Far infrared optical properties of V and Cr doped Sb2Te3 /

The far infrared reflectance of Sb2Te3 , Sbi.97Vo.o3Te3 and Sbi.94Cr .o6Te3 was measured near normal incidence at different temperatures (between 45K and 300K). The direct current resistivities of the above samples were also measured between the temperatures of 4K and 300K. Also Kramers Kronig (KK) analyses were performed on the reflectance spectra to obtain the optical conductivities. In the doped samples, it was observed that a phonon at 62cm-1 softens to about 55cm-1 on decreasing the temperature from 295K to 45K. Also, it was observed that the plasma frequency of the doped samples is independent of doping. The scattering rate for the vanadium doped sample was seen to be greater than that for the chromium doped sample despite the fact that vanadium impurity density is less than that of chromium. The Drude-Lorentz model fits to the KK optical conductivity show that the samples used in this work are conventional metals. Definitive measurements of the temperature dependence of the scattering rate across the ferromagnetic transition await equipment changes allowing measurements at low temperature using the mercury cadmium telluride (MCT) detector.

Optical Properties of Sb2Te3, and Dilute Magnetic Semiconductors Sb1.97 VO.03 Te3 and Sb1.94 CrO.06 Te3

This thesis reports on the optical properties of the dilute magnetic semiconductors, Sb1.97 V 0.03 Te3 and Sb1.94Cr0.06Te3, along with the parent compound Sb2Te3' These materials develop a ferromagnetic state at low temperature with Curie temperatures of 22 K and 16 K respectively. All three samples were oriented such that the electric field vector of the light was perpendicular to the c-axis. The reflectance profile of these samples in the mid-infrared (500 to 3000 cm-1) shows a pronounced plasma edge which retracts with decreasing temperature. The far-infrared region of these samples exhibits a phonon at ~ 60 cm-1 which softens as temperature decreases. Kramers-Kronig analysis and a Drude-Lorentz model were employed to determine the optical constants of the bulk samples. The real part of the optical conductivity is shown to consist of intraband contributions at frequencies below the energy gap (~0.26 eV) and interband contributions at frequencies above the energy gap. The temperature dependence of the scattering rate show that a mix of phonon and impurity scattering are present, while the signature of traditional spin disorder (magnetic) scattering was difficult to confirm.

Analyse cinématique de l'hydrogène ionisé et étude du gaz ionisé diffus de trois galaxies du Groupe Sculpteur : NGC253, NGC300 et NGC247

Mémoire numérisé par la Division de la gestion de documents et des archives de l'Université de Montréal

Studies on the Effect of Randomness on the Synchronization of Coupled Systems and on the Dynamics of Intermittently driven systems

Nonlinear dynamics has emerged into a prominent area of research in the past few Decades.Turbulence, Pattern formation,Multistability etc are some of the important areas of research in nonlinear dynamics apart from the study of chaos.Chaos refers to the complex evolution of a deterministic system, which is highly sensitive to initial conditions. The study of chaos theory started in the modern sense with the investigations of Edward Lorentz in mid 60's. Later developments in this subject provided systematic development of chaos theory as a science of deterministic but complex and unpredictable dynamical systems. This thesis deals with the effect of random fluctuations with its associated characteristic timescales on chaos and synchronization. Here we introduce the concept of noise, and two familiar types of noise are discussed. The classifications and representation of white and colored noise are introduced. Based on this we introduce the concept of randomness that we deal with as a variant of the familiar concept of noise. The dynamical systems introduced are the Rossler system, directly modulated semiconductor lasers and the Harmonic oscillator. The directly modulated semiconductor laser being not a much familiar dynamical system, we have included a detailed introduction to its relevance in Chaotic encryption based cryptography in communication. We show that the effect of a fluctuating parameter mismatch on synchronization is to destroy the synchronization. Further we show that the relation between synchronization error and timescales can be found empirically but there are also cases where this is not possible. Studies show that under the variation of the parameters, the system becomes chaotic, which appears to be the period doubling route to chaos.

