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The geochemical composition of oceanic basalts provides us with a window into the distribution of geochemical elements within the Earth’s mantle in space and time. In conjunction with a throughout knowledge on how the different elements behave e.g. during melt formation and evolution or on their partition behaviour between e.g. minerals and melts this information has been transformed into various models on how oceanic crust is formed along plume influenced or normal mid-ocean ridge segments, how oceanic crust evolves in response to seawater, on subduction recycling of oceanic crust and so forth. The work presented in this habilitation was aimed at refining existing models, putting further constraints on some of the major open questions in this field of research while at the same time trying to increase our knowledge on the behaviour of noble gases as a tracer for melt formation and evolution processes. In the line of this work the author and her co-workers were able to answer one of the major questions concerning the formation of oceanic crust along plume-influenced ridges – in which physical state does the plume material enter the ridge? Based on submarine volcanic glass He, Ne and Ar data, the author and her co-workers have shown that the interaction of mantle plumes with mid-ocean ridges occurs in the physical form of melts. In addition, the author and her co-workers have also put further constraints on one of the major questions concerning the formation of oceanic crust along normal mid-ocean ridges – namely how is the mid-ocean ridge system effectively cooled to form the lower oceanic crust? Based on Ne and Ar data in combination with Cl/K ratios of basaltic glass from the Mid-Atlantic ridge and estimates of crystallisation pressures they have shown, that seawater penetration reaches lower crustal levels close to the Moho, indicating that hydrothermal circulation might be an effective cooling mechanism even for the deep parts of the oceanic crust. Considering subduction recycling, the heterogeneity of the Earth’s mantle and mantle dynamic processes the key question is on which temporal and spatial scales is the Earth’s mantle geochemically heterogeneous? In the line of this work the author along with her co-workers have shown based on Cl/K ratios in conjunction with the Sr, Nd, and Pb isotopes of the OIBs representing the type localities for the different mantle endmembers that the quantity of Cl recycled into the mantle via subduction is not uniform and that neither the HIMU nor the EM1 and EM2 mantle components can be considered as distinct mantle endmembers. In addition, we have shown, based on He, Ne and Ar isotope and trace-element data from the Foundation hotspot that the near ridge seamounts of the Foundation seamount chain formed by the Foundation hotspot erupt lavas with a trace-element signature clearly characteristic of oceanic gabbro which indicates the existence of recycled, virtually unchanged lower oceanic crust in the plume source. This is a clear sign of the inefficiency of the stirring mechanism existing at mantle depth. Similar features are seen in other near-axis hotspot magmas around the world. Based on He, Sr, Nd, Pb and O isotopes and trace elements in primitive mafic dykes from the Etendeka flood basalts, NW Namibia the author along with her co-workers have shown that deep, less degassed mantle material carried up by a mantle plume contributed significantly to the flood basalt magmatism. The Etendeka flood basalts are part of the South Atlantic LIP, which is associated with the breakup of Gondwana, the formation of the Paraná-Etendeka flood basalts and the Walvis Ridge - Tristan da Cunha hotspot track. Thus reinforcing the lately often-challenged concept of mantle plumes and the role of mantle plumes in the formation of large igneous provinces. Studying the behaviour of noble gases during melt formation and evolution the author along with her co-workers has shown that He can be considerable more susceptible to changes during melt formation and evolution resulting not only in a complete decoupling of He isotopes from e.g. Ne or Pb isotopes but also in a complete loss of the primary mantle isotope signal. They have also shown that this decoupling occurs mainly during the melt formation processes requiring He to be more compatible during mantle melting than Ne. In addition, the author along with her co workers were able to show that incorporation of atmospheric noble gases into igneous rocks is in general a two-step process: (1) magma contamination by assimilation of altered oceanic crust results in the entrainment of air-equilibrated seawater noble gases; (2) atmospheric noble gases are adsorbed onto grain surfaces during sample preparation. This implies, considering the ubiquitous presence of the contamination signal, that magma contamination by assimilation of a seawater-sourced component is an integral part of mid-ocean ridge basalt evolution.
