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This paper presents an imaging radar system for structural health monitoring (SHM) of wind turbine blades. The imaging radar system developed here is based on two frequency modulated continuous wave (FMCW) radar sensors with a high output power of 30 dBm. They have been developed for the frequency bands of 24,05 GHz-24,25 GHz and 33.4 GHz-36.0 GHz, respectively. Following the successful proof of damage detection and localization in laboratory conditions, we present here the installation of the sensor system at the tower of a 2 MW wind energy plant at 95 m above ground. The realization of the SHM-system will be introduced including the sensor system, the data acquisition framework and the signal processing procedures. We have achieved an imaging of the rotor blades using inverse synthetic aperture radar techniques under changing environmental and operational condition. On top of that, it was demonstrated that the front wall and back wall radar echo can be extracted from the measured signals demonstrating the full penetration of wind turbine blades during operation.
Far outside the surface of slabs, the exact exchange (EXX) potential vx falls off as −1/z , if z denotes the direction perpendicular to the surface and the slab is localized around z=0 . Similarly, the EXX energy density ex behaves as −n/(2z) , where n is the electron density. Here, an alternative proof of these relations is given, in which the Coulomb singularity in the EXX energy is treated in a particularly careful fashion. This new approach allows the derivation of the next-to-leading order contributions to the asymptotic vx and ex . It turns out that in both cases, the corrections are proportional to 1/z2 in general.
An empirical study of the per capita yield of science Nobel prizes : is the US era coming to an end?
(2018)
We point out that the Nobel prize production of the USA, the UK, Germany and France has been in numbers that are large enough to allow for a reliable analysis of the long-term historical developments. Nobel prizes are often split, such that up to three awardees receive a corresponding fractional prize. The historical trends for the fractional number of Nobelists per population are surprisingly robust, indicating in particular that the maximum Nobel productivity peaked in the 1970s for the USA and around 1900 for both France and Germany. The yearly success rates of these three countries are to date of the order of 0.2–0.3 physics, chemistry and medicine laureates per 100 million inhabitants, with the US value being a factor of 2.4 down from the maximum attained in the 1970s. The UK in contrast managed to retain during most of the last century a rate of 0.9–1.0 science Nobel prizes per year and per 100 million inhabitants. For the USA, one finds that the entire history of science Noble prizes is described on a per capita basis to an astonishing accuracy by a single large productivity boost decaying at a continuously accelerating rate since its peak in 1972.
By the fabrication of periodically arranged nanomagnetic systems it is possible to engineer novel physical properties by realizing artificial lattice geometries that are not accessible via natural crystallization or chemical synthesis. This has been accomplished with great success in two dimensions in the fields of artificial spin ice and magnetic logic devices, to name just two. Although first proposals have been made to advance into three dimensions (3D), established nanofabrication pathways based on electron beam lithography have not been adapted to obtain free-form 3D nanostructures. Here we demonstrate the direct-write fabrication of freestanding ferromagnetic 3D nano-architectures. By employing micro-Hall sensing, we have determined the magnetic stray field generated by our free-form structures in an externally applied magnetic field and we have performed micromagnetic and macro-spin simulations to deduce the spatial magnetization profiles in the structures and analyze their switching behavior. Furthermore we show that the magnetic 3D elements can be combined with other 3D elements of different chemical composition and intrinsic material properties.
Fluctuation spectroscopy measurements of quasi-two-dimensional organic charge-transfer salts (BEDT-TTF) 2 X are reviewed. In the past decade, the method has served as a new approach for studying the low-frequency dynamics of strongly correlated charge carriers in these materials. We review some basic aspects of electronic fluctuations in solids, and give an overview of selected problems where the analysis of 1/f -type fluctuations and the corresponding slow dynamics provide a better understanding of the underlying physics. These examples are related to (1) an inhomogeneous current distribution due to phase separation and/or a percolative transition; (2) slow dynamics due to a glassy freezing either of structural degrees of freedom coupling to the electronic properties or (3) of the electrons themselves, e.g., when residing on a highly-frustrated crystal lattice, where slow and heterogeneous dynamics are key experimental properties for the vitrification process of a supercooled charge-liquid. Another example is (4), the near divergence and critical slowing down of charge carrier fluctuations at the finite-temperature critical endpoint of the Mott metal-insulator transition. Here also indications for a glassy freezing and temporal and spatial correlated dynamics are found. Mapping out the region of ergodicity breaking and understanding the influence of disorder on the temporal and spatial correlated fluctuations will be an important realm of future studies, as well as the fluctuation properties deep in the Mott or charge-ordered insulating states providing a connection to relaxor or ordered ferroelectric states studied by dielectric spectroscopy.
