8 resultados para INTRASEASONAL OSCILLATION
em ArchiMeD - Elektronische Publikationen der Universität Mainz - Alemanha
Resumo:
The standard model (SM) of particle physics is a theory, describing three out of four fundamental forces. In this model the Cabibbo-Kobayashi-Maskawa (CKM) matrix describes the transformation between the mass and weak eigenstates of quarks. The matrix properties can be visualized as triangles in the complex plane. A precise measurement of all triangle parameters can be used to verify the validity of the SM. The least precisely measured parameter of the triangle is related to the CKM element |Vtd|, accessible through the mixing frequency (oscillation) of neutral B mesons, where mixing is the transition of a neutral meson into its anti-particle and vice versa. It is possible to calculate the CKM element |Vtd| and a related element |Vts| by measuring the mass differences Dmd (Dms ) between neutral Bd and bar{Bd} (Bs and bar{Bs}) meson mass eigenstates. This measurement is accomplished by tagging the initial and final state of decaying B mesons and determining their lifetime. Currently the Fermilab Tevatron Collider (providing pbar{p} collisions at sqrt{s}=1.96 TeV) is the only place, where Bs oscillations can be studied. The first selection of the "golden", fully hadronic decay mode Bs->Ds pi(phi pi)X at DØ is presented in this thesis. All data, taken between April 2002 and August 2007 with the DØ detector, corresponding to an integrated luminosity of int{L}dt=2.8/fb is used. The oscillation frequency Dms and the ratio |Vtd|/|Vts| are determined as Dms = (16.6 +0.5-0.4(stat) +0.4-0.3(sys)) 1/ps, |Vtd|/|Vts| = 0.213 +0.004-0.003(exp)pm 0.008(theor). These results are consistent with the standard model expectations and no evidence for new physics is observable.
Resumo:
Gegenstand dieser Arbeit ist die Untersuchung der smektischen Phasen von Polysiloxanen mit flüssigkristallinen Seitengruppen (LC-Polysiloxane). Der erste Teil der vorliegenden Arbeit befasste sich mit der Herstellung verschiedener flüssigkristalliner ferroelektrischer Polysiloxane. Die Polymere wurden in Bezug auf das verwendete Polymerrückgrat (Homo- und Copolysiloxan) sowie durch den zusätzlichen Einbau von vernetzbaren Seitengruppen variiert. Im zweiten Teil der Arbeit wurden die Eigenschaften der smektischen Phasen der hergestellten Substanzen näher untersucht. Ein erster Untersuchungsgegenstand war das Dehnungsverhalten von freistehenden flüssigkristallinen Elastomerfilmen (LCE). Bei der Verwendung eines Polymers, in dem nur ein Teil des Polysiloxanrückgrats mit Seitengruppen substituiert ist, wird die uniaxiale Dehnung des Films parallel zu den smektischen Schichten durch eine gleichmäßige Kontraktion in der Filmebene und parallel zur Schichtnormalen ausgeglichen, was auf einen außergewöhnlich niedrigen smektischen Schichtkompressionsmodul zurückzuführen ist. Im Gegensatz dazu ist dieser Modul bei den Homopolymersystemen so groß, dass praktisch senkrecht zu den smektischen Schichten keine Kontraktion stattfindet. Ein zweiter Untersuchungsgegenstand der Netzwerkbildung bestand in der Bestimmung der dynamisch-mechanischen Eigenschaften der LC-Polysiloxane mittels eines Oszillationsrheometers. Hier erfolgten die Messungen von Speicher- und Verlustmodul in Abhängigkeit vom Polymerrückgrat und von der Vernetzung. Die unvernetzten Systeme zeigten in den smektischen Phasen (oberhalb Tg) noch – im wesentlichen – Festkörpereigenschaften (physikalische Vernetzung) mit einem dominierenden Speichermodul beim LC-Homopolysiloxan. Beim LC-Copolysiloxan haben beide Module eine gleiche Größenordnung. Am Phasenübergang in die isotrope Phase wurden beide Module absolut kleiner, der Verlustmodul aber relativ größer. In der isotropen Phase verhalten sich die LC-Polymere damit überwiegend wie viskose Schmelzen. Außerdem korrelierten die mittels DSC bestimmten Phasenübergangstemperaturen mit einer Änderung der dynamisch-mechanischen Eigenschaften. Nach der Vernetzung dominierte der Speichermodul sowohl beim LC-Homo- als auch beim LC-Copolysiloxan bis in die isotrope Phase, und es war aufgrund der Bildung einer festen Netzwerkstruktur keine Abhängigkeit der Module von Phasenübergängen mehr erkennbar. Als dritter