Und der Zukunft abgewandt
(2010)
Seit dem Ende der DDR, das den Zusammenbruch des Ostblocks und damit die Beendigung des »Kalten Kriegs« einleitete, wird verstärkt versucht, das Wesen dieses Staates zu definieren und damit seine Folgen auf wirtschaftlicher, sozialer, psychologischer und bildungspolitischer Ebene zu verstehen und einzuordnen. Alexandra Budke analysiert in diesem Band das Schulfach Geographie, das neben der Staatsbürgerkunde und der Geschichte ein zentrales Fach war und in dem die in den Lehrplänen definierte »staatsbürgerliche, weltanschauliche oder ideologische Erziehung« auf der Grundlage des Marxismus-Leninismus stattfinden sollte. Sie klärt, inwiefern Geographieunterricht in der DDR genutzt wurde, um geopolitische Interessen des Staates zu kommunizieren und zu verbreiten. Damit lässt sich durch die detaillierte Analyse des Fachunterrichts auch die Frage beantworten, ob SchülerInnen im Unterricht politisch manipuliert wurden und welche Handlungsmöglichkeiten die zentralen Akteure des Unterrichts, die LehrerInnen und die SchülerInnen, im Rahmen der durch die Bildungspolitik gesetzten curricularen Vorgaben wahrgenommen haben.
Proteins are chain molecules built from amino acids. The precise sequence of the 20 different types of amino acids in a protein chain defines into which structure a protein folds, and the three-dimensional structure in turn specifies the biological function of the protein. The reliable folding of proteins is a prerequisite for their robust function. Misfolding can lead to protein aggregates that cause severe diseases, such as Alzheimer's, Parkinson's, or the variant Creutzfeldt-Jakob disease. Small single-domain proteins often fold without experimentally detectable metastable intermediate states. The folding dynamics of these proteins is thought to be governed by a single transition-state barrier between the unfolded and the folded state. The transition state is highly instable and cannot be observed directly. However, mutations in which a single amino acid of the protein is substituted by another one can provide indirect access. The mutations slightly change the transition-state barrier and, thus, the folding and unfolding times of the protein. The central question is how to reconstruct the transition state from the observed changes in folding times. In this habilitation thesis, a novel method to extract structural information on transition states from mutational data is presented. The method is based on (i) the cooperativity of structural elements such as alpha-helices and beta-hairpins, and (ii) on splitting up mutation-induced free-energy changes into components for these elements. By fitting few parameters, the method reveals the degree of structure formation of alpha-helices and beta-hairpins in the transition state. In addition, it is shown in this thesis that the folding routes of small single-domain proteins are dominated by loop-closure dependencies between the structural elements.
This book is concerned with the diachronic development of selected topic and focus markers in Spanish, Portuguese and French. On the one hand, it focuses on the development of these structures from their relational meaning to their topic-/ focus-marking meaning, and on the other hand, it is concerned with their current form und use. Thus, Romance topic and focus markers – such as sp. en cuanto a, pt. a propósito de, fr. au niveau de or sentence-initial sp. Lo que as well as clefts and pseudo-clefts – are investigated from a quantitative and qualitative perspective. The author argues that topic markers have procedural meaning and that their function is bound to their syntactic position. An important contribution of this study is the fact that real linguistic evidence (in the form of data from various corpora) is analyzed instead of operating with constructed examples.
Quantitative thermodynamic and geochemical modeling is today applied in a variety of geological environments from the petrogenesis of igneous rocks to the oceanic realm. Thermodynamic calculations are used, for example, to get better insight into lithosphere dynamics, to constrain melting processes in crust and mantle as well as to study fluid-rock interaction. The development of thermodynamic databases and computer programs to calculate equilibrium phase diagrams have greatly advanced our ability to model geodynamic processes from subduction to orogenesis. However, a well-known problem is that despite its broad application the use and interpretation of thermodynamic models applied to natural rocks is far from straightforward. For example, chemical disequilibrium and/or unknown rock properties, such as fluid activities, complicate the application of equilibrium thermodynamics.
