such a role requires basic experimental information, however lacking. The goal of this thesis was to develop an efficient experimental set-up to produce clusters in the laboratory in concentrations large enough to allow their high resolution spectra to be recorded, thus providing the necessary data allowing the physico-chemical properties of the clusters to be studied.<p>The study of this subject however suffers from the lack of basic experimental data. The goal is therefore to produce clusters in the laboratory in concentration large enough to record their high resolution spectrum. This is the initial aim of the present thesis.<p>During this work, we have built and extensively tested a new experimental set-up called FANTASIO (``Fourier trANsform, Tunable diode and quadrupole mAss spectrometers interfaced to a Supersonic expansIOn'). With the help of this new device, various experiments on jet-cooled species have been performed.<p>The cartography of the supersonic expansion was established, using the mass spectrometer as a moving pressure probe. This enabled us to characterize the geometrical properties of the supersonic jet produced by circular and slit nozzles and to determine the position of the virtual nozzle. The effect of the axisymmetric expansion geometry on the R(0) lineshape in the nu_3 band of N_2O, recorded by FTIR, was also investigated.<p>The rotational temperature of the jet-cooled molecules was determined to be a few K by measuring the intensity of lines in spectra recorded by FTIR spectroscopy.<p>Vibrational energy transfer occuring in the expansion between N_2O molecules and different collision partners was investigated on the nu_2+nu_3-nu_2 band of N_2O, again using FTIR spectroscopy. The trend of these transfers was found to be related to the energy difference between the v_2=1 level of N_2O and the closest vibrational state in the collision partner, with the largest population.<p>The sensitivity of the set-up was enhanced by a factor of 5 by increasing the absorption path length, using a multipass system. A procedure to remove the residual gas contribution from the IR spectra was developped, based on the mass spectrometer. Thanks to this sensitivity increase, broadband absorption features of clusters were observed for a C_2H_2-Ar mixture in circular and slit expansions.<p>The optical sensitivity of FANTASIO was again increased by the implementation of the CW-CRDS system. The enhancement over FTIR was calculated to be over a factor 750. Thanks to this drastic improvement, spectral signatures of various clusters were recorded, such as C_2H_2-Ar, C_2H_2 multimers, C_2H_2-N_2O and C_2H_2-CO_2, at high resolution.<p>The role of clustering in generating unusual line shapes of acetylene in an axisymmetric expansion was investigated. We demonstrated that C_2H_2 aggregates produced in the expansion are responsible for central dips observed in the monomer absorption. These acetylene clusters thus appear to be formed in the centre of the expansion, while, unexpectedly, acetylene-Ar complexes are formed at the edge of the conical expansion.<p>Various research prospects were explored during this thesis thanks to the FANTASIO device, opening new research directions. FANTASIO is today operational and defines a useful tool to achieve the study of small clusters by infrared spectroscopy./<p><p>Le rôle des agrégats dans les atmosphères planétaires et dans le milieu interstellaire est potentiellement important. Cependant, les études sur ce sujet souffrent du manque de données expérimentales. Le but de cette thèse était de développer un dispositif expérimental efficace pour produire au laboratoire des agrégats en quantité suffisante pour permettre l'enregistrement de leur spectre infrarouge à haute résolution et donc l'étude de leurs propriétés physico-chimiques.<p>Durant ce travail, nous avons construit et testé un nouveau dispositif expérimental appelé FANTASIO, basé sur un jet supersonique couplé à un spectromètre de masse, un spectromètre à transformée de Fourier et un système CRDS. Grâce à cet appareillage, différentes expériences sur des molécules à basse température ont été menées.<p>L'expansion supersonique a été cartographiée en utilisant le spectromètre de masse comme une sonde de pression mobile. Cette cartographie nous a permis d'établir les propriétés géométriques des jets supersoniques produits par les orifices circulaire et de type fente, et de déterminer la position de l'orifice virtuel. L'effet de la géométrie de l'expansion sphérique sur le profil de la raie R(0) de la bande nu_3 de N_2O, enregistré par FTIR, a aussi été étudié.<p>Une température rotationnelle de quelques K a été déterminée pour les molécules refroidies en jet supersonique par mesure de la distribution d'intensité de raies dans les spectres enregistrés par FTIR.<p>Le transfert d'énergie vibrationnelle entre des molécules de N_2O et différents partenaires collisionnels a été étudié en analysant l'intensité de la bande nu_2+nu_3-nu_2 de N_2O, enregistré également par spectroscopie FTIR. Il a été trouvé que la tendance de ces transferts est liée à la différence d'énergie entre le niveau v_2=1 de N_2O et l'état vibrationnel le plus proche et le plus peuplé du partenaire collisionnel.