Untersuchungsgegenstand wurde der Phasenübergang zwischen den beiden smektischen Phasen (SmC* nach SmA*) der flüssigkristallinen Polysiloxane näher behandelt. Als wichtigstes Ergebnis ist festzuhalten, dass die verdünnten LC-Polysiloxane an diesem Übergang fast keine Schichtdickenänderung aufweisen. Dazu wurde jeweils die röntgenographisch ermittelte Schichtdicke mit der aus den optischen Tiltwinkeln theoretisch berechneten Schichtdicke verglichen. Dadurch konnte gezeigt werden, dass sich die Phasenübergänge nach dem de Vries-Modell verhalten. Damit konnte zum ersten Mal an Polymersystemen ein de Vries-Verhalten nachgewiesen werden. Im Gegensatz dazu zeigte das Homopolysiloxan mit dem Dreiringmesogen beim Übergang von SmC* nach SmA* einen ausgeprägten Sprung in der Schichtdicke. Wie auch durch DSC-Messungen nachweisbar, lag ein Phasenübergang 1. Ordnung vor. Bei den LC-Copolysiloxanen liegt dagegen ein Phasenübergang 2. Ordnung vor. Schließlich wurde die Schichtdicke unter dem Einfluss der Vernetzung untersucht. Beim LC-Copolysiloxan mit dem Dreiringmesogen und einem Anteil an vernetzbaren Gruppen von 15 % wurde eine Stabilisierung der smektischen Phasen erreicht. Zum einen war die Änderung der Schichtdicke am SmC*-SmA*-Phasenübergang geringer im Vergleich zum unvernetzten System und zum anderen war noch 50 °C über der ursprünglichen Klärtemperatur eine smektische Schichtstruktur röntgenographisch nachzuweisen. Insgesamt ist es mit den verschiedenen Untersuchungsmethoden gelungen, einen systematischen Unterschied zwischen smektischen Homo- und Copolysiloxanen aufzuzeigen, der seinen Ursprung – aller Wahrscheinlichkeit nach – in der Mikrophasenseparation von Mesogenen und Polysiloxanketten findet.
Resumo:
The research has included the efforts in designing, assembling and structurally and functionally characterizing supramolecular biofunctional architectures for optical biosensing applications. In the first part of the study, a class of interfaces based on the biotin-NeutrAvidin binding matrix for the quantitative control of enzyme surface coverage and activity was developed. Genetically modified ß-lactamase was chosen as a model enzyme and attached to five different types of NeutrAvidin-functionalized chip surfaces through a biotinylated spacer. All matrices are suitable for achieving a controlled enzyme surface density. Data obtained by SPR are in excellent agreement with those derived from optical waveguide measurements. Among the various protein-binding strategies investigated in this study, it was found that stiffness and order between alkanethiol-based SAMs and PEGylated surfaces are very important. Matrix D based on a Nb2O5 coating showed a satisfactory regeneration possibility. The surface-immobilized enzymes were found to be stable and sufficiently active enough for a catalytic activity assay. Many factors, such as the steric crowding effect of surface-attached enzymes, the electrostatic interaction between the negatively charged substrate (Nitrocefin) and the polycationic PLL-g-PEG/PEG-Biotin polymer, mass transport effect, and enzyme orientation, are shown to influence the kinetic parameters of catalytic analysis. Furthermore, a home-built Surface Plasmon Resonance Spectrometer of SPR and a commercial miniature Fiber Optic Absorbance Spectrometer (FOAS), served as a combination set-up for affinity and catalytic biosensor, respectively. The parallel measurements offer the opportunity of on-line activity detection of surface attached enzymes. The immobilized enzyme does not have to be in contact with the catalytic biosensor. The SPR chip can easily be cleaned and used for recycling. Additionally, with regard to the application of FOAS, the integrated SPR technique allows for the quantitative control of the surface density of the enzyme, which is highly relevant for the enzymatic activity. Finally, the miniaturized portable FOAS devices can easily be combined as an add-on device with many other in situ interfacial detection techniques, such as optical waveguide lightmode spectroscopy (OWLS), the quartz crystal microbalance (QCM) measurements, or impedance spectroscopy (IS). Surface plasmon field-enhanced fluorescence spectroscopy (SPFS) allows for an absolute determination