One major aspect of the publications presented in this Habilitationsschrift are new approaches to unravel dynamic and chemical histories of rocks that include applications to chemically open system behaviour. This approach is especially important in rocks that are affected by element fractionation due to fractional crystallisation and fluid loss during dehydration reactions. Furthermore, chemically open system behaviour has also to be considered for studying fluid-rock interaction processes and for extracting information from compositionally zoned metamorphic minerals. In this Habilitationsschrift several publications are presented where I incorporate such open system behaviour in the forward models by incrementing the calculations and considering changing reacting rock compositions during metamorphism. I apply thermodynamic forward modelling incorporating the effects of element fractionation in a variety of geodynamic and geochemical applications in order to better understand lithosphere dynamics and mass transfer in solid rocks.
In three of the presented publications I combine thermodynamic forward models with trace element calculations in order to enlarge the application of geochemical numerical forward modeling. In these publications a combination of thermodynamic and trace element forward modeling is used to study and quantify processes in metamorphic petrology at spatial scales from µm to km. In the thermodynamic forward models I utilize Gibbs energy minimization to quantify mineralogical changes along a reaction path of a chemically open fluid/rock system. These results are combined with mass balanced trace element calculations to determine the trace element distribution between rock and melt/fluid during the metamorphic evolution. Thus, effects of mineral reactions, fluid-rock interaction and element transport in metamorphic rocks on the trace element and isotopic composition of minerals, rocks and percolating fluids or melts can be predicted.
One of the included publications shows that trace element growth zonations in metamorphic garnet porphyroblasts can be used to get crucial information about the reaction path of the investigated sample. In order to interpret the major and trace element distribution and zoning patterns in terms of the reaction history of the samples, we combined thermodynamic forward models with mass-balance rare earth element calculations. Such combined thermodynamic and mass-balance calculations of the rare earth element distribution among the modelled stable phases yielded characteristic zonation patterns in garnet that closely resemble those in the natural samples. We can show in that paper that garnet growth and trace element incorporation occurred in near thermodynamic equilibrium with matrix phases during subduction and that the rare earth element patterns in garnet exhibit distinct enrichment zones that fingerprint the minerals involved in the garnet-forming reactions.
In two of the presented publications I illustrate the capacities of combined thermodynamic-geochemical modeling based on examples relevant to mass transfer in subduction zones. The first example focuses on fluid-rock interaction in and around a blueschist-facies shear zone in felsic gneisses, where fluid-induced mineral reactions and their effects on boron (B) concentrations and isotopic compositions in white mica are modeled. In the second example, fluid release from a subducted slab and associated transport of B and variations in B concentrations and isotopic compositions in liberated fluids and residual rocks are modeled. I show that, combined with experimental data on elemental partitioning and isotopic fractionation, thermodynamic forward modeling unfolds enormous capacities that are far from exhausted.
In my publications presented in this Habilitationsschrift I compare the modeled results to geochemical data of natural minerals and rocks and demonstrate that the combination of thermodynamic and geochemical models enables quantification of metamorphic processes and insights into element cycling that would have been unattainable so far.
Thus, the contributions to the science community presented in this Habilitatonsschrift concern the fields of petrology, geochemistry, geochronology but also ore geology that all use thermodynamic and geochemical models to solve various problems related to geo-materials.
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.
The habilitation thesis presented here includes results from several studies dealing with fluid-rock interactions and rock deformation processes in active fault zones. The focus in all of these studies is on the influence of clay minerals on the geochemical and the hydro-mechanical behavior of the fault rocks. The research was conducted on rock cores and cuttings from four scientific drilling projects at the San Andreas Fault (USA), the Nankai Trough subduction zone and the Japan Trench subduction zone (Japan), as well as the Alpine Fault in New Zealand. These ICDP (International Continental Scientific Drilling Program) and IODP (International Ocean Discovery Program) funded projects were all conducted with the aim to monitor and better understand earthquakes.
