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Philosophiae Doctor - PhD / Low- and medium-spin bands of 187Os have been studied using the AFRODITE array, following the 186W(4He,3n)187Os reaction at a beam energy of 37 MeV. The measurements of 􀀀 coincidences, angular distribution ratios (RAD), polarization and -intensities were performed using eleven High Purity Germanium (HPGe) clover detectors. In the current work, all the previously known bands have been signi cantly extended and ve new bands have been added to the level scheme. The observed bands are interpreted within the cranked shell model (CSM), cranked Nilsson-Strutinsky- Bogoliubov (CNSB) formalism and Quasiparticle-plus-Triaxial-Rotor (QTR) model. Systematic comparison of bands with the neighbouring isotopes has also been made. Comparison of the models with experimental data shows good agreement.

Philosophiae Doctor - PhD / Lying in a rapidly-changing transitional region between nuclei that may behave as spherical vibrators (N ≤ 88) or good rotors (N ≥ 92), the N = 90 isotones present a unique testing ground where new nuclear collective phenomena may be uncovered. As part of a general investigation of collective structures and the coupling of single-particle states to these structures, the 150Sm(12C,4nγγ) and 150Sm(13C,4nγγ) reactions at a beam energy of Elab = 65 MeV were used to study the low and medium spin structure of 158,159Er nuclei below spin 20~. The γ-γ coincidence events were detected in the nine escape-suppressed HPGe Clover detectors using the AFRODITE γ-ray spectrometer at the iThemba Laboratory for Accelerator Based Sciences. DCO ratios and γ-ray polarization measurements were used to establish the spins and parities of newly observed and confirm previously established rotational bands. The observed bands will be discussed in terms of both traditional quadrupole rotational-vibration models and recent predictions of octupole correlations in the N = 90 isotones and neighbouring nuclei. The data obtained will be compared with the spectroscopic systematics of neighbouring nuclei.

Philosophiae Doctor - PhD / Low- and medium-spin bands of 187Os have been studied using the AFRODITE array, following the 186W(4He,3n)187Os reaction at a beam energy of 37 MeV. The measurements of γ − γ coincidences, angular distribution ratios (RAD), polarization and γ-intensities were performed using eleven High Purity Germanium (HPGe) clover detectors. In the current work, all the previously known bands have been significantly extended and five new bands have been added to the level scheme. The observed bands are interpreted within the cranked shell model (CSM), cranked Nilsson-StrutinskyBogoliubov (CNSB) formalism and Quasiparticle-plus-Triaxial-Rotor (QTR) model. Systematic comparison of bands with the neighbouring isotopes has also been made. Comparison of the models with experimental data shows good agreement. The configurations of some of the previously observed bands have been modified. Most importantly, the coupling of 2+ γ band to the 11/2+[615] neutron configuration is observed for the first time.

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Submitted by Edileide Reis (leyde-landy@hotmail.com) on 2013-04-23T14:35:12Z No. of bitstreams: 1 Yuji Watanabe.pdf: 3696013 bytes, checksum: 64d732d452c08c675e78db3f991bf851 (MD5) / Made available in DSpace on 2013-04-23T14:35:12Z (GMT). No. of bitstreams: 1 Yuji Watanabe.pdf: 3696013 bytes, checksum: 64d732d452c08c675e78db3f991bf851 (MD5) Previous issue date: 2002 / Este trabalho é constituído de três etapas, a saber: · planejamento e construção de um aparato experimental para medidas de fluorescência total (LIF) e depolarização fluorescente (PLF) em sistema de injeção em fluxo (FI); testes operacionais visando otimizar parâmetros experimentais; avaliação fotoquímica/fotofísica da cinética e dinâmica molecular duma reação química em FI. O aparato experimental automatizado é constituído de um sistema de detecção de fluorescência, um sistema FI e um sistema ótico. Permite a aquisição com alta resolução espacial (20mm) de perfis de distribuição de concentração (LIF) e de orientação molecular vertical e horizontal (PLF) em função do tempo de transporte do fluxo. Os perfis interpolados em mapas bidimensionais fornecem informações sobre a cinética e a dinâmica molecular dos processos de dispersão axial e radial de amostras em fluxo carregador. Foram medidas tensões interfaciais estáticas, pelo método do ângulo de contato, para escolher a constituição química do percurso analítico e minimizar a sua influência na cinética e na dinâmica molecular de dispersão. Foi determinada a influência da aceleração gravitacional e do número de injeções por período de amostragem, dentre outros parâmetros usuais, no processo de dispersão.Observou-se a existência de padrões de dispersão diferenciados para a Rodamina B (RB) a depender da sua orientação espacial. Isto foi atribuído ao grupo benzóico perpendicular ao grupo xantênico e comprovado pela utilização da Rodamina 6G (R6G) sob as mesmas condições. A contribuição da cinética e da dinâmica moleculares de dispersão no rendimento de uma reaçãoquímica em fluxo foi avaliado com adição de Ca(II), um agente supressor da fluorescência da RB. / Salvador

