Refine
Year of publication
Document Type
- Habilitation Thesis (103) (remove)
Keywords
- Biophysik (3)
- biophysics (3)
- Datenanalyse (2)
- Oberfläche (2)
- Resonanzenergietransfer (2)
- Selbstorganisation (2)
- Stochastische Prozesse (2)
- Zelladhäsion (2)
- carbon nitride (2)
- cell adhesion (2)
Institute
- Institut für Physik und Astronomie (24)
- Institut für Biochemie und Biologie (17)
- Institut für Chemie (15)
- Institut für Geowissenschaften (12)
- Institut für Umweltwissenschaften und Geographie (6)
- Department Sport- und Gesundheitswissenschaften (5)
- Institut für Ernährungswissenschaft (5)
- Institut für Romanistik (4)
- Department Psychologie (2)
- Extern (2)
Eco-physiological processes are expressing the interaction of organisms within an environmental context of their habitat and their degree of adaptation, level of resistance as well as the limits of life in a changing environment. The present study focuses on observations achieved by methods used in this scientific discipline of “Ecophysiology” and to enlarge the scientific context in a broader range of understanding with universal character. The present eco-physiological work is building the basis for classifying and exploring the degree of habitability of another planet like Mars by a bio-driven experimentally approach. It offers also new ways of identifying key-molecules which are playing a specific role in physiological processes of tested organisms to serve as well as potential biosignatures in future space exploration missions with the goal to search for life. This has important implications for the new emerging scientific field of Astrobiology. Astrobiology addresses the study of the origin, evolution, distribution and future of life in the universe. The three fundamental questions which are hidden behind this definition are: how does life begin and evolve? Is there life beyond Earth and, if so, how can we detect it? What is the future of life on Earth and in the universe? It means that this multidisciplinary field encompasses the search for habitable environments in our Solar System and habitable planets outside our Solar System. It comprises the search for the evidence of prebiotic chemistry and life on Mars and other bodies in our Solar System like the icy moons of the Jovian and Saturnian system, laboratory and field research into the origins and early evolution of life on Earth, and studies of the potential for life to adapt to challenges on Earth and in space. For this purpose an integrated research strategy was applied, which connects field research, laboratory research allowing planetary simulation experiments with investigation enterprises performed in space (particularly performed in the low Earth Orbit.
This cumulative habilitation thesis presents new work on the systematics, paleoecology, and evolution of antelopes and other large mammals, focusing mainly on the late Miocene to Pleistocene terrestrial fossil record of Africa and Arabia. The studies included here range from descriptions of new species to broad-scale analyses of diversification and community evolution in large mammals over millions of years. A uniting theme is the evolution, across both temporal and spatial scales, of the environments and faunas that characterize modern African savannas today. One conclusion of this work is that macroevolutionary changes in large mammals are best characterized at regional (subcontinental to continental) and long-term temporal scales. General views of evolution developed on records that are too restricted in spatial and temporal extent are likely to ascribe too much influence to local or short-lived events. While this distinction in the scale of analysis and interpretation may seem trivial, it is challenging to implement given the geographically and temporally uneven nature of the fossil record, and the difficulties of synthesizing spatially and temporally dispersed datasets. This work attempts to do just that, bringing together primary fossil discoveries from eastern Africa to Arabia, from the Miocene to the Pleistocene, and across a wide range of (mainly large mammal) taxa. The end result is support for hypotheses stressing the impact of both climatic and biotic factors on long-term faunal change, and a more geographically integrated view of evolution in the African fossil record.
Continental rift systems open up unique possibilities to study the geodynamic system of our planet: geodynamic localization processes are imprinted in the morphology of the rift by governing the time-dependent activity of faults, the topographic evolution of the rift or by controlling whether a rift is symmetric or asymmetric. Since lithospheric necking localizes strain towards the rift centre, deformation structures of previous rift phases are often well preserved and passive margins, the end product of continental rifting, retain key information about the tectonic history from rift inception to continental rupture.
Current understanding of continental rift evolution is based on combining observations from active rifts with data collected at rifted margins. Connecting these isolated data sets is often accomplished in a conceptual way and leaves room for subjective interpretation. Geodynamic forward models, however, have the potential to link individual data sets in a quantitative manner, using additional constraints from rock mechanics and rheology, which allows to transcend previous conceptual models of rift evolution. By quantifying geodynamic processes within continental rifts, numerical modelling allows key insight to tectonic processes that operate also in other plate boundary settings, such as mid ocean ridges, collisional mountain chains or subduction zones.
In this thesis, I combine numerical, plate-tectonic, analytical, and analogue modelling approaches, whereas numerical thermomechanical modelling constitutes the primary tool. This method advanced rapidly during the last two decades owing to dedicated software development and the availability of massively parallel computer facilities. Nevertheless, only recently the geodynamical modelling community was able to capture 3D lithospheric-scale rift dynamics from onset of extension to final continental rupture.