Chapter 1 contains a short introduction to the topic with basic principles and objectives regarding the research approach. Chapter 2 describes the state of the art in clay mineral and fault zone science, gives a short description of the individual drilling projects and their locations on which the research was based, and summarizes the most important analytical methods used. Chapter 3 comprises ten peer-reviewed publications that are connected thematically and methodologically. The papers were published in the years 2006-2015, and additional related publications including myself as co-author are given in the literature list. The ten publications address different questions concerning the formation of clay minerals and processes of fluid-rock interaction in active fault zones. Six papers contain results from the SAFOD drilling project, USA (San Andreas Fault Observatory at Depth), with the main focus on fluid-rock interaction processes in fault rocks and the formation and location of clay minerals. Three publications report on research from the NanTroSEIZE drilling project (Nankai Trough Seismogenic Zone Experiment) and the JFAST drilling project (Japan Trench Fast Drilling Project). Both projects are situated in Japan. Here, the swelling behavior of smectite clay minerals in relation to changing environmental conditions (e.g. temperature and/or humidity) was investigated. The last publication included here concerns a study from the DFDP project (Deep Fault Drilling Project) in New Zealand, where I investigated the deformation of clay minerals on the context of the hydro-mechanical behavior of the fault zone rocks. I was first author in nine of the publications and in charge of the project preparation, measurements and data analyses, and the completion of the manuscript. As co-author on the other publication I was responsible for electronmicroscopy analyses (SEM and TEM) and their interpretation.
The key results from the publications in Chapter 3 are discussed in Chapter 4 with additional considerations from more recent papers. Following the major theses in Chapter 5, Chapter 6 highlights a future research project in clay mineralogy research at the GFZ. An appendix includes more detailed descriptions of the laboratory equipment and lists of all publications, conference contributions and teaching courses and modules.
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.
Understanding the formation of stars in galaxies is central to much of modern astrophysics. For several decades it has been thought that the star formation process is primarily controlled by the interplay between gravity and magnetostatic support, modulated by neutral-ion drift. Recently, however, both observational and numerical work has begun to suggest that supersonic interstellar turbulence rather than magnetic fields controls star formation. This review begins with a historical overview of the successes and problems of both the classical dynamical theory of star formation, and the standard theory of magnetostatic support from both observational and theoretical perspectives. We then present the outline of a new paradigm of star formation based on the interplay between supersonic turbulence and self-gravity. Supersonic turbulence can provide support against gravitational collapse on global scales, while at the same time it produces localized density enhancements that allow for collapse on small scales. The efficiency and timescale of stellar birth in Galactic gas clouds strongly depend on the properties of the interstellar turbulent velocity field, with slow, inefficient, isolated star formation being a hallmark of turbulent support, and fast, efficient, clustered star formation occurring in its absence. After discussing in detail various theoretical aspects of supersonic turbulence in compressible self-gravitating gaseous media relevant for star forming interstellar clouds, we explore the consequences of the new theory for both local star formation and galactic scale star formation. The theory predicts that individual star-forming cores are likely not quasi-static objects, but dynamically evolving. Accretion onto these objects will vary with time and depend on the properties of the surrounding turbulent flow. This has important consequences for the resulting stellar mass function. Star formation on scales of galaxies as a whole is expected to be controlled by the balance between gravity and turbulence, just like star formation on scales of individual interstellar gas clouds, but may be modulated by additional effects like cooling and differential rotation. The dominant mechanism for driving interstellar turbulence in star-forming regions of galactic disks appears to be supernovae explosions. In the outer disk of our Milky Way or in low-surface brightness galaxies the coupling of rotation to the gas through magnetic fields or gravity may become important.
Biological materials, in addition to having remarkable physical properties, can also change shape and volume. These shape and volume changes allow organisms to form new tissue during growth and morphogenesis, as well as to repair and remodel old tissues. In addition shape or volume changes in an existing tissue can lead to useful motion or force generation (actuation) that may even still function in the dead organism, such as in the well known example of the hygroscopic opening or closing behaviour of the pine cone. Both growth and actuation of tissues are mediated, in addition to biochemical factors, by the physical constraints of the surrounding environment and the architecture of the underlying tissue. This habilitation thesis describes biophysical studies carried out over the past years on growth and swelling mediated shape changes in biological systems. These studies use a combination of theoretical and experimental tools to attempt to elucidate the physical mechanisms governing geometry controlled tissue growth and geometry constrained tissue swelling. It is hoped that in addition to helping understand fundamental processes of growth and morphogenesis, ideas stemming from such studies can also be used to design new materials for medicine and robotics.
The ecohydrological transfers, interactions and degradation arising from high-intensity storm events
(2015)
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).
