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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.