Cette thèse présente l'étude de l'interaction de lumière cohérente avec une couche sub-longueur d'onde de vapeur alcaline atomique confinée en nano-cellule et applications pour la formation de résonances optiques étroites.Nous développons un modèle théorique décrivant l'interaction résonante de lumière laser avec la couche mince de vapeur alcaline en présence d'un champ magnétique. Nous montrons qu'en raison d'un régime transitoire d'interaction, seuls les atomes lents contribuent au signal et leur spectre de transmission est essentiellement sans effet Doppler. La nature des spectres obtenus fait de la spectroscopie de transmission, en nano-cellule, une technique pratique pour l'étude de transitions très rapprochées et l'évolution de leur comportement dans un champ magnétique. Des expériences réalisées pour des champs magnétiques jusqu'à 7000 G montrent un excellent accord entre théorie et expérience.Nous explorons aussi la rotation Faraday du plan de polarisation de la lumière lors de sa propagation dans la couche mince atomique. Bien que l'angle de rotation soit très faible, nous observons que les résonances des spectres de rotation Faraday sont plus étroites que celles de transmission. Enfin, nous étudions de nouvelles possibilités pour former des résonances optiques étroites et montrons qu'un traitement par deuxième dérivée des spectres de transmission donne le meilleur rétrécissement de raies parmi toutes les méthodes étudiées dans cette thèse. / This thesis presents the study of coherent light interaction with a sub-wavelength atomic alkali vapor layer confined in a nano-cell and applications for the formation of narrow optical resonances.We develop a theoretical model describing the resonant interaction of the laser light with the thin alkali vapor layer in the presence of an external static magnetic field. We show that due to a transient regime of interaction, only slow atoms contribute to the signal and their transmission spectrum is essentially Doppler-free. The nature of the obtained spectra makes the transmission spectroscopy from a nano-cell a convenient technique to perform studies of closely-spaced atomic transitions and investigate their behavior in magnetic fields. Experimental realizations for magnetic field up to 7000~G show an excellent agreement between theory and experiment.We also explore the Faraday rotation of the plane polarization of light with the propagation through the thin atomic slab. We see that despite a small angle of rotation, Faraday rotation spectra exhibit resonances narrower than that for transmission. At last, we investigate new possibilities to form narrow optical resonances in nano-cells and show that second derivation processing of transmission spectra yields the strongest line narrowing among all methods studied in this thesis.

We calculate the circularly polarized Stokes V(λ) profile for emission lines, formed in hot-star winds threaded with a weak radial magnetic field. For simplicity, the field is treated as a split monopole under the assumptions that it has been radially combed by the wind, and rotation is not playing a central role. Invoking the weak-field approximation, we find that the V(λ) profile has a characteristic “heartbeat” shape exhibiting multiple sign inversions, which might be mistaken for noise in the absence of theoretical guidance. We also conclude that there is a tendency for the V(λ) profile to integrate to zero on each side of the line separately. The overall scale of V(λ)/I(λ) is set by the ratio of the field strength to the flow speed, B/v, characteristic of the line-forming region, and is of the order of 0.1% for a wind magnetic field B ≅ 100G at depths where the wind speed is v ≅ 100 km s−1.

No description available.