In this thesis, a collection of studies is presented that advance research on complex food webs in several directions. Food webs, as the networks of predator-prey interactions in ecosystems, are responsible for distributing the resources every organism needs to stay alive. They are thus central to our understanding of the mechanisms that support biodiversity, which in the face of increasing severity of anthropogenic global change and accelerated species loss is of highest importance, not least for our own well-being.
The studies in the first part of the thesis are concerned with general mechanisms that determine the structure and stability of food webs. It is shown how the allometric scaling of metabolic rates with the species' body masses supports their persistence in size-structured food webs (where predators are larger than their prey), and how this interacts with the adaptive adjustment of foraging efforts by consumer species to create stable food webs with a large number of coexisting species. The importance of the master trait body mass for structuring communities is further exemplified by demonstrating that the specific way the body masses of species engaging in empirically documented predator-prey interactions affect the predator's feeding rate dampens population oscillations, thereby helping both species to survive. In the first part of the thesis it is also shown that in order to understand certain phenomena of population dynamics, it may be necessary to not only take the interactions of a focal species with other species into account, but to also consider the internal structure of the population. This can refer for example to different abundances of age cohorts or developmental stages, or the way individuals of different age or stage interact with other species.
Building on these general insights, the second part of the thesis is devoted to exploring the consequences of anthropogenic global change on the persistence of species. It is first shown that warming decreases diversity in size-structured food webs. This is due to starvation of large predators on higher trophic levels, which suffer from a mismatch between their respiration and ingestion rates when temperature increases. In host-parasitoid networks, which are not size-structured, warming does not have these negative effects, but eutrophication destabilises the systems by inducing detrimental population oscillations. In further studies, the effect of habitat change is addressed. On the level of individual patches, increasing isolation of habitat patches has a similar effect as warming, as it leads to decreasing diversity due to the extinction of predators on higher trophic levels. In this case it is caused by dispersal mortality of smaller and therefore less mobile species on lower trophic levels, meaning that an increasing fraction of their biomass production is lost to the inhospitable matrix surrounding the habitat patches as they become more isolated. It is further shown that increasing habitat isolation desynchronises population oscillations between the patches, which in itself helps species to persist by dampening fluctuations on the landscape level. However, this is counteracted by an increasing strength of local population oscillations fuelled by an indirect effect of dispersal mortality on the feeding interactions. Last, a study is presented that introduces a novel mechanism for supporting diversity in metacommunities. It builds on the self-organised formation of spatial biomass patterns in the landscape, which leads to the emergence of spatio-temporally varying selection pressures that keep local communities permanently out of equilibrium and force them to continuously adapt. Because this mechanism relies on the spatial extension of the metacommunity, it is also sensitive to habitat change.
In the third part of the thesis, the consequences of biodiversity for the functioning of ecosystems are explored. The studies focus on standing stock biomass, biomass production, and trophic transfer efficiency as ecosystem functions. It is first shown that increasing the diversity of animal communities increases the total rate of intra-guild predation. However, the total biomass stock of the animal communities increases nevertheless, which also increases their exploitative pressure on the underlying plant communities. Despite this, the plant communities can maintain their standing stock biomass due to a shift of the body size spectra of both animal and plant communities towards larger species with a lower specific respiration rate. In another study it is further demonstrated that the generally positive relationship between diversity and the above mentioned ecosystem functions becomes steeper when not only the feeding interactions but also the numerous non-trophic interactions (like predator interference or competition for space) between the species of an ecosystem are taken into account. Finally, two studies are presented that demonstrate the power of functional diversity as explanatory variable. It is interpreted as the range spanned by functional traits of the species that determine their interactions. This approach allows to mechanistically understand how the ecosystem functioning of food webs with multiple trophic levels is affected by all parts of the food web and why a high functional diversity is required for efficient transportation of energy from primary producers to the top predators.
The general discussion draws some synthesising conclusions, e.g. on the predictive power of ecosystem functioning to explain diversity, and provides an outlook on future research directions.