Temperature- and field-dependent 1H-, 19F-, and 79,81Br-NMR measurements together with zero - field 79,81Br-NQR measurements on polycrystalline samples of barlowite, Cu4(OH)6FBr are conducted to study the magnetism and possible structural distortions on a microscopic level. The temperature dependence of the 79,81Br-NMR spin-lattice relaxation rates 1/T1 indicate a phase transition at TN ≃ 15 K which is of magnetic origin, but with an unusually weak slowing down of fluctuations below TN. Moreover, 1/T1T scales linear with the bulk susceptibility which indicates persisting spin fluctuations down to 2 K. Quadupolare resonance (NQR) studies reveal a pair of zero-field NQR- lines associated with the two isotopes of Br with the nuclear spins of I = 3/2. Quadrupole coupling constants of vQ ≃ 28.5 MHz and 24.7 MHz for 79Br- and 81Br-nuclei are determined from Br-NMR and the asymmetry parameter of the electric field gradient was estimated to η ≃ 0.2. The Br-NQR lines are consistent with our findings from Br-NMR and they are relatively broad, even above TN. This broadening and the relative large η value suggests a symmetry reduction at the Br- site reflecting the presence of a local distortion in the lattice. Our density-functional calculations show that the displacements of Cu2 atoms located between the kagome planes do not account for this relatively large η. On the other hand, full structural relaxation, including the deformation of kagome planes, leads to a better agreement with the experiment.
This thesis is concerned with systematic investigations of electronic noise in novel condensed matter systems. Although fluctuations are frequently considered a nuisance, that is, a disturbance limiting the accuracy of scientific measurements, in many cases they can reveal fundamental information about the inherent system dynamics. During the past decades, the study of electronic fluctuations has evolved into an indispensable tool in condensed matter physics.
The focus of the present work lies both in a further development of the fluctuation spectroscopy technique and in the study of materials of current interest. In particular, a comprehensive study of the charge carrier dynamics in the archetypal diluted magnetic semiconductors (Ga,Mn)As and (Ga,Mn)P was performed. In spite of extensive research work carried out during the last years, there still exists no theoretical consensus on the precise mechanism of ferromagnetic order and the electronic structure in these materials. Moreover, disorder and correlation effects complicate the understanding of these compounds.
Fluctuation spectroscopy experiments presented in this work provide strong evidence that a percolation transition is observed in samples with localized charge carriers, since the normalized resistance noise magnitude displays a significant enhancement around the Curie temperature. In addition, this quantity exhibits a power law scaling behavior as a function of the resistance, which is in good agreement with theoretical models of percolating systems.
By contrast, it was found that the resistance noise in metallic samples is mainly dominated by the physics of defects such as manganese interstitials and arsenic antisites. Furthermore, first noise studies were carried out on hafnia- and yttria-based resistive random access memories. In these memristor devices, the rupture and re-formation of oxygen deficient conducting filaments caused by the electric field and Joule heating driven motion of mobile anions lead to an unusual resistance switching behavior. For the first time, comparative noise measurements on oxygen deficient and stoichiometric hafnium oxide devices, as well as on novel yttrium oxide based devices were performed in this work. Finally, new strategies for noise measurements of highly insulating and extremely low-resistive samples were developed and realized. In detail, an experimental setup for the measurements of dielectric polarization fluctuations in insulating systems was designed and successfully tested. Here, the polarization noise of a sample is measured as current or voltage fluctuations produced within a capacitance cell. The study of dielectric polarization noise allows for conclusions to be drawn regarding equilibrium structural dynamics in insulators such as relaxor ferroelectrics. On the other hand, as successfully demonstrated for a heavy-fermion compound, focused ion beam etching enables to introduce a meander-shaped geometry in single crystal platelets, in order to strongly enhance the sample resistance and thus make resistance noise measurements possible. First results indicate a connection of the noise properties with the Kondo effect in the investigated material.