<p>La sensibilité du dispositif a été augmentée d'un facteur 5 dû à l'allongement du chemin d'absorption, grâce à l'utilisation d'un système multipassage. Une procédure basée sur l'utilisation du spectromètre de masse et visant à enlever la contribution du gaz chaud résiduel dans les spectres infrarouges a été mise au point. Grâce à cette augmentation de sensibilité, des structures d'absorption non résolues d'agrégats ont été observées dans des expansions en trou et en fente d'un mélange de C_2H_2-Ar.<p>La sensibilité optique de FANTASIO a encore été augmentée par l'ajout au dispositif d'un système CW-CRDS. L'amélioration par rapport au spectromètre à transformée de Fourier a été calculée comme étant supérieure à un facteur 750. Grâce à cette importante amélioration, les signatures spectrales de divers agrégats, tels que C_2H_2-Ar, des multimères de C_2H_2, C_2H_2-N_2O et C_2H_2-CO_2, ont été enregistrées à haute résolution.<p>Le rôle de l'agrégation dans la génération de profils de raie inhabituels dans une expansion en trou de l'acétylène a été étudié. Nous avons démontré que les agrégats de C_2H_2 produits dans le jet supersonique sont responsables des creux observés dans le profil d'absorption du monomère. Ces agrégats apparaissent donc comme étant formés au centre de l'expansion, tandis que, de manière inattendue, les agrégats de C_2H_2-Ar sont formés aux bords de l'expansion conique.<p>Plusieurs idées de recherche ont été explorées durant cette thèse grâce au dispositif FANTASIO, ouvrant de nouvelles directions de recherche. FANTASIO est aujourd'hui opérationnel et se présente comme un outil utile dans l'étude des petits agrégats par spectroscopie infrarouge. / Doctorat en Sciences / info:eu-repo/semantics/nonPublished

In forensic chemistry, a quicker and more accurate analysis of a sample is always being pursued. Speedy analyses allow the analyst to provide quick turn-around times and potentially decrease back-logs that are known to be a problem in the field. Accurate analyses are paramount with the futures and lives of the accused potentially on the line. One of the most common methods of analysis in forensic chemistry laboratories is gas chromatography, chosen for the relative speed and efficiency afforded by this method. Two major routes were attempted to further improve on gas chromatography applications in forensic chemistry.<br> The first route was to decrease separation times for analysis of ignitable liquid residues by using micro-bore wall coated open-tubular columns. Micro-bore columns are much shorter and have higher separation efficiencies than the standard columns used in forensic chemistry, allowing for faster analysis times while maintaining the expected peak separation. Typical separation times for fire debris samples are between thirty minutes and one hour, the micro-bore columns were able to achieve equivalent performance in three minutes. The reduction in analysis time was demonstrated by analysis of ignitable liquid residues from simulated fire debris exemplars.<br> The second route looked at a relatively new detector for gas chromatography known as a vacuum ultraviolet (VUV) spectrophotometer. The VUV detector uses traditional UV and far-ultraviolet light to probe the pi and sigma bonds of the gas phase analytes as well as Rydberg traditions to produce spectra that are nearly unique to a compound. Thus far, the only spectra that were not discernable were from enantiomers, otherwise even diastereomers have been differentiated. The specificity attained with the VUV detector has achieved differentiation of compounds that mass spectrometry, the most common detection method for chromatography in forensic chemistry labs, has difficulty distinguishing. This specificity has been demonstrated herein by analyzing various classes of drugs of abuse and applicability to “real world” samples has been demonstrated by analysis of de-identified seized samples.<br>

In this diploma thesis, SERRS(Surface - enhanced resonance Raman Scattering) and SERS (Surface - enhanced Raman Scattering), surface of plasmon extinction spectra and TEM images of systems with tetracationic zinc porphyrin ZnTMPyP and silver nanoparticles (Ag NPs) were studied and interpreted. The systems with isolated nanoparticles and the systems with compact aggregates were investigated. The systems with isolated nanoparticles were prepared by addition of ZnTMPyP to hydrosol of Ag NPs. NaCl was added to this system and so compact aggregates were prepared. SERRS and SERS spectra of ZnTMPyP were studied at excitation wavelengths λexc= 441.6 nm a 532 nm. Firstly, stationary systems and secondly dynamic development of hydrosol Ag NPs → Ag NPs/ ZnTMPyP → Ag NPs/ ZnTMPyP/ NaCl systems for 680 s was investigated. Time evolution of SERRS and SERS spectra were analyzed by factor analysis (FA) and time evolution of spectra extinction plasmon were measured. FA showed a strong increase of the signal of ZnTMPyP after the addition of NaCl, i.e. after conversion of isolated nanoparticles to compact aggregates. In these systems with high concentration of ZnTMPyP the increase of signal was succeeded by its decreased. With help of FA the limit of SERRS spectral detection (λexc= 441,6 nm) and limit of SERS spectral...