The direct conversion of light from the sun into usable forms of energy marks one of the central cornerstones of the change of our living from the use of fossil, non-renewable energy resources towards a more sustainable economy. Besides the necessary societal changes necessary, it is the understanding of the solids employed that is of particular importance for the success of this target. In this work, the principles and approaches of systematic-crystallographic characterisation and systematisation of solids is used and employed to allow a directed tuning of the materials properties. The thorough understanding of the solid-state forms hereby the basis, on which more applied approaches are founded.
Two material systems, which are considered as promising solar absorber materials, are at the core of this work: halide perovskites and II-IV-N2 nitride materials. While the first is renowned for its high efficiencies and rapid development in the last years, the latter is putting an emphasis on true sustainability in that toxic and scarce elements are avoided.
Das Therapiemanagement bei Lipödem stellt auf Grund unzureichenden Wissensstandes in entscheidenden Aspekten eine besondere Herausforderung dar. Da die Pathogenese der Erkrankung nicht hinreichend geklärt ist und bislang kein pathognomonisches Diagnostikkriterium definiert wurde, beklagen viele Betroffene einen langjährigen Leidensweg bis zur Einleitung von Therapiemaßnahmen. Durch Steigerung der Awareness der Erkrankung in den letzten Jahren konnten die Intervalle bis zur korrekten Diagnose erfreulicherweise erheblich verkürzt werden. Obwohl die Zuordnung der Beschwerden zu einer klar definierten Erkrankung für viele Patientinnen eine Erleichterung ist, stellt die Erkenntnis über begrenzte Therapiemöglichkeiten häufig eine neuerliche Belastung dar.
Als Konsequenz der ungeklärten Pathogenese konnte bis dato keine kausale Therapie für das Lipödem definiert werden. Zu Beginn waren die Möglichkeiten konservativer Behandlungsstrategien nur eingeschränkt in den Rahmen eines allgemeingültigen Konzeptes involviert und insbesondere Limitationen nicht klar definiert. Obwohl in diversen Bereichen der Therapie weiterhin keine ausreichende Evidenz besteht, konnten durch eine systematische Aufarbeitung die grundsätzlichen Behandlungsoptionen in Relation zueinander gesetzt werden. Betroffene Patientinnen, sowie die verschiedenen in die Behandlung integrierte medizinische Disziplinen verfügen somit über einen grundsätzlichen Handlungsalgorithmus, deren Empfehlungen über einfache Rezeptierung von Lymphdrainage und Kompressionsbekleidung hinausgehen. Durch kritische Reflexion der geltenden Dogmata wurde ein interdisziplinärer Leitfaden vorgeschlagen, der auf nachvollziehbare Weise im Sinne eines Stufenschemas alle wesentlichen Therapiesäulen in einen allgemeingültigen Behandlungsplan einbindet.
Im vielschichten Management der Erkrankung verbleibt die operative Behandlung, die Liposuktion, allerdings häufig als „ultima ratio“ nach ausbleibender Linderung unter konservativen Therapiemaßnahmen. Die wesentliche Zielstellung der vorliegenden Arbeit konzentriert sich demnach auf die Optimierung des operativen Vorgehens in der Durchführung von Liposuktionen bei Patientinnen mit Lipödem und zeigt sowohl Grenzen der Indikationsstellung, als auch Potenzial des Behandlungserfolges im Langzeitverlauf auf. Langzeitergebnisse zeigen, dass die Liposuktion als sicherer Eingriff mit dem Potenzial einer nachhaltigen Symptomreduktion für Lipödem-Patientinnen angesehen werden kann. Betont werden soll zudem die Notwendigkeit der Verzahnung operativer Maßnahmen mit konservativen Therapien und somit die Integration der Liposuktion als sinnvolle Behandlungsalternative in ein klar umrissenes Therapiekonzept.