The first chapter of this thesis provides a broad introduction to continental rifting, a summary of the applied rift modelling methods and a short overview of previews studies. The following chapters, which constitute the main part of this thesis feature studies on plate boundary dynamics in two and three dimension followed by global scale analyses (Fig. 1).
Chapter II focuses on 2D geodynamic modelling of rifted margin formation. It highlights the formation of wide areas of hyperextended crustal slivers via rift migration as a key process that affected many rifted margins worldwide. This chapter also contains a study of rift velocity evolution, showing that rift strength loss and extension velocity are linked through a dynamic feed-back. This process results in abrupt accelerations of the involved plates during rifting illustrating for the first time that rift dynamics plays a role in changing global-scale plate motions. Since rift velocity affects key processes like faulting, melting and lower crustal flow, this study also implies that the slow-fast velocity evolution should be imprinted in rifted margin structures.
Chapter III relies on 3D Cartesian rift models in order to investigate various aspects of rift obliquity. Oblique rifting occurs if the extension direction is not orthogonal to the rift trend. Using 3D lithospheric-scale models from rift initialisation to breakup I could isolate a characteristic evolution of dominant fault orientations. Further work in Chapter III addresses the impact of rift obliquity on the strength of the rift system. We illustrate that oblique rifting is mechanically preferred over orthogonal rifting, because the brittle yielding requires a lower tectonic force. This mechanism elucidates rift competition during South Atlantic rifting, where the more oblique Equatorial Atlantic Rift proceeded to breakup while the simultaneously active but less oblique West African rift system became a failed rift. Finally this Chapter also investigates the impact of a previous rift phase on current tectonic activity in the linkage area of the Kenyan with Ethiopian rift. We show that the along strike changes in rift style are not caused by changes in crustal rheology. Instead the rift linkage pattern in this area can be explained when accounting for the thinned crust and lithosphere of a Mesozoic rift event.
Chapter IV investigates rifting from the global perspective. A first study extends the oblique rift topic of the previous chapter to global scale by investigating the frequency of oblique rifting during the last 230 million years. We find that approximately 70% of all ocean-forming rift segments involved an oblique component of extension where obliquities exceed 20°. This highlights the relevance of 3D approaches in modelling, surveying, and interpretation of many rifted margins. In a final study, we propose a link between continental rift activity, diffuse CO2 degassing and Mesozoic/Cenozoic climate changes. We used recent CO2 flux measurements in continental rifts to estimate worldwide rift-related CO2 release, which we based on the global extent of rifts through time. The first-order correlation to paleo-atmospheric CO2 proxy data suggests that rifts constitute a major element of the global carbon cycle.
The anatomically modern human Homo sapiens sapiens is distinguished by a high adaptability in physiology, physique and behaviour in short term changing environmental conditions. Since our environmental factors are constantly changing because of anthropogenic influences, the question arises as to how far we have an impact on the human phenotype in the very sensitive growth phase in children and adolescents. Growth and development of all children and adolescents follow a universal and typical pattern. This pattern has evolved as the result of trade-offs in the 6-7 million years of human evolution. This typically human growth pattern differs from that of other long-living social primate species. It can be divided into different biological age stages, with specific biological, cognitive and socio-cultural signs. Phenotypic plasticity is the ability of an organism to react to an internal or external environmental input with a change in the form, state, and movement rate of activity (West-Eberhard 2003). The plasticity becomes visible and measurable particularly when, in addition to the normal variability of the phenotypic characteristics within a population, the manifestation of this plasticity changes within a relatively short time. The focus of the present work is the comparison of age-specific dimensional changes. The basic of the presented studies are more than 75,000 anthropometric data-sets of children and adolescence from 1980 up today and historical data of height available in scientific literature. Due to reduced daily physical activity, today's 6-18 year-olds have lower values of pelvic and elbow breadths. The observed increase in body height can be explained by hierarchies in social networks of human societies, contrary to earlier explanations (influence of nutrition, good living conditions and genetics). A shift towards a more feminine fat distribution pattern in boys and girls is parallel to the increase in chemicals in our environment that can affect the hormone system. Changing environmental conditions can have selective effects over generations so that that genotype becomes increasingly prevalent whose individuals have a higher progeny rate than other individuals in this population. Those then form the phenotype which allows optimum adaptation to the changes of the environmental conditions. Due to the slow patterns of succession and the low progeny rate (Hawkes et al. 1998), fast visible in the phenotype due to changes in the genotype of a population are unlikely to occur in the case of Homo sapiens sapiens within short time. In the data sets on which the presented investigations are based, such changes appear virtually impossible. The study periods cover 5-30 to max.100 years (based on data from the body height from historical data sets).