Die vorliegende Arbeit befasst sich mit der Molekularstrahlepitaxie und Charakterisierung von CdSe und (Cd,Mn)Se-Quantenpunkten (QP) auf ZnSe-Puffer. Die QP werden durch einen thermisch aktivierten 2D-3D Übergang eines ursprünglich zweidimensionalen CdSe/(Cd,Mn)Se-Films erzeugt. Die Mechanismen der QP-Bildung werden in-situ mittels Reflexionsbeugung hochenergetischer Elektronen und Atom-Kraft-Mikroskopie (UHV-AFM) studiert. Ex-situ Untersuchungen an vergrabenen QP-Strukturen mittels Transmissionselektronenmikroskopie (TEM) und Photolumineszenz (PL) /Magneto-PL ergänzen die in-situ Analyse der CdSe Oberfläche. Die Kombination der Analysemethoden ermöglicht erstmalig den Nachweis, dass mit der thermischen Aktivierung eine Stranski-Krastanov-Morphologie aus CdSe QP, mit einem Kern aus reinem CdSe, auf einem geschlossenen CdSe Film erzeugt werden kann. Die statistische Auswertung im UHV-AFM ergibt eine mittlere QP-Höhe von 1,6 nm, eine QP-Dichte von 1100/µm² sowie einen Durchmesser von unterhalb 10 nm. Aus diesen Parametern lässt sich als oberes Limit des QP-Volumens ein Wert von < 0,15 ML ermitteln. TEM-Messungen ergeben, dass Interdiffusion bei der Bildung der QP sowie während dem Überwachsen von untergeordneter Bedeutung ist. Im UHV-AFM zeigt sich, dass CdSe-QP unter Labormaßstäben morphologisch stabil sind. Über einen Zeitraum von 5 Tagen, sowohl im UHV als auch an Umgebungsluft, sind bei Raumtemperatur keine Reifungserscheinungen der CdSe-QP-Morphologie beobachtbar. Das Studium der Bildungskinetik führt zu der Erkenntnis, dass der 2D-3D Übergang von einem zeitlich instabilen Ausgangszustand abhängig ist und somit kinetisch determiniert. Die experimentellen Befunde deuten darauf hin, dass unmittelbar nach dem Wachstum eine Glättung der Oberfläche auf atomarer Ebene einsetzt. In einem einfachen Modell wird die QP-Bildung als Superposition der Glättung und dem Verhältnis der Wahrscheinlichkeiten des Aufwärtssprungs zum Abwärtssprung zwischen zwei ML-Terrassen beschrieben. Erste Untersuchungen zum Wachstum von (Cd,Mn)Se QP ergeben, dass es mit der thermischen Aktivierung möglich ist bis zu einer Konzentration von ca. 10 % Mn (Cd,Mn)Se QP zu erhalten. Der Einbau des Mn bewirkt eine Reduktion der mittleren QP-Dichte und QP-Höhe. Experimente auf pseudomorphem und relaxiertem ZnSe-Puffer zeigen, dass der entscheidende Einfluss des Mn nicht in der Veränderung der Verspannung liegt, sondern in einer Veränderung der Oberflächendiffusivität. In magneto-optischen Untersuchungen der (Cd,Mn)Se-QP-Strukturen wird eindeutig der Riesen-Zeemaneffekt nachgewiesen. Es werden experimentell effektive g-Faktoren bis zu einem Wert von 220 ermittelt (B = 6T). Der Vergleich mit der Rechnung zeigt, dass das Mn in den QP eingebaut ist. In dieser Arbeit wird das Verständnis der II-VI-QP-Bildung erweitert und eine verbesserte Kontrolle des QP-Ensembles erreicht. Die erzeugten semimagnetischen Strukturen stellen einen Ausgangspunkt für weitergehende optische Experimente dar, an denen in naher Zukunft gezielt einzelne Spins manipuliert und studiert werden können. / In this work CdSe and (Cd,Mn)Se Quantum Dots (QD`s) are grown on ZnSe by molecular beam epitaxy. The QD`s are obtained within a thermicall activated 2D-3D transition of an initially two-dimensional CdSe/(Cd,Mn)Se thin film. The physics behind the 2D-3D transition is investigated in-situ by reflection of high energy electron diffraction and atomic force microscopy (UHV-AFM) measurements. Additionally ex-situ data gained on buried QD structures within Transmission Electron Microscopy (TEM) and Photoluminescence (PL) /Magneto-PL measurements are presented. The study proves for the first time that after the thermal activation a Stranski-Krastanov morphology is established. A statistical evaluation of the QD morphology by UHV-AFM supplies an average QD-height of about 1.6 nm, a QD-density of about 1100/µm² and an upper diameter of about 10 nm. The total QD volume is determined to a value of below 0.15 ML. TEM on overgrown structures reveals QD`s, with a core of pure CdSe, on a closed wetting layer. The data show that interdiffusion is of minor importance for the QD formation as well as during the overgrowth. The stability of the QD morphology is investigated with the UHV-AFM at room temperature. It is shown that the CdSe QD morphology is stable at UHV as well as ambient-air conditions over a time period of 5 days. The experiments demonstrate that CdSe QD`s do not ripen on a laboratory time scale. The investigation of the formation kinetics reveals that the 2D-3D transition is dependent from a unstable precursor state and is therefore determined by kinetics. The experiments indicate that immediately after growth the surface begins to smoothen on an atomar scale. In a simple model the QD formation is described as a superposition of the smoothening and the ratio of upwards and downwards hopping between two ML terraces. First investigations on the growth of (Cd,Mn)Se QD`s show that after the incorporation of up to 10 % Mn semimagnetic QD´s are obtained by the thermal activation. The incorporation of Mn leads to a reduction of the average QD density and QD height. Experiments on pseudomorphic and relaxed ZnSe buffer are compared. It is concluded that strain is not a crucial factor for the QD formation and that probably surface processes like diffusibility of the atomic species play an important role. Magneto-optical investigations of the (Cd,Mn)Se QD structures prove the appearance of the giant-Zeemaneffect. Effective g-values of about 220 have been measured (B = 6T). In a comparison with the calculation the incorporation of Mn into the QD`s is concluded. Within this work the comprehension of the II-VI QD formation is extended and an improved control over the QD morphology is reached. The produced semimagnetic QD structures appear as a starting point for future optical investigations concerning the control of single spins.