Fluoreszenz und Lasertätigkeit in dünnen amorphen Schichten von Spirobifluorenderivaten

Es wurden die optischen Eigenschaften einiger Spirooligophenylverbindungen untersucht. Bei den Verbindungen handelte es sich um lineare und verzweigte Derivate des Spirobifluorens. Es wurden dünne amorphe Schichten der Verbindungen mittels spincoating und Vakuumverdampfen (OMBD) auf unterschiedlichen Substraten hergestellt. Mit spektroskopischer Ellipsometrie konnten die Schichtdicken und optische Konstanten der dünnen Schichten bestimmt werden. Dafür sind die Extinktionsspektren mit Tauc-Lorentz-Oszillatoren modelliert worden. Auf diese Weise ließen sich die optischen Konstanten der amorphen Filme besser beschreiben als mit den üblicherweise verwendeten Gauß-Oszillatoren. In dünnen Filmen von Spirosexiphenyl konnte uniaxiale Anisotropie nachgewiesen werden. Im Bereich der pie,pie*-Bande beträgt das Verhältnis des ordentlichen zum außerordentlichen Extinktionskoeffizienten 2.09. Mit einer Integrationskugel wurden die absoluten Quantenausbeuten der Fluoreszenz in festen Filmen bestimmt. Dafür ist ein vereinfachtes Verfahren der Auswertung entwickelt worden. Im Vergleich der untersuchten Substanzen zeigt sich, dass die Verbindungen mit dem Sexiphenyl-Chromophor höhere Quantenausbeuten im Festkörper haben (31 % - 48 %) als die Verbindungen mit Quaterphenyl als Chromophor (15 % - 30 %). In den beiden Klassen haben jeweils die sterisch anspruchsvollen Octopusvarianten die höchsten Festkörperquantenausbeuten. Durch verdünnen mit m,m-Spirosexiphenyl konnte die Quantenausbeute von p,p-Spirosexiphenyl in dünnen festen Filmen bis auf 65 % (95 % m,m- und 5 % p,p-Spirosexiphenyl) gesteigert werden. Eine Korrelation der Quantenausbeuten in Lösung und im festen, unverdünnten Film wurde nicht festgestellt. Als dünne Filme in Wellenleitergeometrie zeigen Spirooligophenyle bei optischer Anregung verstärkte spontane Emission (ASE). Dies manifestiert sich in einer Einengung des Emissionsspektrums mit zunehmender Pumpleistungsdichte. Auch für stimulierte Emission sind die Verbindungen mit Sexiphenylchromophor besser geeignet. Die niedrigste Schwelle in einer unverdünnten Reinsubstanz wurde mit 0.23 µJ/cm² in einer aufgeschleuderten Schicht Spirosexiphenyl gemessen. Auch 4-Spiro³, Spiro-SPO und Octo-2 zeigten niedrige ASE-Schwellen von 0.45 µJ/cm², 0.45 µJ/cm² und 0.5 µJ/cm². Die ASE-Schwellwerte von Spiroquaterphenyl und seinen beiden Derivaten Methoxyspiroquaterphenyl und Octo-1 sind mit 1.8 µJ/cm², 1.4 µJ/cm² und 1.2 µJ/cm² höher als die der Sexiphenylderivate. Im gemischten System aus m,m- und p,p-Spirosexiphenyl konnte die ASE-Schwelle noch weiter gesenkt werden. Bei einer Konzentration von 5 % p,p-Spirosexiphenyl wurde ein Schwellwert von nur 100 nJ/cm² bestimmt. Durch Dotierung mit unterschiedlichen Farbstoffen in Spirosexiphenyl als Matrix konnte ASE fast über den gesamten sichtbaren Spektralbereich gezeigt werden. Mit der „variable Streifenlänge“ (VSL-) -Methode wurden die pumpleistungsabhängigen Gainspektren dünner aufgedampfter Proben gemessen. Hieraus konnten die Wechselwirkungsquerschnitte der stimulierten Emission der Substanzen ermittelt werden. In Übereinstimmung mit den Verhältnissen bei den Festkörperfluoreszenzquantenausbeuten und den Schwellwerten der ASE sind auch bei den Gainkoeffizienten reiner Spirooligophenyle die besten Werte bei den Sexiphenylderivaten gefunden worden. Der Wirkungsquerschnitt der stimulierten Emission beträgt für Methylspiroquaterphenyl und Octo-1 ca. 1.8*10^-17 cm². Für Spiro-SPO und Spirosexiphenyl wurden Wirkungsquerschnitte von 7.5*10^-17 cm² bzw. 9.2*10^-17 cm² bestimmt. Noch etwas größer waren die Werte im gemischten System aus m,m- und p,p-Spirosexiphenyl (1.1*10^-16 cm²) und für DPAVB dotiert in Spirosexiphenyl (1.4*10^-16 cm²). Der höchste Maximalwert des Gainkoeffizienten von 328 cm-1 bei einer absorbierten Pumpenergiedichte von 149 µJ/cm² wurde mit Spirosexiphenyl erreicht. Abschließend wurden DFB-Laser-Strukturen mit reinen und dotierten Spirooligophenylverbindungen als aktiven Materialien vorgestellt. Mit Spiroterphenyl konnte ein DFB-Laser mit der bisher kürzesten Emissionswellenlänge (361.9 nm) in einem organischen Festkörperlaser realisiert werden. Mit reinen Spirooligophenylverbindungen und Mischungen daraus habe ich DFB-Lasing bei Wellenlängen zwischen 361.9 nm und 479 nm aufgezeigt. Durch Dotierung mit DPAVB wurde der Bereich der erreichbaren Wellenlängen bis 536 nm erweitert, bei gleichzeitiger Erniedrigung der Schwellenergiedichten für Lasertätigkeit. Bei Emissionswellenlängen von 495 nm bis 536 nm blieb die Laserschwelle zwischen 0.8 µJ/cm² und 1.1 µJ/cm². Diese Werte sind für DFB-Laser zweiter Ordnung sehr niedrig und geben Anlass zu glauben, dass sich mit DFB-Strukturen erster Ordnung Schwellen im Nanojoule Bereich erzielen lassen. Damit würde man den Bedingungen für elektrisch gepumpten Betrieb nahe kommen.