Crystal growth and characterization of cerium- and ytterbium-based quantum critical materials
(2018)
In der Festkörperphysik werden heutzutage Themen wie Supraleitung, Magnetismus und Quantenkritikalität sowohl von experimenteller als auch von theoretischer Seite stark untersucht. Quantenkritikalität und Quantenphasenübergänge können in Systemen erforscht werden, für welche ein Kontroll Parameter existiert, durch den z.B. eine magnetische Ordnung soweit unterdrückt wird, bis der Phasenübergang bei Null Kelvin, bei einem quantenkritischen Punkt (QCP), stattfindet. Vorzugsweise wird quantenkritisches Verhalten an Einkristallen untersucht, da diese in sehr reiner Qualität gezüchtet werden können und da deren gemessenen physikalischen Eigenschaften ausschließlich intrinsisch sind und nicht durch Verunreinigungseffekte überlagert werden. Der Schwerpunkt dieser Arbeit lag auf der Züchtung von Einkristallen und der Charakterisierung von Materialien, die quantenkritische Phänomene aufweisen. Als Ausgangsstoffe dienten dabei Elemente höchstmöglicher Reinheit. Es wurden die Serie YbNi4(P1-xAsx)2 mit einem ferromagnetischen QCP bei x=0,1, die Verbindung YbRh2Si2 mit einem feldinduzierten QCP bei Bcrit = 60mT und die Serie Ce(Ru1-xFex)PO mit einem QCP bei x = 0,86 untersucht. Für alle Verbindungen wurde das Züchtungsverfahren entwickelt, dann wurden Einkristalle gezüchtet und charakterisiert. Die Züchtung wurde zum einen mittels der Bridgman-Methode, zum anderen mit der Czochralski Methode durchgeführt. Neben struktureller und chemischer Charakterisierung der Einkristalle mittels Röntgen-Pulverdiffraktometrie, Laue-Methode und Energie-dispersiver Röntgen-Spektroskopie, wurden auch deren spezifische Wärme, elektrischer Widerstand und Magnetisierung im Temperaturbereich 1,8 – 300 K untersucht. Im weiteren Verlauf wurden die Kristalle in verschiedenen Kooperationen untersucht und bis in den Tieftemperatur- Bereich (20 mK), bei YbRh2Si2 bis in den Submillikelvin-Bereich, charakterisiert. Ausserdem wurden im Rahmen dieser Dissertation Einkristalle weiterer antiferromagnetischer Verbindungen SmRh2Si2, GdRh2Si2, GdIr2Si2, HoRh2Si2 und HoIr2Si2 gezüchtet. Bei diesen Verbindungen stand die Untersuchung elektronischer Oberflächenzustände mittels winkelaufgelöster Photoemissionsspektroskopie im Vordergrund.
Spontaneous brain activity is characterized in part by a balanced asynchronous chaotic state. Cortical recordings show that excitatory (E) and inhibitory (I) drivings in the E-I balanced state are substantially larger than the overall input. We show that such a state arises naturally in fully adapting networks which are deterministic, autonomously active and not subject to stochastic external or internal drivings. Temporary imbalances between excitatory and inhibitory inputs lead to large but short-lived activity bursts that stabilize irregular dynamics. We simulate autonomous networks of rate-encoding neurons for which all synaptic weights are plastic and subject to a Hebbian plasticity rule, the flux rule, that can be derived from the stationarity principle of statistical learning. Moreover, the average firing rate is regulated individually via a standard homeostatic adaption of the bias of each neuron’s input-output non-linear function. Additionally, networks with and without short-term plasticity are considered. E-I balance may arise only when the mean excitatory and inhibitory weights are themselves balanced, modulo the overall activity level. We show that synaptic weight balance, which has been considered hitherto as given, naturally arises in autonomous neural networks when the here considered self-limiting Hebbian synaptic plasticity rule is continuously active.
Recent experiments have demonstrated that visual cortex engages in spatio-temporal sequence learning and prediction. The cellular basis of this learning remains unclear, however. Here we present a spiking neural network model that explains a recent study on sequence learning in the primary visual cortex of rats. The model posits that the sequence learning and prediction abilities of cortical circuits result from the interaction of spike-timing dependent plasticity (STDP) and homeostatic plasticity mechanisms. It also reproduces changes in stimulus-evoked multi-unit activity during learning. Furthermore, it makes precise predictions regarding how training shapes network connectivity to establish its prediction ability. Finally, it predicts that the adapted connectivity gives rise to systematic changes in spontaneous network activity. Taken together, our model establishes a new conceptual bridge between the structure and function of cortical circuits in the context of sequence learning and prediction.