of intrinsic rate constants describing the true parameters that control interfacial hybridization. Thus it also allows for a study of the difference of the surface coupling influences between OMCVD gold particles and planar metal films presented in the second part. The multilayer growth process was found to proceed similarly to the way it occurs on planar metal substrates. In contrast to planar bulk metal surfaces, metal colloids exhibit a narrow UV-vis absorption band. This absorption band is observed if the incident photon frequency is resonant with the collective oscillation of the conduction electrons and is known as the localized surface plasmon resonance (LSPR). LSPR excitation results in extremely large molar extinction coefficients, which are due to a combination of both absorption and scattering. When considering metal-enhanced fluorescence we expect the absorption to cause quenching and the scattering to cause enhancement. Our further study will focus on the developing of a detection platform with larger gold particles, which will display a dominant scattering component and enhance the fluorescence signal. Furthermore, the results of sequence-specific detection of DNA hybridization based on OMCVD gold particles provide an excellent application potential for this kind of cheap, simple, and mild preparation protocol applied in this gold fabrication method. In the final chapter, SPFS was used for the in-depth characterizations of the conformational changes of commercial carboxymethyl dextran (CMD) substrate induced by pH and ionic strength variations were studied using surface plasmon resonance spectroscopy. The pH response of CMD is due to the changes in the electrostatics of the system between its protonated and deprotonated forms, while the ionic strength response is attributed from the charge screening effect of the cations that shield the charge of the carboxyl groups and prevent an efficient electrostatic repulsion. Additional studies were performed using SPFS with the aim of fluorophore labeling the carboxymethyl groups. CMD matrices showed typical pH and ionic strength responses, such as high pH and low ionic strength swelling. Furthermore, the effects of the surface charge and the crosslink density of the CMD matrix on the extent of stimuli responses were investigated. The swelling/collapse ratio decreased with decreasing surface concentration of the carboxyl groups and increasing crosslink density. The study of the CMD responses to external and internal variables will provide valuable background information for practical applications.
Resumo:
In linearen Paulfallen gespeicherte und lasergekühlte Ionen stellen in weiten Bereichen der Physik ideale Objekte hinsichtlich störungsfreier und präziser Messungen atomarer Übergangsfrequenzen und der gezielten Manipulation von Quantenzuständen dar. Eine Einschränkung dieser optimalen Bedingungen erfolgt durch Heizmechanismen, die aus Abweichungen des Speicherpotentials von der idealen Quadrupolform resultieren. Höhere Potentialordnungen führen zu einer Kopplung der radialen Bewegungsmoden und bei bestimmten Speicherparametern zu nichtlinearen Resonanzen. Hierbei werden die Ionenbahnen durch eine Energieaufnahme aus dem Speicherfeld destabilisiert. Dieses kann zu Linienverbreiterungen, einer Limitierung der Kohärenzzeiten und unter Umständen zu einem Ionenverlust führen. Die systematische Untersuchung dieser Instabilitäten in einer linearen Paulfalle erfolgt durch Spektroskopie an einer kleinen Anzahl lasergekühlter ^40Ca^+ - Ionen. Der experimentell zugängliche Speicherbereich wird mit hoher Auflösung abgetastet. Durch eine eingehende Quantifizierung der Falleneigenschaften werden die nichtlinearen Resonanzen eindeutig den erzeugenden Potentialtermen zugeordnet. Die Resonanzlinien zeigen eine charakteristische Aufspaltung, deren Größe vom angelegten Axialpotential bestimmt wird. Diese zusätzliche Kopplung der Radialbewegung an die Axialbewegung führt zu einer modifizierten Resonanzbedingung. Nichtlineare Resonanzen treten massenspezifisch auf. Da eine präzise Kontrolle der Axialpotentiale sehr einfach ist, könnten die beobachteten radial-axial koppelnden Resonanzen eine Anwendung in der Massenspektrometrie finden.