No description available.

We have used a series of observations of HD119419, performed in 2012 and 2013at the European Southern Observatory 3.6-m telescope in La Silla, Chile. These are high resolutionspectropolarimetric observations with coverage in all four Stokes parameters. We performed a chemical abundance analysis of HD119419, in the absence of any being published previously for this star. We used a LLmodels stellar atmosphere code with effective temperature11500 K and surface gravity log g = 4.0, together with the spectrum synthesis code synmast. Abundances were adjusted until the synthetic spectra matched the mean observed spectra as well as possible, and these abundances were assumed to be representative of the photosphere of HD119419. We found good estimates for some Fe-peak elements and rare-earth elements. The abundance estimates were used to compute least-squares deconvolution Stokes spectra, from which we calculated how the longitudinal magnetic field and net linear polarization varies with rotational phase for HD119419. We calculated an improved rotational period for HD119419 using our longitudinal magnetic field measurements together with previous measurements from the literature, determining it to be 2.60059(1) days. We found that the Stokes QUV are unusually strong for the rare-earth elements in HD119419, considering their weaker Stokes I profiles compared to the Fe-peak elements in particular.

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior / We investigate the anomalous Zeeman effect for the hydrogen atom in noncommutative quantum mechanics. By using of the Bopp's shift method the nonrelativistic regime is evaluated and the noncommutative Hamiltonian is determined. By means the first order perturbation theory, the energy correction is calculated for the case of weak external magnetic field. We obtained the orbital and spin Landé factors on noncommutative space. It is shown that the experimental value for the orbital and spin Landé factors put an upper bound on the magnitude of the parameter of noncommutativity of the order of 0 . (8GeV )-2and 0 . (0; 01GeV )-2, respectively. We use the same perturbation calculation for the null external magnetic eld case, showing that some energy shift appears, modifying the ne structure spectrum. Finally, we calculate the Lamb shift and comparing the result with the experimental value from spectroscopy, we got a new bound for the noncommutative parameter, 0 . (3GeV )-2. / Investigamos o efeito Zeeman anâmalo para o átomo de hidrogênio em mecânica quântica não comutativa. Utilizando-se do método Bopp's shift, o regime não relativístico de avaliado e o Hamiltoniano não comutativo é determinado. Usando a teoria de perturbação de primeira ordem, a correção para a energia é calculada para o caso de campo magnético externo fraco. Obtemos os fatores de Landé orbital e de spin em espaço não comutativo. É mostrado que o valor experimental para os fatores de Landé orbital e de spin, impõem um limite superior na magnitude do parâmetro de não comutatividade da ordem de 0 (8GeV )-2 e (0; 01GeV )-2, respectivamente. Utilizamos o mesmo cálculo de perturbação para o caso de campo magnético externo nulo, mostrando que algum shift de energia aparece, que modica espectro de estrutura fina. Finalmente, calculamos o Lamb shift e comparando o resultado com o valor experimental da espectroscopia, obtemos um novo limite para o parâmetro não comutativo, 0 . (3GeV )-2.

