Measurement of the elastic electron-proton cross section and separation of the electric and magnetic form factor in the Q 2 range from 0.004 to 1 (GeV/c) 2

The electromagnetic form factors of the proton are fundamental quantities sensitive to the distribution of charge and magnetization inside the proton. Precise knowledge of the form factors, in particular of the charge and magnetization radii provide strong tests for theory in the non-perturbative regime of QCD. However, the existing data at Q^2 below 1 (GeV/c)^2 are not precise enough for a hard test of theoretical predictions.rnrnFor a more precise determination of the form factors, within this work more than 1400 cross sections of the reaction H(e,e′)p were measured at the Mainz Microtron MAMI using the 3-spectrometer-facility of the A1-collaboration. The data were taken in three periods in the years 2006 and 2007 using beam energies of 180, 315, 450, 585, 720 and 855 MeV. They cover the Q^2 region from 0.004 to 1 (GeV/c)^2 with counting rate uncertainties below 0.2% for most of the data points. The relative luminosity of the measurements was determined using one of the spectrometers as a luminosity monitor. The overlapping acceptances of the measurements maximize the internal redundancy of the data and allow, together with several additions to the standard experimental setup, for tight control of systematic uncertainties.rnTo account for the radiative processes, an event generator was developed and implemented in the simulation package of the analysis software which works without peaking approximation by explicitly calculating the Bethe-Heitler and Born Feynman diagrams for each event.rnTo separate the form factors and to determine the radii, the data were analyzed by fitting a wide selection of form factor models directly to the measured cross sections. These fits also determined the absolute normalization of the different data subsets. The validity of this method was tested with extensive simulations. The results were compared to an extraction via the standard Rosenbluth technique.rnrnThe dip structure in G_E that was seen in the analysis of the previous world data shows up in a modified form. When compared to the standard-dipole form factor as a smooth curve, the extracted G_E exhibits a strong change of the slope around 0.1 (GeV/c)^2, and in the magnetic form factor a dip around 0.2 (GeV/c)^2 is found. This may be taken as indications for a pion cloud. For higher Q^2, the fits yield larger values for G_M than previous measurements, in agreement with form factor ratios from recent precise polarized measurements in the Q2 region up to 0.6 (GeV/c)^2.rnrnThe charge and magnetic rms radii are determined as rn⟨r_e⟩=0.879 ± 0.005(stat.) ± 0.004(syst.) ± 0.002(model) ± 0.004(group) fm,rn⟨r_m⟩=0.777 ± 0.013(stat.) ± 0.009(syst.) ± 0.005(model) ± 0.002(group) fm.rnThis charge radius is significantly larger than theoretical predictions and than the radius of the standard dipole. However, it is in agreement with earlier results measured at the Mainz linear accelerator and with determinations from Hydrogen Lamb shift measurements. The extracted magnetic radius is smaller than previous determinations and than the standard-dipole value.

Chimäre Archonta?: vergleichend-morphologische Studien zur Hyolaryngealregion

Chimäre Archonta? Vergleichend-morphologische Studien zur Hyolaryngealregion. Mit Brevia zur Dental- und Tarsalmorphologie. Die Dissertation greift aus phylogenetisch-systematischer Perspektive das Problem des Primatenursprungs auf. Traditionell wurde die Überordnung Archonta (= Primates + Scandentia + Dermoptera + Chiroptera) angenommen, die aufgrund molekularer Befunde nicht mehr als valide eingestuft wird. Eine Klassifikation anhand der Superordo Euarchontoglires (= Primates + Scandentia + Dermoptera + Glires) wird derzeit bevorzugt. Beide Verwandtschaftshypothesen werden in den taxonomischen Analysen berücksichtigt, um den potentiellen Einfluss der Außengruppenwahl auf die Konstellation der Euarchonta (= Primates + Dermoptera + Scandentia) zu bestimmen. Der Schwerpunkt der Untersuchung liegt in der 3D-Rekonstruktion ontogenetischer Stadien der Hyolaryngealregion diverser Spezies der Ordnungen Artiodactyla, Chiroptera, Dermoptera, Primates, Rodentia, Scandentia und Soricomorpha. Mit AMIRA® 3.1.1 konnten basierend auf histologischen Schnittserien 18 dreidimensionale Modelle der überwiegend spätfetalen Zungenbein- und Kehlkopfregion dargestellt werden. Durch das Studium der Knorpelmorphologie und der Larynx-Myologie wurden 150 Merkmale definiert und in eine MacClade®-Datenmatrix überführt. Die auf dem Parsimonie-Prinzip basierenden PAUP®-Analysen sprechen für eine Schwestergruppenbeziehung der Primates und der Dermoptera (= Primatomorpha). Die als Chimäre titulierte Überordnung Archonta wurde als Vehikel verwendet, um die Integration der Chiropteren zu ermöglichen und die Hyolaryngealforschung zu intensivieren, da auch Echolot-Peilung verwendende Taxa Bestandteil der Untersuchung waren. Die morphologischen Ähnlichkeiten des Zungenbein- und Kehlkopfapparates zwischen der basalen Form Rousettus (Pteropodidae) und dem Dermoptera-Vertreter Cynocephalus wurden als symplesiomorphe Merkmale gedeutet. Bei der Außengruppenwahl eines Rodentia-Repräsentanten hingegen konnte in Übereinstimmung mit den molekularen Befunden und nach dem Gros der Lehrmeinung die Schwestergruppenbeziehung der Primates und der Sundatheria bestätigt werden. Zwecks eines umfassenderen Ansatzes wurden im Rahmen einer „total evidence“-Methodik dental- und tarsalmorphologische Merkmale integriert. Das Resultat der Clusteranalyse, basierend auf 263 Merkmalen, modifiziert das Zwischenergebnis und befürwortet in Übereinstimmung mit molekularen Daten als Schwestergruppe der Primaten das Taxon Sundatheria (= Dermoptera + Scandentia). Damit konnte erstmals mittels eines konsequenten phylogenetisch-systematischen Ansatzes der Primaten-Grundplan hinsichtlich der Merkmalsausstattung der Hyolaryngealregion mit 27 Merkmalen rekonstruiert werden. Der Primatenursprung kann mit dem Euarchonta-Grundplan rekonstruiert werden. Für die Sundatheria wurden 12 Grundplanmerkmale definiert