Geometría y luz : papeles para el bachillerato.

Ejemplar fotocopiado

Teoría de la relatividad sin el segundo postulado.

Reflexión sobre la Teoría de la Relatividad. Se pretende llenar un hueco presentando una deducción a partir de las transformaciones de Lorentz, pero con la peculiaridad de prescindir del famoso segundo postulado de Einstein, es decir, de la invariancia de la velocidad de la luz, en su demostración. Se hace especial mención a la teoría de la relatividad, a las transformaciones de Lorente sin el segundo postulado, a la masa en relatividad, y como último elemento, al límite de la mecánica relativista.

Introducci??n a la Teor??a de la Relatividad

Desarrollo de los fundamentos y conceptos b??sicos de la teor??a de la relatividad en un intento de hacerla asequible para los alumnos de secundaria, como las transformaciones de Lorentz o la composici??n de velocidades.

The geometry of optimal control solutions on some six dimensional lie groups

This paper examines optimal solutions of control systems with drift defined on the orthonormal frame bundle of particular Riemannian manifolds of constant curvature. The manifolds considered here are the space forms Euclidean space E-3, the spheres S-3 and the hyperboloids H-3 with the corresponding frame bundles equal to the Euclidean group of motions SE(3), the rotation group SO(4) and the Lorentz group SO(1,3). The optimal controls of these systems are solved explicitly in terms of elliptic functions. In this paper, a geometric interpretation of the extremal solutions is given with particular emphasis to a singularity in the explicit solutions. Using a reduced form of the Casimir functions the geometry of these solutions are illustrated.

Integrating control systems defined on the frame bundles of the space forms

This paper considers left-invariant control systems defined on the orthonormal frame bundles of simply connected manifolds of constant sectional curvature, namely the space forms Euclidean space E-3, the sphere S-3 and Hyperboloid H-3 with the corresponding frame bundles equal to the Euclidean group of motions SE(3), the rotation group SO(4) and the Lorentz group SO(1, 3). Orthonormal frame bundles of space forms coincide with their isometry groups and therefore the focus shifts to left-invariant control systems defined on Lie groups. In this paper a method for integrating these systems is given where the controls are time-independent. In the Euclidean case the elements of the Lie algebra se(3) are often referred to as twists. For constant twist motions, the corresponding curves g(t) is an element of SE(3) are known as screw motions, given in closed form by using the well known Rodrigues' formula. However, this formula is only applicable to the Euclidean case. This paper gives a method for computing the non-Euclidean screw motions in closed form. This involves decoupling the system into two lower dimensional systems using the double cover properties of Lie groups, then the lower dimensional systems are solved explicitly in closed form.

Integrating Hamiltonian systems defined on the Lie groups SO(4) and SO(1,3)

This paper examines optimal solutions of control systems with drift defined on the orthonormal frame bundle of particular Riemannian manifolds of constant curvature. The manifolds considered here are the space forms Euclidean space E³, the spheres S³ and the hyperboloids H³ with the corresponding frame bundles equal to the Euclidean group of motions SE(3), the rotation group SO(4) and the Lorentz group SO(1,3). The optimal controls of these systems are solved explicitly in terms of elliptic functions. In this paper, a geometric interpretation of the extremal solutions is given with particular emphasis to a singularity in the explicit solutions. Using a reduced form of the Casimir functions the geometry of these solutions is illustrated.