Oxidische Materialien bieten ein weites Spektrum an möglichen Anwendungen. Vor allem Isolatoren mit Perowskitstruktur eignen sich hervorragend für die optische Datenverarbeitung und -speicherung. Andere, leitende, Oxide können für die magnetische Datenspeicherung eingesetzt werden. Vorraussetzung für den praktischen Einsatz der Werkstoffe sind jedoch grundlegende Kenntnisse über deren mikroskopischen Eigenschaften und ablaufende Prozesse. Mittels Photoelektronen- und Röntgenspektroskopie können Aussagen über die elektronische Struktur getroffen werden. Die noch junge Methode der Fluoreszenz weicher Röntgenstrahlung (SXF) wurde zur Charakterisierung der elektronischen Struktur hinzugezogen. SXF-Messungen wurden an der Beamline 8.0.1 am ALS in Berkeley, Kalifornien, durchgeführt. An der Modellsubstanz MgO wurden Röntgenabsorptions- und Röntgenemissionsspektren an der Sauerstoffkante erstellt. Es zeigt sich eine hervorragende Übereinstimmung mit Modellrechnungen. Ein Bandmapping unter Ausnutzung von Resonanzphänomenen, ähnlich wie in Graphit, scheint jedoch nicht möglich zu sein. In TiO2 wurde das Ti 3d Niveau untersucht. Die Emissionsspetkren zeigen Verluststrukturen, deren Feinstruktur mit der berechneten rJDOS nachvollzogen werden konnte. In KNbO3 wurde der Beitrag der Nb 5p und O 2p-Zustandsdichte zum Valenzband untersucht. Es wurde versucht, die Anregungsenergieabhängigkeit der O 2p-Emissionsspektren mit der Bandstruktur in Verbindung zu bringen. In KTaO3 wurde erstmals der Ta 5d-pDOS-Anteil am Valenzband direkt nachgewiesen. Zudem weisen die anregungsenergieabhängigen Emissionsspektren Verluststrukturen auf, die auf eine O 2p-Ta 5d Interbandanregung schließen lassen. An Sr2FeMoO6 wurden erstmals XES-Messungen zur Bestimmung der elektronischen Struktur durchgeführt. Es zeigen sich hybridisierte O 2p-Mo 4d Zustände, die Leitungselektronen haben einen leichten Fe-Charakter. Eine gute Übereinstimmung mit Bandstrukturrechnungen wird beobachtet. Für photorefraktive Material Sn2P2S6 wurde die elektronische Struktur mittels XPS, XES und FP-LAW-Rechnungen detailliert bestimmt. An Fe-dotiertem Ba0.77Ca0.23TiO3 wurde mittels XPD unter erstmaliger Erstellung von Azimuthalspektren der Einbauplatz von Ca verifiziert und der Einbauplatz von Eisen bestimmt. Für beide Elemente ergibt sich ein vollständiger bzw. überwiegender Einbau auf dem Ba-Platz.

Quasi-particles formed in lithium niobate after pulse exposure were investigated by transient absorption and photoluminescence spectroscopy as well as numerical simulations. This includes the formation process, the transport through the crystal, interim pinning on defects during the relaxation process, and the final recombination with deep centers. It was shown that the charge-transport through the crystal can be described by a hopping transport including different types of hops between regular or defective lattice sites, i.e., the transport includes a mixture of free and bound small polarons. Furthermore, the different types of hops connected with varying activation energies and their distribution are responsible for an altered temporal decay curve when changing the crystal composition or temperature. Additionally, it was shown that the hitherto accepted recombination model is insufficient to describe all transient absorption and luminescence effects in lithium niobate under certain experimental conditions, i.e., long-living absorption dynamics in the blue/UV spectral range do not follow the typical polaron dynamics and cannot be described under the assumption of charge compensation. However, similar decay characteristics between self-trapped excitons known from photoluminescence spectroscopy and the unexpected behavior of the transient absorption were found leading to a revised model. This includes, besides the known polaron relaxation and recombination branch, a significant role of self-trapped excitons and their pinning on defects (pinned STEs). Since the consideration of further absorption centers in the relaxation path after pulse exposure might result in misinterpretations of previously determined polaron absorption cross-sections and shapes, the necessity to perform a review became apparent. Therefore, a supercontinuum pump-probe experiment was designed and all measurements applied under the same experimental conditions (temperature, polarization) so that one can extract the absorption amplitudes of the single quasi-particles in a spectral range of 0.7-3.0eV. The detailed knowledge might be used to deconvolve the absorption spectra and transform them to number densities of the involved centers which enables one to obtain an easier insight into recombination and decay dynamics of small polarons and self-trapped excitons. As the hopping transport of quasi-particles and the concept of pinned STEs might be fundamental processes, a thorough understanding opens up the possibility of their exploitation in various materials. In particular, results presented herein are not only limited to lithium niobate and its applications; an extension to a wide range of further strongly polar crystals in both their microscopic processes and their use in industry can be considered.