Quantum chromodynamics (QCD) is the theory of the strong interaction between quarks and gluons. Due to Confinement, at lower energies quarks and gluons are bound into colorless states called hadrons. QCD is also asymptotically free, i.e. at large energies or densities it enters a deconfined state, termed quark-gluon plasma (QGP), where quarks and gluons are quasi-free. This transition occurs at an energy scale around 200 MeV where QCD cannot be treated perturbatively. Instead it can be formulated on a space-time grid. The resulting theory, lattice quantum chromodynamics (LQCD), can be simulated efficiently on high performance parallel-computing clusters. In recent years graphic processing units (GPUs), which outperform CPUs in terms of parallel-computing and memory bandwidth capabilities, became very popular for LQCD computations. In this work the QCD deconfinement transition is studied using CL2QCD, a LQCD application that runs efficiently on GPUs. Furthermore, CL2QCD is extended by a Rational Hybrid Monte Carlo algorithm for Wilson fermions to allow for simulations of an odd number of quark flavors.
Due to the sign-problem LQCD simulations are restricted to zero or very small baryon densities, where, in the limit of infinite quark mass QCD has a first order deconfinement phase transition associated to the breaking of the global centre symmetry. Including dynamical quarks breaks this symmetry explicitly. Lowering their mass weakens the first order transition until it terminates in a second order Z2 point. Beyond this point the transition is merely an analytic crossover. As the lattice spacing is decreased, the reduction of discretization errors causes the region of first order transitions to expand towards lower masses. In this work the deconfinement critical point with 2 and 3 flavors of standard Wilson fermions is studied. To this end several kappa values are simulated on temporal lattice extents 6,8,10 (4) for two flavors (three flavors) and various aspect ratios (spatial lattice extent / temporal lattice extent) so as to extrapolate to the thermodynamic limit, applying finite size scaling. For two flavors an estimate is done if and when a continuum extrapolation is possible.
The chiral and deconfinement phase transitions at zero density for light and heavy quarks, respectively, have analytic continuations to purely imaginary chemical potential, where no sign-problem exists and LQCD simulations can be applied. At some critical value of the imaginary chemical potential, the transitions meet the endpoint of the Roberge-Weiss transition between adjacent Z3 sectors. For light and heavy quarks the transition lines meet in a triple point, while for intermediate masses they meet in a second order point. At the boundary between these regimes the junction is a tricritical point, as shown in studies with two and three flavors of staggered and Wilson quarks on lattices with a temporal lattice extent of 4. Employing finite size scaling the nature of this point as a function of the quark mass is studied in this work for two flavors of Wilson fermions with a temporal lattice extent of 6. Of particular interest is the change of the location of tricritical points compared to an earlier study on lattices with temporal extent of 4.
The quasi-two-dimensional organic charge-transfer salt κ -(BEDT-TTF) 2 Cu 2 (CN) 3 is one of the prime candidates for a quantum spin-liquid due the strong spin frustration of its anisotropic triangular lattice in combination with its proximity to the Mott transition. Despite intensive investigations of the material’s low-temperature properties, several important questions remain to be answered. Particularly puzzling are the 6 K anomaly and the enigmatic effects observed in magnetic fields. Here we report on low-temperature measurements of lattice effects which were shown to be particularly strongly pronounced in this material (R. S. Manna et al., Phys. Rev. Lett. 2010, 104, 016403)). A special focus of our study lies on sample-to-sample variations of these effects and their implications on the interpretation of experimental data. By investigating overall nine single crystals from two different batches, we can state that there are considerable differences in the size of the second-order phase transition anomaly around 6 K, varying within a factor of 3. In addition, we find field-induced anomalies giving rise to pronounced features in the sample length for two out of these nine crystals for temperatures T< 9 K. We tentatively assign the latter effects to B-induced magnetic clusters suspected to nucleate around crystal imperfections. These B-induced effects are absent for the crystals where the 6 K anomaly is most strongly pronounced. The large lattice effects observed at 6 K are consistent with proposed pairing instabilities of fermionic excitations breaking the lattice symmetry. The strong sample-to-sample variation in the size of the phase transition anomaly suggests that the conversion of the fermions to bosons at the instability is only partial and to some extent influenced by not yet identified sample-specific parameters.