Experimental investigation of the reactions 25 Mg(alpha,n)28 Si, 26 Mg(alpha,n)29 Si, 18 O(alpha,n)21 Ne and their impact on stellar nucleosynthesis

In der vorliegenden Dissertation werden die Kernreaktionen 25Mg(alpha,n)28Si, 26Mg(alpha,n)29Si und 18O(alpha,n)21Ne im astrophysikalisch interessanten Energiebereich von E alpha = 1000 keV bis E alpha = 2450 keV untersucht.rnrnDie Experimente wurden am Nuclear Structure Laboratory der University of Notre Dame (USA) mit dem vor Ort befindlichen Van-de-Graaff Beschleuniger KN durchgeführt. Hierbei wurden Festkörpertargets mit evaporiertem Magnesium oder anodisiertem Sauerstoff mit alpha-Teilchen beschossen und die freigesetzten Neutronen untersucht. Zum Nachweis der freigesetzten Neutronen wurde mit Hilfe von Computersimulationen ein Neutrondetektor basierend auf rn3He-Zählrohren konstruiert. Weiterhin wurden aufgrund des verstärkten Auftretens von Hintergrundreaktionen verschiedene Methoden zur Datenanalyse angewendet.rnrnAbschliessend wird mit Hilfe von Netzwerkrechnungen der Einfluss der Reaktionen 25Mg(alpha,n)28Si, 26Mg(alpha,n)29Si und 18O(alpha,n)21Ne auf die stellare Nukleosynthese untersucht.rn

Lattice preferred orientation in omphacite: Examples from the Tauern Window, Austria and the Western Gneiss Region, Norway

It is lively debated how eclogites find their way from deep to mid-crustal levels during exhumation. Different exhumation models for high-pressure and ultrahigh-pressure rocks were suggested in previous studies, based mainly on field observations and less on microstructural studies on the exhumed rocks. The development and improvement of electron microscopy techniques allows it, to focus interest on direct investigations of microstructures and crystallographic properties in eclogites. In this case, it is of importance to study the applicability of crystallographic measurements on eclogites for exhumation processes and to unravel which processes affect eclogite textures. Previous studies suggested a strong relationship between deformation and lattice preferred orientation (LPO) in omphacite but it is still unclear if the deformation is related to the exhumation of eclogites. This study is focused on the questions which processes affect omphacite LPO and if textural investigations of omphacite are applicable for studying eclogite exhumation. Therefore, eclogites from two examples in the Alps and in the Caledonides were collected systematically and investigated with respect to omphacite LPO by using the electron backscattered diffraction (EBSD) technique. Omphacite textures of the Tauern Window (Austria) and the Western Gneiss Region (Norway) were studied to compare lattice preferred orientation with field observations and suggested exhumation models from previous studies. The interpretation of omphacite textures, regarding the deformation regime is mainly based on numerical simulations in previous studies. Omphacite LPO patterns of the Eclogite Zone are clearly independent from any kind of exhumation process. The textures were generated during omphacite growth on the prograde path of eclogite development until metamorphic peak conditions. Field observations in the Eclogite Zone show that kinematics in garnet mica schist, surrounding the eclogites, strongly indicate an extrusion wedge geometry. Stretching lineations show top-N thrusting at the base and a top-S normal faulting with a sinistral shear component at the top of the Eclogite Zone. The different shear sense on both sides of the unit does not affect the omphacite textures in any way. The omphacite lattice preferred orientation patterns of the Western Gneiss Region can not be connected with any exhumation model. The textures were probably generated during the metamorphic peak and reflect the change from subduction to exhumation. Eclogite Zone and Western Gneiss Region differ significantly in size and especially in metamorphic conditions. While the Eclogite Zone is characterized by constant P-T conditions (600-650°C, 20-25 kbar), the Western Gneiss Region contains a wide P-T range from high- to ultrahigh pressure conditions (400-800°C, 20-35 kbar). In contrast to this, the omphacite textures of both units are very similar. This means that omphacite LPO is independent from P-T conditions and therefore from burial depth. Further, in both units, omphacite LPO is independent from grain and subgrain size as well as from any shape preferred orientation (SPO) on grain and subgrain scale. Overall, omphacite lattice preferred orientation are generated on the prograde part of omphacite development. Therefore, textural investigations on omphacite LPO are not applicable to study eclogite exhumation.