Die klassische Physik/Chemie unterscheidet zwischen drei Bindungstypen: Der kovalenten Bindung, der ionischen Bindung und der metallischen Bindung. Moleküle untereinander werden hingegen durch schwache Wechselwirkungen zusammen gehalten, sie sind trotz ihrer schwachen Kräfte weniger verstanden, aber dabei nicht weniger wichtig. In zukunftsweisenden Gebieten wie der Nanotechnologie, der Supramolekularen Chemie und Biochemie sind sie von elementarer Bedeutung.
Um schwache, intermolekulare Wechselwirkungen zu beschreiben, vorauszusagen und zu verstehen, sind sie zunächst theoretisch zu erfassen. Hierzu gehören verschiedene quantenchemische Methoden, die in dieser Arbeit vorgestellt, verglichen, weiterentwickelt und schließlich auch exemplarisch auf Problemstellungen in der Chemie angewendet werden. Aufbauend auf einer Hierarchie von Methoden unterschiedlicher Genauigkeit werden sie für diese Ziele eingesetzt, ausgearbeitet und kombiniert.
Berechnet wird die Elektronenstruktur, also die Verteilung und Energie von Elektronen, die im Wesentlichen die Atome zusammen halten. Da Ungenauigkeiten von der Beschreibung der Elektronenstruktur von den verwendeten Methoden abhängen, kann man die Effekte detailliert untersuchen, sie beschreiben und darauf aufbauend weiter entwickeln, um sie anschließend an verschiedenen Modellen zu testen. Die Geschwindigkeit der Berechnungen mit modernen Computern ist eine wesentliche, zu berücksichtigende Komponente, da im Allgemeinen die Genauigkeit mit der Rechenzeit exponentiell steigt, und die damit an die Grenzen der Möglichkeiten stoßen muss.
Die genaueste der verwendeten Methoden basiert auf der Coupled-Cluster-Theorie, die sehr gute Voraussagen ermöglicht. Für diese wird eine sogenannte spektroskopische Genauigkeit mit Abweichungen von wenigen Wellenzahlen erzielt, was Vergleiche mit experimentellen Daten zeigen. Eine Möglichkeit zur Näherung von hochgenauen Methoden basiert auf der Dichtefunktionaltheorie: Hier wurde das „Boese-Martin for Kinetics“ (BMK)-Funktional entwickelt, dessen Funktionalform sich in vielen nach 2010 veröffentlichten Dichtefunktionalen wiederfindet.
Mit Hilfe der genaueren Methoden lassen sich schließlich semiempirische Kraftfelder zur Beschreibung intermolekularer Wechselwirkungen für individuelle Systeme parametrisieren, diese benötigen weit weniger Rechenzeit als die Methoden, die auf der genauen Berechnung der Elektronenstruktur von Molekülen beruhen.
Für größere Systeme lassen sich auch verschiedene Methoden kombinieren. Dabei wurden Einbettungsverfahren verfeinert und mit neuen methodischen Ansätzen vorgeschlagen. Sie verwenden sowohl die symmetrieadaptierte Störungstheorie als auch die quantenchemische Einbettung von Fragmenten in größere, quantenchemisch berechnete Systeme.
Die Entwicklungen neuer Methoden beziehen ihren Wert im Wesentlichen durch deren Anwendung:
In dieser Arbeit standen zunächst die Wasserstoffbrücken im Vordergrund. Sie zählen zu den stärkeren intermolekularen Wechselwirkungen und sind nach wie vor eine Herausforderung. Im Gegensatz dazu sind van-der-Waals Wechselwirkungen relativ einfach durch Kraftfelder zu beschreiben. Deshalb sind viele der heute verwendeten Methoden für Systeme, in denen Wasserstoffbrücken dominieren, vergleichsweise schlecht.
Eine Untersuchung molekularer Aggregate mit Auswirkungen intermolekularer Wechselwirkungen auf die Schwingungsfrequenzen von Molekülen schließt sich an. Dabei wird auch über die sogenannte starrer-Rotor-harmonischer-Oszillator-Näherung hinausgegangen.
Eine weitreichende Anwendung behandelt Adsorbate, hier die von Molekülen auf ionischen/metallischen Oberflächen. Sie können mit ähnlichen Methoden behandelt werden wie die intermolekularen Wechselwirkungen, und sind mit speziellen Einbettungsverfahren sehr genau zu beschreiben. Die Resultate dieser theoretischen Berechnungen stimulierten eine Neubewertung der bislang bekannten experimentellen Ergebnisse.