Für das bessere Verständnis der Nukleosynthese der schweren Elemente im s-Prozess wurde im Rahmen dieser Arbeit die Messung zur Bestimmung der Neutroneneinfangsreaktion von 83Kr durchgeführt. Als Messinstrument wurde DANCE am LANL verwendet, ein 4pi-Kalorimeter zur Detektion der entstehenden g-Kaskaden bei (n,g)-Reaktionen. Darüber hinaus wurden außerdem noch Proben mit 85Kr und 86Kr vermessen.
Die Herausforderung an diesem Experiment bestand vor allem in der Probenherstellung. Das Edelgas Kr erforderte eine Neukonstruktion der normalerweise bei DANCE verwendeten Probenhalterung. Das Hauptaugenmerk lag auf der Maximierung der Kr-Exposition durch den Neutronenstrahl. Im Gegenzug wurde versucht das umgebende Material nach Möglichkeit keinen Neutronen auszusetzen. Für die Isotope 83,86Kr wurden Hochdruckgaskugeln verwendet, die an der Goethe-Universität Frankfurt gefüllt und in eine der neuen Probenhalterungen eingesetzt wurden. Zur Beachtung des bei der Messung entstehenden Untergrundes wurde eine Messung mit baugleicher Probenhalterung und leerer Gaskugel durchgeführt. Da bereits kleine Mengen 85Kr eine hohe Radioaktivität aufweisen, wurde eine in einen Stahlzylinder eingeschweißte, existierende Quelle verwendet.
Bei der Analyse zu 86Kr wurde schnell eine zu starke Verunreinigung der Kr-Probe mit Xe offensichtlich, einen signifikanten Anteil des Spektrums ausmachte. Aus diesem Grund kam es vor allem zu Problemen den korrekten Untergrund von den 86Kr Messdaten zu subtrahieren. Die weitere Bestimmung inklusive Streukorrekturen, Normierung anhand des Flussmonitors und DICEBOX/GEANT3 Effizienzbestimmung lieferte zwar einen energieabhängigen Wirkungsquerschnitt, dieser zeigte allerdings große Abweichungen von den evaluierten ENDF/B-VII.1 Daten, was besonders ersichtlich in der deutlichsten 86Kr Resonanz bei 5515 eV zu erkennen war. Aus diesem Grund konnte aus den Messdaten kein MACS extrahiert werden.
Bei einer Untersuchung der Aktivität der 85Kr-Probe mit Hilfe der einzelnen BaF2-Detektoren in der DANCE Kugel zeigte sich zunächst eine um fast einen Faktor vier geringere Aktivität als vom Hersteller angegeben. Auch bei der weiteren Analyse traten massive Untergrundprobleme auf. Die Form des Stahlzylinders, in dem das Kr-Gasgemisch eingeschweißt war, konnte aufgrund seiner Form nur schwer im Strahlrohr untergebracht werden. Beim Experiment selbst zeigte sich dann, dass Teile der Halterung vom Neutronenstrahl getroffen wurden, was einen Untergrund mit sehr hohem Q-Wert erzeugte, der nicht durch ein Esum Fenster entfernt werden konnte. Durch eine Beschädigung der Halterung mit der Probe kam es darüber hinaus zu Abweichungen mit der verwendeten Leerhalterung. All das führte trotz einer langen Messzeit von fast 18 d dazu, dass nur ein sehr schwaches Signal von der eigentlichen Kr-Probe zu erkennen war. Es wurde eine mögliche 85Kr Resonanz bei 675 eV gefunden, allerdings ist die endgültige Zuordnung aufgrund der nicht eindeutigen Untergrundsituation äußerst schwierig. Im Vorfeld des Kr-Experimentes wurde eine Messung von RbCl an DANCE durchgeführt, da ursprünglich zu erwarten war, dass bereits ein Teil des 85Kr zu 85Rb zerfallen war. Durch diese Messung sollte dieser Anteil leicht von der späteren Messung zu subtrahieren sein. Allerdings trat ein unerwartetes Problem während der Datenaufnahme auf. Die Verbindung der DAQ Boards wurde getrennt, wodurch ca. 3/4 der Detektoren nicht mehr zeitsynchron liefen. Im Zuge dieser Arbeit wurde eine Rekonstruktion dieser Daten angestrebt. Durch Modifikationen am FARE Code, der zur Auswertung verwendet wurde, konnte Flugzeitspektren für jeden Beschleunigerpuls erzeugt werden. Es zeigte sich zunächst ein offensichtlicher Trend einer Verschiebung der getrennten Boards zu späteren Zeiten. Durch mehrere Fits an die Abweichungsverteilung und anschließende Korrektur konnte zunächst ein Spektrum wiederhergestellt werden, das vergleichbar mit den unbeschädigten Daten war. Bei einer detaillierten Analyse dieser neu gewonnen Daten zeigte sich jedoch eine Nichtlinearität in der Zeitverschiebung. Dies resultierte letztlich in einer Korrektur des Spektrums, allerdings nicht in einem Koinzidenzfenster von 10 ns, das für eine Wirkungsquerschnittsanalyse notwendig ist. Es wurde geschlussfolgert, dass durch die geringe Statistik in den einzelnen Flugzeitspektren solch eine Genauigkeit nicht zu erreichen ist.