Resumo:
A numerical model for studying the influences of deep convective cloud systems on photochemistry was developed based on a non-hydrostatic meteorological model and chemistry from a global chemistry transport model. The transport of trace gases, the scavenging of soluble trace gases, and the influences of lightning produced nitrogen oxides (NOx=NO+NO2) on the local ozone-related photochemistry were investigated in a multi-day case study for an oceanic region located in the tropical western Pacific. Model runs considering influences of large scale flows, previously neglected in multi-day cloud resolving and single column model studies of tracer transport, yielded that the influence of the mesoscale subsidence (between clouds) on trace gas transport was considerably overestimated in these studies. The simulated vertical transport and scavenging of highly soluble tracers were found to depend on the initial profiles, reconciling contrasting results from two previous studies. Influences of the modeled uptake of trace gases by hydrometeors in the liquid and the ice phase were studied in some detail for a small number of atmospheric trace gases and novel aspects concerning the role of the retention coefficient (i.e. the fraction of a dissolved trace gas that is retained in the ice phase upon freezing) on the vertical transport of highly soluble gases were illuminated. Including lightning NOx production inside a 500 km 2-D model domain was found to be important for the NOx budget and caused small to moderate changes in the domain averaged ozone concentrations. A number of sensitivity studies yielded that the fraction of lightning associated NOx which was lost through photochemical reactions in the vicinity of the lightning source was considerable, but strongly depended on assumptions about the magnitude and the altitude of the lightning NOx source. In contrast to a suggestion from an earlier study, it was argued that the near zero upper tropospheric ozone mixing ratios which were observed close to the study region were most probably not caused by the formation of NO associated with lightning. Instead, it was argued in agreement with suggestions from other studies that the deep convective transport of ozone-poor air masses from the relatively unpolluted marine boundary layer, which have most likely been advected horizontally over relatively large distances (both before and after encountering deep convection) probably played a role. In particular, it was suggested that the ozone profiles observed during CEPEX (Central Equatorial Pacific Experiment) were strongly influenced by the deep convection and the larger scale flow which are associated with the intra-seasonal oscillation.
Resumo:
The present study describes a Late Miocene (early Tortonian - early Messinian) transitional carbonate system that combines elements of tropical and cool-water carbonate systems (Irakleion Basin, island of Crete, Greece). As documented by stratal geometries, the submarine topography of the basin was controlled by tilting blocks. Coral reefs formed by Porites and Tarbellastrea occurred in a narrow clastic coastal belt along a „central Cretan landmass“, and steep escarpments formed by faulting. Extensive covers of level-bottom communities existed in a low-energy environment on the gentle dip-slope ramps of the blocks that show the widest geographical distribution within the basin. Consistent patterns of landward and basinward shift of coastal onlap in all outcrop studies reveal an overriding control of 3rd and 4th order sea level changes on sediment dynamics and facies distributions over block movements. An increasingly dry climate and the complex submarine topography of the fault block mosaic kept sediment and nutrient discharge at a minimum. The skeletal limestone facies therefore reflects oligotrophic conditions and a sea surface temperature (SST) near the lower threshold temperature of coral reefs in a climatic position transitional between the tropical coral reef belt and the temperate zone. Stable isotope records (δ18O, δ13C) from massiv, exceptionally preserved Late Miocene aragonite coral skeletons reflect seasonal changes in sea surface temperature and symbiont autotrophy. Spectral analysis of a 69 years coral δ18O record reveals significant variance at interannual time scales (5-6 years) that matches the present-day eastern Mediterranean climate variability controlled by the Arctic Oscillation/North Atlantic Oscillation (AO/NAO), the Northern Hemisphere’s dominant mode of atmospheric variability. Supported by simulations with a complex atmospheric general circulation model coupled to a mixed-layer ocean model, it is suggested, that climate dynamics in the eastern Mediterranean and central Europe reflect atmospheric variability related to the Icelandic Low 10 million years ago. Usually, Miocene corals are transformed in calcite spar in geological time and isotope values are reset by diagenetic alteration. It is demonstrated that the relicts of growth bands represent an intriguing source of information for the growth conditions of fossil corals. Recrystallized growth bands were measured systematically in massive Porites from Crete. The Late Miocene corals were growing slowly with 2-4 mm/yr, compatible with present-day Porites from high latitude reefs, a relationship that fits the position of Crete at the margin of the Miocene tropical reef belt. Over Late Miocene time (Tortonian - early Messinian) growth rates remained remarkably constant, and if the modern growth temperature relationship for massive Porites applies to the Neogene, minimum (winter) SST did not exceed 19-21°C.