Molekulare Kristalle sind ein äußerst wichtiges Forschungsgebiet. Sie werden durch schwache Wechselwirkungen zusammengehalten, die von van-der-Waals Kräften bis zu Wasserstoffbrücken reichen. Auch hier wurden neuentwickelte Methoden eingesetzt, die eine interessante, mindestens ebenso genaue Alternative zu den derzeit gängigen Methoden darstellen.
Von daher sind die entwickelten Methoden, als auch deren Anwendung äußerst vielfältig. Die behandelten Berechnungen der Elektronenstruktur erstrecken sich von den sogenannten post-Hartree-Fock-Methoden über den Einsatz der Dichtefunktionaltheorie bis zu semiempirischen Kraftfeldern und deren Kombinationen. Die Anwendung reicht von einzelnen Molekülen in der Gasphase über die Adsorption auf Oberflächen bis zum molekularen Festkörper.
Ferroelectrets are internally charged polymer foams or cavity-containing polymer-_lm systems that combine large piezoelectricity with mechanical flexibility and elastic compliance. The term “ferroelectret” was coined based on the fact that it is a space-charge electret that also shows ferroic behavior. In this thesis, comprehensive work on ferroelectrets, and in particular on their preparation, their charging, their piezoelectricity and their applications is reported.
For industrial applications, ferroelectrets with well-controlled distributions or even uniform values of cavity size and cavity shape and with good thermal stability of the piezoelectricity are very desirable. Several types of such ferroelectrets are developed using techniques such as straightforward thermal lamination, sandwiching sticky templates with electret films, and screen printing. In particular, uoroethylenepropylene (FEP) _lm systems with tubular-channel openings, prepared by means of the thermal lamination technique, show piezoelectric d33 coefficients of up to 160 pC/N after charging through dielectric barrier discharges (DBDs) . For samples charged at suitable elevated temperatures, the piezoelectricity is stable at temperatures of at least 130°C. These preparation methods are easy to implement at laboratory or industrial scales, and are quite flexible in terms of material selection and cavity geometry design. Due to the uniform and well-controlled cavity structures, samples are also very suitable for fundamental studies on ferroelectrets.
Charging of ferroelectrets is achieved via a series of dielectric barrier discharges (DBDs) inside the cavities. In the present work, the DBD charging process is comprehensively studied by means of optical, electrical and electro-acoustic methods. The spectrum of the transient light from the DBDs in cellular polypropylene (PP) ferroelectrets directly confirms the ionization of molecular nitrogen, and allows the determination of the electric field in the discharge. Detection of the light emission reveals not only DBDs under high applied voltage but also back discharges when the applied voltage is reduced to sufficiently low values. Back discharges are triggered by the internally deposited charges, as the breakdown inside the cavities is controlled by the sum of the applied electric field and the electric field of the deposited charges. The remanent effective polarization is determined by the breakdown strength of the gas-filled cavities. These findings form the basis of more efficient charging techniques for ferroelectrets such as charging with high-pressure air, thermal poling and charging assisted by gas exchange. With the proposed charging strategies, the charging efficiency of ferroelectrets can be enhanced significantly.
After charging, the cavities can be considered as man-made macroscopic dipoles whose direction can be reversed by switching the polarity of the applied voltage. Polarization-versus-electric-field (P(E)) hysteresis loops in ferroelectrets are observed by means of an electro-acoustic method combined with dielectric resonance spectroscopy. P(E) hysteresis loops in ferrroelectrets are also obtained by more direct measurements using a modified Sawyer-Tower circuit. Hysteresis loops prove the ferroic behavior of ferroelectrets. However, repeated switching of the macroscopic dipoles involves complex physico-chemical processes. The DBD charging process generates a cold plasma with numerous active species and thus modifies the inner polymer surfaces of the cavities. Such treatments strongly affect the chargeability of the cavities. At least for cellular PP ferroelectrets, repeated DBDs in atmospheric conditions lead to considerable fatigue of the effective polarization and of the resulting piezoelectricity.
The macroscopic dipoles in ferroelectrets are highly compressible, and hence the piezoelectricity is essentially the primary effect. It is found that the piezoelectric d33 coefficient is proportional to the polarization and the elastic compliance of the sample, providing hints for developing materials with higher piezoelectric sensitivity in the future. Due to their outstanding electromechanical properties, there has been constant interest in the application of ferroelectrets. The antiresonance frequencies (fp) of ferroelectrets are sensitive to the boundary conditions during measurement. A tubular-channel FEP ferroelectret is conformably attached to a self-organized minimum-energy dielectric elastomer actuator (DEA). It turns out that the antiresonance frequency (fp) of the ferroelectret film changes noticeably with the bending angle of the DEA. Therefore, the actuation of DEAs can be used to modulate the fp value of ferroelectrets, but fp can also be exploited for in-situ diagnosis and for precise control of the actuation of the DEA. Combination of DEAs and ferroelectrets opens up various new possibilities for application.