Die Messung des Neutroneneinfangsquerschnitts von 83Kr konnte im Zuge dieser Arbeit erfolgreich durchgeführt werden. Es wurden zwei Messungen mit verschiedenen Strömen kombiniert. Eine Messung mit 40 µA wurde durchgeführt, um Pile-Up in der größten Resonanz bei 28 eV zu reduzieren. Die zweite Messung diente dann dem Sammeln von ausreichend Statistik in den nicht resonanten Bereichen. Die eingesetzte Leerkugel erlaubte eine saubere Subtraktion des Untergrundes von Probenhalterung, Gaskugel und Umgebung. Für die Skalierung der Messergebnisse wurde eine weitere Messung mit einer 5000 Å dicken Goldfolie durchgeführt. Zur Bestimmung der Detektoreffizienz konnten zunächst die durch den Neutroneneinfang entstandenen Abregungskaskaden der 84Kr Kerne mit DICEBOX modelliert werden. Diese Kaskaden wurden dann anschließend in GEANT3 Simulationen verwendet, um die Effizienz bestimmen zu können. Mit diesen Methoden erhielt man die Maxwell-gemittelten Wirkungsquerschnitte von kT = 5 keV - 100 keV. Bei der für den s-Prozess wichtigen Temperatur von kT = 30 keV wurde der Querschnitt bestimmt zu: MACS (30 keV) = (256,6 +- 14,2 (stat) +- 18,1(sys)) mb.
Dieser Wert ist in guter Übereinstimmung mit dem in der KADoNIS v0.3 Datenbank angegebenen Wert von MACS;KADoNIS (30 keV) = (243 +- 15) mb. Mit den so gewonnenen Wirkungsquerschnitten wurden außerdem die Reaktionsraten berechnet. Bei den anschließenden Netzwerkrechnungen mit dem Programm NETZ wurden die Auswirkungen der in dieser Arbeit gewonnenen Wirkungsquerschnitte im Vergleich zu den KADoNIS v0.3 Werten betrachtet. Dabei zeigte sich eine leicht erhöhte Produktion der stabilen Isotope 84Kr, 86Kr, 85Rb und 87Rb, sowie eine leichte Unterproduktion der stabilen Isotope 86-88Sr in der Hauptkomponente des s-Prozess. Ein ähnliches Bild zeigte sich in der He-Brennphase der schwachen Komponente. Der in dieser Arbeit gemessene Wirkungsquerschnitt bei hohen Temperaturen ist geringer als der in KADoNIS v0.3 angegebene, weswegen es bei der Simulation mit NETZ zu einer stark erhöhten Produktion von 83Kr in der C-Brennphase kommt.
Compact objects - black holes and neutron stars - are fascinating objects, not only for the astrophysicists, but for a wide range of researchers, including astronomers, theoretical physicists, particle and nuclear physicists, condensed matter physicists and arguably for the layman as well.
First theorized in the first part of the twentieth century, for a long time these objects have been considered just exotic ideas or mathematical curiosities. Pulsar were however detected in the late 1960s and readily identified as rotating, radiating neutron stars, while the first candidate black hole, Cygnus X-1, was observed in 1972. Since then the interest in these objects has steadily grown.