Methodisch greift die Arbeit auf insgesamt 10 Publikationen zurück. Die hier postulierte mehrzeitige Megaliposuktion zur Therapie des Lipödems, mit summierten Gesamtaspirationsvolumina über alle Eingriffe von bis zu 66.000 ml, konnte als evidenzbasiertes Therapieverfahren bestätigt und validiert werden. Die beschriebenen niedrigen Komplikationsraten sind unter Anderem Resultat einer differenzierten, individualisierten perioperativen Strategie. Neben der Berücksichtigung grundsätzlicher methodischer Prinzipien existieren allerdings vielfältige Variationen, deren Implikationen auf Komplikationsraten jeweils differenziert zu betrachten sind. Es existiert zwar kein Konsensus für ein allgemeingültiges Standardverfahren der Liposuktion, allerdings konnten zahlreiche Elemente im perioperativen Management definiert werden, die unabhängig von der verwendeten Operationstechnik einen potenziellen positiven Einfluss auf das Outcome haben. Obwohl die Liposuktion bei Lipödem somit zusammenfassend mittlerweile als sicheres Verfahren gelten kann, sind einige Aspekte weiterhin nicht abschließend geklärt. Hierbei stehen vor allem das Volumenmanagement und die standardisierte Festlegung des maximalen Aspirationsvolumens im Fokus.
Die Analyse verschiedener Kovariablen auf die Linderung Lipödem-assoziierter Symptome nach Liposuktion zeigt, dass Alter, Body-Mass-Index (BMI) und präoperatives Stadium der Erkrankung einen signifikanten Einfluss auf das postoperative Ergebnis haben und in der Planung des mehrzeitigen operativen Vorgehens berücksichtigt werden müssen. BMI- oder körpergewichtsabhängige Zielgrößen der Absaugvolumina waren als Prognosefaktor für das postoperative Outcome dagegen nicht relevant. Inwieweit dies möglicherweise an der Überschreitung des „notwendigen“ Volumengrenzwerts für adäquate Symptomlinderung durch reguläre Durchführung von Megaliposuktionen liegen könnte, oder ob dieser Parameter tatsächlich keinen Einfluss auf das Ergebnis nach Operation besitzt, konnte nicht abschließend geklärt werden.
Weiterhin konnte ein positiver Nutzen auf assoziierte Begleiterkrankungen bei Lipödem nachgewiesen werden. Das Spektrum der Behandlungsmethoden kann durch reguläre Integration der Liposuktion in das Therapieschema somit um eine nachhaltige Alternative sinnvoll ergänzt werden. Im Unterschied zur alleinigen konservativen Therapie kann hierdurch ein wesentlicher Schritt weg von der alleinigen symptomatischen Therapie gemacht werden. Zudem die vielfältige Symptomatik der diversen assoziierten Komorbiditäten zu berücksichtigen. Als Konsequenz und für die Notwendigkeit eines ganzheitlichen, interdisziplinären Therapieansatzes wäre der Terminus „Lipödem-Syndrom“ möglicherweise treffender und wird zur Diskussion gestellt.
Für ein gesondertes Patientenklientel wurden zudem basale Grundsätze im perioperativen Vorgehen differenziert aufgearbeitet. Lipödem-Patientinnen mit begleitendem von-Willebrand-Syndrom stellen im Hinblick auf Blutungskomplikationen eine außerordentliche Herausforderung dar. Die vorliegenden evidenzbasierten Empfehlungen zum Therapiemanagement dieser Patientinnen bei Eingriffen ähnlicher Risikoklassifizierung wurden systematisch aufgearbeitet und in Bezug zu den speziellen Anforderungen bei Megaliposuktionen gebracht. Das dabei erarbeitete Therapieschema wird die präoperative Detektion von Koagulopathien im Allgemeinen, sowie die perioperative Komplikationsrate bei von-Willebrand-Patientinnen im Speziellen zukünftig erheblich verbessern.
Zusammenfassend konnte somit ein allgemeingültiger Algorithmus für die moderne und langfristig erfolgreiche Therapie von Lipödem-Patientinnen mit besonderem Fokus auf die Megaliposuktion erarbeitet werden. Bei adäquatem perioperativem Management und Berücksichtigung der großen Volumenverschiebungen kann der Eingriff komplikationsarm und sicher durchgeführt werden. Nicht abschließend geklärt ist derzeit die Pathophysiologie der Erkrankung wobei eine immunologische Genese sowie die primäre Pathologie des Lymphgefäßsystems bzw. der Fett(vorläufer)zellen als Erklärungmodelle favorisiert werden. Die Entwicklung diagnostischer Biomarker sollte dabei verfolgt werden.