Resumo:
Atmosphärische Neutrinos erlauben es Prinzipien der Relativitätstheorie, wie die Lorentz-Invarianz und das schwache Äquivalenzprinzip, zu überprüfen. Kleine Abweichungen von diesen Prinzipien können in einigen Theorien zu messbaren Neutrinooszillationen führen. In dieser Arbeit wird in den aufgezeichneten Neutrinoereignissen des AMANDA-Detektors nach solchen alternativen Oszillationseffekten gesucht. Das Neutrinoteleskop AMANDA befindet sich am geographischen Südpol und ist in einer Tiefe zwischen 1500 m und 2000 m im antarktischen Eispanzer eingebettet. AMANDA weist Myonneutrinos über das Tscherenkow-Licht neutrinoinduzierter Myonen nach, woraus die Richtung der Bahn des ursprünglichen Neutrinos rekonstruiert werden kann. Aus den AMANDA-Daten der Jahre 2000 bis 2003 wurden aus circa sieben Milliarden aufgezeichneten Ereignissen, die sich hauptsächlich aus dem Untergrund aus atmosphärischen Myonen zusammensetzen, 3401 Ereignisse neutrinoinduzierter Myonen selektiert. Dieser Datensatz wurde auf alternative Oszillationseffekte untersucht. Es wurden keine Hinweise auf solche Effekte gefunden. Für maximale Mischungswinkel konnte die untere Grenze für Oszillationsparameter, welche die Lorentz-Invarianz oder das Äquivalenzprinzip verletzen, auf DeltaBeta (2PhiDeltaGamma) < 5,15*10e-27 festgelegt werden.
Resumo:
This thesis reports on the experimental investigation of controlled spin dependent interactions in a sample of ultracold Rubidium atoms trapped in a periodic optical potential. In such a situation, the most basic interaction between only two atoms at one common potential well, forming a micro laboratory for this atom pair, can be investigated. Spin dependent interactions between the atoms can lead to an intriguing time evolution of the system. In this work, we present two examples of such spin interaction induced dynamics. First, we have been able to observe and control a coherent spin changing interaction. Second, we have achieved to examine and manipulate an interaction induced time evolution of the relative phase of a spin 1/2-system, both in the case of particle pairs and in the more general case of N interacting particles. The first part of this thesis elucidates the spin-changing interaction mechanism underlying many fascinating effects resulting from interacting spins at ultracold temperatures. This process changes the spin states of two colliding particles, while preserving total magnetization. If initial and final states have almost equal energy, this process is resonant and leads to large amplitude oscillations between different spin states. The measured coupling parameters of such a process allow to precisely infer atomic scattering length differences, that e.g. determine the nature of the magnetic ground state of the hyperfine states in Rubidium. Moreover, a method to tune the spin oscillations at will based on the AC-Zeeman effect has been implemented. This allowed us to use resonant spin changing collisions as a quantitative and non-destructive particle pair probe in the optical lattice. This led to a series of experiments shedding light on the Bosonic superfluid to Mott insulator transition. In a second series of experiments we have been able to coherently manipulate the interaction induced time evolution of the relative phase in an ensemble of spin 1/2-systems. For two particles, interactions can lead to an entanglement oscillation of the particle pair. For the general case of N interacting particles, the ideal time evolution leads to the creation of spin squeezed states and even Schrödinger cat states. In the experiment we have been able to control the underlying interactions by a Feshbach resonance. For particle pairs we could directly observe the entanglement oscillations. For the many particle case we have been able to observe and reverse the interaction induced dispersion of the relative phase. The presented results demonstrate how correlated spin states can be engineered through control of atomic interactions. Moreover, the results point towards the possibility to simulate quantum magnetism phenomena with ultracold atoms in optical traps, and to realize and analyze many novel quantum spin states which have not been experimentally realized so far.