The reasons behind this interest are easily understood considering that compact object dwell at the intersection of many different areas of physics, and are ideal laboratories to explore the interplay between these areas.
Black holes, which are purely gravitational objects, are perfectly suited to study the nature of gravity, its manifestations such as gravitational waves, and the differences between various theories of gravity in the regime where they are expected to be most relevant, i.e. the strong field regime. However, just like any massive astrophysical object, black holes are interested by accretion phenomena, which are thought to be the power source of some very bright astrophysical emitters of electromagnetic signals, such as active galactic nuclei or X-ray binaries.
At the same time, black holes exist in a variety of different mass scales, from stellar mass to supermassive black holes billions of times heavier. The latter play a very important and yet not fully understood role in the formation and evolution of galaxies, as well as in shaping the large scale structure of the universe, making them relevant to cosmology as well.
Neutron stars share with black holes the characteristic of being gravitationally dominated systems; but because they are composed of baryon matter, they display a much richer behaviour. It has been realized early on that the matter in neutron star cores reaches extreme densities, exceeding the one in atomic nuclei. This means that neutron stars could provide invaluable information on the behaviour of matter in such extreme conditions (which are impossible to achieve in laboratory experiments), such as details of the nucleonic interaction, the properties of hyperons or of quark-gluon plasmas.
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The mission of the Compressed Baryonic Matter (CBM) experiment is to investigate the phase diagram of strongly interacting matter in the region of high net-baryon densities and moderate temperatures. According to various transport models, matter densities of more than 5 times saturation density can be reached in collisions between gold nuclei at beam energies between 5 and 11 GeV per nucleon, which will be available at FAIR. The core detector of the CBM experiment is the Silicon Tracking System (STS), which is used to measure the tracks of up to 700 particles per collision with high efficiency (>95%) and good momentum resolution (<1.5%). The technological and experimental challenge is to realize a detector system with very low material budget, in order to reduce multiple scattering of the particles, and a free-streaming data readout chain, in order to achieve reaction rates up to 10 MHz together with an online event reconstruction and selection.
The STS comprises 8 tracking stations positioned between 30 cm and 100 cm downstream the target inside a magnetic field, covering polar emission angles up to 25 degrees. A station consists of vertical structures with increasing number (between 8 and 16, depending on station number), each structure carrying between 2 and 10 double-sided microstrip silicon sensors, which are connected through low-mass microcables to the readout electronics placed at the detector periphery outside the active detector area.
The work presented in this thesis focuses on the detector performance simulation and local hit pattern reconstruction in the STS. For efficient detector design and reconstruction performance, a reliable detector response model is of utmost importance. Within this work, a realistic detector response model was designed and implemented in the CBM software framework. The model includes non-uniform energy loss of an incident particle within a sensor, electric field of a planar p-n junction, Lorentz shift of the charge carriers, their diffusion, and the influence of parasitic capacitances. The developed model has been verified with experimental data from detector tests in a relativistic proton beam. Cluster size distributions at different beam incident angles are sensitive to charge sharing effects and were chosen as an observable for the verification. Taking into account parasitic capacitances further improves the agreement with measured data.
Using the developed detector response model, the cluster position finding algorithm was improved. For two-strip clusters, a new, unbiased algorithm has been developed, which gives smaller residuals than the Centre-Of-Gravity algorithm. For larger clusters, the head-tail algorithm is used as the default one. For an estimate of the track parameters, the Kalman Filter based track fit requires not only hit positions but their uncertainties as an input. A new analytic method to estimate the hit position errors has been designed in this work. It requires as input neither measured spatial resolution nor information about an incident particle track. The method includes all the sources of uncertainties independently, namely: the cluster position finding algorithm itself, the non-uniform energy loss of incident particles, the electronics noise, and the discretisation of charge in the readout chip.
The verification with simulations shows improvements in hit and track pull distributions as well as x²-distributions in comparison to the previous simple approach. The analytic method improves the track parameters reconstruction by 5-10%.
Several STS module prototypes have been tested in a relativistic proton beam. A signal to-noise ratio was obtained at the level of 10-15 for modules made of 30 cm long microcable and of either one or two 6.2 x 6.2 cm² CiS sensors.