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Diese Arbeit befasst sich mit den optischen Eigenschaften von dünnen GaN-Schichten gewachsen in verschiedenen Orientierungen. Hierbei werden die optischen Eigenschaften von verspannten M- und A-plane sowie unverspannten C-plane GaN-Schichten untersucht und die Ergebnisse im Rahmen von Bandstrukturberechnungen diskutiert. Im Rahmen dieser Arbeit werden die Bandstrukturverschiebungen theoretisch mittels eines k.p-Näherungsansatzes untersucht. Diese Bandverschiebungen beeinflussen sowohl die Übergangsenergien als auch die Oszillatorstärken. Man findet, dass die C-plane Schicht im Falle einer isotropen Verspannung in der Filmebene keine Anisotropie der optischen Polarisation zeigt. In beiden Fällen zeigen die drei Übergänge von den drei oberen Valenzbändern in das untere Leitungsband andere Polarisationseigenschaften als die entsprechenden Übergänge in C-plane GaN-Schichten. Es wird beobachtet, dass für einen bestimmten Wertebereich der Verspannung in der Filmebene diese Übergänge nahezu vollständig x-,z- bzw. y-artig polarisiert sind. Die verwendeten Schichten wurden auch mittels Transmissionspektroskopie untersucht. Im Falle der M-plane GaN-Schichten können zwei fundamentale Übergänge identifiziert werden, wobei der elektrische Feldvektor E des einfallenden Lichtes einmal parallel (z-Polarisation) und einmal senkrecht (x-Polarisation) auf der c-Achse steht. Die M-plane GaN-Schicht besitzt unterschiedliche Dielektrizitätskonstanten für z-Polarisation und x-Polarisation, welche zu zusätzlichem Dichroismus und Doppelbrechung führen. Als Resultat findet eine Filterung der Polarisation für einfallendes, linear polarisiertes Licht statt. Die elektrische Feldkomponente mit x-Polarisation wird stärker absorbiert als die Komponente mit z-Polarisation. Diese Polarisationsfilterung äußert sich für schmalbandiges Licht in Form einer Drehung der Polarisationsebene in Richtung der c-Achse, wobei ein maximaler Rotationswinkel von 40 Grad gefunden wurde. / In this work, we focus on the optical response of GaN thin films grown along various orientations. The optical properties of strained M- and A- and unstrained C-plane GaN thin films are investigated, and the results are explained with help of band-structure calculations. We calculate the strain-induced band-structure modification using the k.p perturbation approach. The valence-band (VB) states are modified affecting both the transition energies as well as the oscillator strengths. We observe that C-plane GaN does not show any in-plane polarization anisotropy, when an isotropic in-plane strain is applied. For the case of M- and A-plane GaN, one expects to see an in-plane polarization anisotropy even for the unstrained case. Additionally, the in-plane strain significantly changes the band structure and the symmetry of the VB states. The three transitions, involving electrons in the conduction band (CB) and holes in the top three VBs, will exhibit a very different polarization characteristic than the ones for C-plane GaN. These transitions are predominantly x, z, and y polarized, respectively, for a certain range of in-plane strain values, present in our samples. For M-plane GaN thin films, two fundamental transitions can be identified, which occur when the electric field vector E is perpendicular (x-polarization) and parallel c (z-polarization). These transitions give rise to a transmittance spectrum separated by 50 meV at room temperature with respect to each other. This result in a polarization filtering of an incident linearly polarized light beam after transmission, because the electric field component with x-polarization is more strongly absorbed than with z-polarization. This filtering manifests as a rotation of the polarization vector toward the c axis and can be as large as 40 degrees for an initial angle of 60 degrees, for our samples.