Singularities of optimal control problems on some 6-D lie groups

This paper considers the motion planning problem for oriented vehicles travelling at unit speed in a 3-D space. A Lie group formulation arises naturally and the vehicles are modeled as kinematic control systems with drift defined on the orthonormal frame bundles of particular Riemannian manifolds, specifically, the 3-D space forms Euclidean space E-3, the sphere S-3, and the hyperboloid H'. The corresponding frame bundles are equal to the Euclidean group of motions SE(3), the rotation group SO(4), and the Lorentz group SO (1, 3). The maximum principle of optimal control shifts the emphasis for these systems to the associated Hamiltonian formalism. For an integrable case, the extremal curves are explicitly expressed in terms of elliptic functions. In this paper, a study at the singularities of the extremal curves are given, which correspond to critical points of these elliptic functions. The extremal curves are characterized as the intersections of invariant surfaces and are illustrated graphically at the singular points. It. is then shown that the projections, of the extremals onto the base space, called elastica, at these singular points, are curves of constant curvature and torsion, which in turn implies that the oriented vehicles trace helices.

Classification of instability modes in a model of aluminium reduction cells with a uniform magnetic field

A unified view on the interfacial instability in a model of aluminium reduction cells in the presence of a uniform, vertical, background magnetic field is presented. The classification of instability modes is based on the asymptotic theory for high values of parameter β, which characterises the ratio of the Lorentz force based on the disturbance current, and gravity. It is shown that the spectrum of the travelling waves consists of two parts independent of the horizontal cross-section of the cell: highly unstable wall modes and stable or weakly unstable centre, or Sele’s modes. The wall modes with the disturbance of the interface being localised at the sidewalls of the cell dominate the dynamics of instability. Sele’s modes are characterised by a distributed disturbance over the whole horizontal extent of the cell. As β increases these modes are stabilized by the field.

THREE-DIMENSIONAL NUMERICAL SIMULATIONS OF MAGNETIZED WINDS OF SOLAR-LIKE STARS

By means of self-consistent three-dimensional magnetohydrodynamics (MHD) numerical simulations, we analyze magnetized solar-like stellar winds and their dependence on the plasma-beta parameter (the ratio between thermal and magnetic energy densities). This is the first study to perform such analysis solving the fully ideal three-dimensional MHD equations. We adopt in our simulations a heating parameter described by gamma, which is responsible for the thermal acceleration of the wind. We analyze winds with polar magnetic field intensities ranging from 1 to 20 G. We show that the wind structure presents characteristics that are similar to the solar coronal wind. The steady-state magnetic field topology for all cases is similar, presenting a configuration of helmet streamer-type, with zones of closed field lines and open field lines coexisting. Higher magnetic field intensities lead to faster and hotter winds. For the maximum magnetic intensity simulated of 20 G and solar coronal base density, the wind velocity reaches values of similar to 1000 km s(-1) at r similar to 20r(0) and a maximum temperature of similar to 6 x 10(6) K at r similar to 6r(0). The increase of the field intensity generates a larger ""dead zone"" in the wind, i.e., the closed loops that inhibit matter to escape from latitudes lower than similar to 45 degrees extend farther away from the star. The Lorentz force leads naturally to a latitude-dependent wind. We show that by increasing the density and maintaining B(0) = 20 G the system recover back to slower and cooler winds. For a fixed gamma, we show that the key parameter in determining the wind velocity profile is the beta-parameter at the coronal base. Therefore, there is a group of magnetized flows that would present the same terminal velocity despite its thermal and magnetic energy densities, as long as the plasma-beta parameter is the same. This degeneracy, however, can be removed if we compare other physical parameters of the wind, such as the mass-loss rate. We analyze the influence of gamma in our results and we show that it is also important in determining the wind structure.

Formulation of the standard model in terms of spinor fields

We propose an alternative formulation of the Standard Model which reduces the number of free parameters. In our framework, fermionic fields are assigned to fundamental representations of the Lorentz and the internal symmetry groups, whereas bosonic field variables transform as direct products of fundamental representations of all symmetry groups. This allows us to reduce the number of fundamental symmetries. We formulate the Standard Model by considering the SU(3) and SU(2) symmetry groups as the underlying symmetries of the fundamental interactions. This allows us to suggest a model, for the description of the interactions of the intermediate bosons among themselves and interactions of fermions, that makes use of just two parameters. One parameter characterizes the symmetric phase, whereas the other parameter (the asymmetry parameter) gives the breakdown strength of the symmetries. All coupling strengths of the Standard Model are then derived in terms of these two parameters. In particular, we show that all fermionic electric charges result from symmetry breakdown.