First simulations have shown that this signal-to-noise ratio is sufficient to reach the required efficiency and momentum resolution. The high-radiation environment of CBM operation will deteriorate the sensor performance. Radiation hardness of sensors has been studied in the beam with sensors irradiated to 2 x 10[hoch 14] 1MeV [neq/cm²], twice the lifetime dose expected for CBM operation. Charge collection efficiency drops by 17-25%, and simultaneously noise levels increase 1.5-1.75 times. The simulations show that if all sensors in the STS setup are exposed to such a fluence uniformly, the track reconstruction efficiency drops from 95.5% to 93.2% and the momentum resolution degrades from 1.6% to 1.7%.
We present a study of the influence of disorder on the Mott metal-insulator transition for the organic charge-transfer salt κ -(BEDT-TTF) 2 Cu[N(CN) 2 ]Cl. To this end, disorder was introduced into the system in a controlled way by exposing the single crystals to X-ray irradiation. The crystals were then fine-tuned across the Mott transition by the application of continuously controllable He-gas pressure at low temperatures. Measurements of the thermal expansion and resistance show that the first-order character of the Mott transition prevails for low irradiation doses achieved by irradiation times up to 100 h. For these crystals with a moderate degree of disorder, we find a first-order transition line which ends in a second-order critical endpoint, akin to the pristine crystals. Compared to the latter, however, we observe a significant reduction of both, the critical pressure pc and the critical temperature Tc . This result is consistent with the theoretically-predicted formation of a soft Coulomb gap in the presence of strong correlations and small disorder. Furthermore, we demonstrate, similar to the observation for the pristine sample, that the Mott transition after 50 h of irradiation is accompanied by sizable lattice effects, the critical behavior of which can be well described by mean-field theory. Our results demonstrate that the character of the Mott transition remains essentially unchanged at a low disorder level. However, after an irradiation time of 150 h, no clear signatures of a discontinuous metal-insulator transition could be revealed anymore. These results suggest that, above a certain disorder level, the metal-insulator transition becomes a smeared first-order transition with some residual hysteresis.
Most of the elements in the universe are produced via charged-particle fusion reactions during the primordial nucleosynthesis and different stellar burning stages, as well as via neutron-capture reactions. Around 35 heavy, proton-rich isotopes are bypassed by those reaction paths, the p nuclei. A series of photo-disintegration reactions occurring in supernovae, called the γ process, was suggested as a mechanisms to produce the p nuclei. Numerical simulations of the γ process have been unable to reproduce the observed abundances of the light p isotopes. Recent models showed that a series of proton capture reactions could provide the observed abundances. Hence, the cross sections of the crucial capture reactions have to be measured in order to test those assumptions.
Radiative proton captures in addition to the γ-process could reproduce the observed abundance pattern. This thesis presents preparations of a proton capture measurement on the radioactive 91Nb in standard kinematics with a calorimetric 4π setup. The 91Nb(p,γ)92Mo reaction might be the key to explain the production of one of the most abundant p-nuclei, 92Mo. So far, no experimental data for this reaction is available.
We produced a sample of 91Nb, with a half-life of 680 yr, at the Physikalisch Technische Bundesanstalt in Braunschweig, Germany, by irradiating 92Mo with protons in the energy range of 12 – 20MeV. 91Nb was produced via the reaction 92Mo(p,2p)91Nb and via 92Mo(p,pn)91Mo, where 91Mo decays to 91Nb with a half-life of 15.5min. To predict the amount of produced 91Nb the cross section of 92Mo(p, 2p) was measured. It was found to be higher than the value given by theoretical calculations with TALYS. Finally, 91Nb was chemically separated from the molybdenum carried at Paul-Scherrer- Institut, Villigen, Switzerland.
In-beam total absorption cross-section measurement of the reaction 91Nb(p,γ)92Mo with 2 MeV protons at FRANZ is planed with the produced 91Nb. A 4π BaF2 detector consisting of 41 crystals will be used. During this experiment we will measure the sum energy and the multiplicity of each event. The freshly produced 91Nb constitutes only a minor component of the sample material. The sum energy and multiplicity are crucial to distinguish the desired 91Nb(p,γ) from all the other more dominant reactions. The expected multiplicity and the efficiency of the setup were carefully simulated with DICEBOX and GEANT4. It was possible to show that background reactions can be effectively suppressed. The most important background contributions could be identified and result from 92Mo(p,γ), 19F(p,γ), and 19F(p,α).