Depuis sa découverte en 1964, l’étude du Fond Diffus Cosmologique dans le domaine des longueurs d’ondes millimétriques est devenue un enjeu majeur de la recherche expérimentale dans le domaine de la cosmologie. En particulier, ses anisotropies en température, mesurées pour la première fois par le satellite COBE puis plus finement par l’expérience WMAP et le satellite PLANCK. L’existence prédite d’anisotropies de polarisation du Fond Diffus Cosmologique est fait actuellement parti du champ d’expérimentation privilégié de l’étude du CMB. En effet, la preuve d’existence des modes B de polarisation, signature unique des ondes gravitationnelles primordiales, fait actuellement l’objet d’une recherche expérimentale intensive par le biais notamment de l’instrument BICEP2 qui aurait détecté sa signature en 2014 dans des valeurs du rapport tenseur sur scalaire r = 0,2. Le projet QUBIC fait parti de ces expériences destinées à révéler les modes B de polarisation grâce à son instrument basé sur la technique des interféromètres et sur le développement de matrice de bolomètres, demandant un champ d’investigation poussé englobant, entre autre, la physique des solides, la physique des basses températures et la cosmologie. La thèse présentée ici se situe dans ce cadre, avec pour objectif l’élaboration d’une matrice de bolomètres dont la performance et l’optimisation devrait permettre d’acquérir la sensibilité nécessaire à l’observation des modes B de polarisation. Les différentes techniques expérimentales acquises au CSNSM d’Orsay permettent en effet d’envisager l’optimisation des éléments clé de la matrice de bolomètre en s’appuyant notamment sur l’alliage amorphe de NbxSi1-x pour l’élaboration d’un senseur thermique optimisé, et sur un matériau novateur, l’alliage de titane-vanadium, pour la mise au point d’un absorbeur de rayonnement supraconducteur efficace, dont la faible chaleur spécifique doit permettre d’atteindre un temps de réponse du détecteur de l’ordre de la dizaine de milliseconde, valeur du temps de réponse nécessaire à une lecture efficace du signal du Fond Diffus Cosmologique. Le manuscrit de thèse ici présent a pour ambition de développer les principes physiques nécessaires au champ d’investigation du travail à accomplir. Ainsi, cette étude propose d’élaborer les différents éléments d’un bolomètre, réunissant un senseur thermique optimisé ainsi qu’un absorbeur de rayonnement de faible chaleur spécifique, permettant d’envisager la mise au point d’une matrice de bolomètres optimisée dans le cadre du projet QUBIC dont la campagne d’observation est prévue courant 2015 au dôme C du pôle Sud. / Since its discovery in 1964, the study of the Cosmic Microwave Background (CMB) in the field as of millimetre-length wavelengths became a major stake of experimental research in the field of cosmology. In particular, its anisotropies in temperature, measured for the first time by satellite COBE then more finely by the experiment WMAP and the PLANCK satellite. The predicted existence of anisotropies of polarization of the Cosmic Microwave Background is currently been part of the privileged field of experimentation of the study of the CMB. Indeed, the proof of exists modes B of polarization, single signature of the paramount gravitational waves, currently is the object of an intensive experimental research by the means in particular of the instrument BICEP2 which would have detected its signature in 2014 in values of the tensor report on scalar R = 0.2. Project QUBIC makes party of these experiments intended to reveal the modes B of polarization thanks to its instrument based on the technique of the interferometers and the development of bolometers array, asking for a thorough field of investigation including, amongst other things, the solid state physics, the physics of the low temperatures and cosmology. The thesis presented here is within this framework, with for objective making of a bolometers array whose performance and optimization should make it possible to acquire the necessary sensitivity to the observation of the B-mode polarization. The various experimental techniques acquired with the CSNSM of Orsay indeed make it possible to consider the optimization of the key elements of the bolometers array while being pressed in particular on amorphous alloy of NbxSi1-x for making of an optimized thermal sensor, and on an innovative material, titanium-vanadium alloy, for the clarification of an effective superconducting absorber of radiation, whose low specific heat must make it possible to reach a response time of the detector about ten millisecond, value of the response time necessary to an effective reading of the signal of the Cosmic Microwave Background. The manuscript of thesis here present has as an ambition to develop the physical principles necessary to the field of investigation of work to be achieved. Thus, this study proposes to work out the various elements of a bolometer, joining together a thermal sensor optimized as well as an absorber of radiation of low specific heat, making it possible to consider the clarification of a bolometers array optimized within the framework of the project QUBIC whose observation campaign is envisaged during 2015 with the dome C of the south pole.