The effect of electromagnetically induced transparency is observed, using nanocelland microcell. The EIT-resonance with good parameters (high contrast and small FWHM) is obtained in thick cells. The EIT-resonance splitting in magnetic field is observed for the cases of D1-line of 85Rb and 85Rb. The theoretical model, explaining the EIT-resonance components frequency shift dependence on magnetic field strength is presented. The theoretical and experimental results are compared and good agreement is shown. Also the EIT-resonance behavior in hyperfine Paschen-Back regime is presented and explained. For the first time the N-type resonance in microcell is observed. Good parameters of theN-type resonance in microcell are obtained. It allows us to observe the N-type resonance behavior in magnetic field. The N-resonance splitting in magnetic field is observed for the cases of 85Rb and 85Rb. The theoretical calculations of the N-resonance components frequency shift dependence on magnetic field is presented. The theoretical and experimental results are compared and good agreement is shown. Also the N-resonance behavior in hyperfine Paschen-Back regime is presented and explained. Simultaneous observation of N- and EIT-resonance is shown. Comparison of EIT- and N-resonance is made

This theoretical thesis presents detailed study of negatively charged excitons - trions - confined in single quantum well in presence of perpendicular magnetic field. Complex valence band of GaAs/GaAlAs compound is described within Luttinger Hamiltonian framework. Singlet and triplet states of negative trion are introduced. Advanced theoretical analysis of Zeeman effect for different states of trion is performed. Landau gauge of magnetic field and unusual wavefunctions basis is chosen and its accuracy is tested. Evolution of ground state energy and photoluminescence spectra with magnetic field is evaluated for different values of Landé g-factors. Probability of occurrence of electrons with respect to the hole position and their spatial correlation function are investigated.

Using the method of the star product, the non-relativistic regime of the Dirac equation is evaluated and the NC hamiltonian to the Zeeman e ect is determined. Using the rst-order perturbation theory, the correction to the energy is calculated. We obtain the orbital and spin Land e factors. It is shown that the experimental value for the spin Land e factor put the following upper limit on the magnitude of the momentum NC parameter, p . 0; 34 eV=c. Established also a possible correction of the NC phase space to the presently accepted value of Planck's constant with an uncertainty of 2 part in 1035. By mapping via Boop's shift we obtain the Landau levels and the Hall conductivity for graphene in NC phase space. Using the current experimental precision, respectively, of the Hall conductivity and of the Landau levels in graphene, we obtain the following upper limit to the magnitude of the momentum NC parameter, p . 2; 5eV=c e p . 8; 5eV=c. Finally, by Newton's law in NC space and using the Langevin equations, we describe the Browniano motion, and thus we de ne a new physical parameter that shows the possibility of detecting NC eff ects on the macroscopic scale. / Utilizando-se do m étodo do produto estrela, o regime não relativí stico da equa ção de Dirac é avaliado e o hamiltoniano NC para o efeito Zeeman é determinado. Usando a teoria de perturba ção de primeira ordem, a corre ção para a energia é calculada. Obtemos assim, os fatores de Land é orbital e de spin. É mostrado que o valor experimental para o fator de Land é de spin impõe o seguinte limite superior na magnitude do parâmetro NC de momento,p . 0; 34 eV=c. Estabelecemos tamb ém uma possí vel corre ção do espa ço de fase NC para o valor atualmente aceito da constante de Planck, com uma incerteza de 2 partes em 10 elevado a 35. Atrav és do mapeamento via Boop's shift obtemos os n íveis de Landau e a condutividade Hall para o grafeno no espa ço de fase NC. Utilizando a atual precisão experimental, respectivamente, da condutividade Hall e dos n veis de Landau no grafeno, obtemos os seguintes limites superiores para a magnitude do parâmetro NC de momento,p . 2; 5eV=c ep . 8; 5eV=c. Por fim, atrav és das leis de Newton num espa ço NC e utilizando as equa ções de Langevin, descrevemos o movimento Browniano, e assim defi nimos um novo parâmetro f ísico que mostra a possibilidade de detectar efeitos NC na escala macrosc ópica.