Resonanzionisation zum Nachweis und zur Erzeugung radioaktiver Ionenstrahlen

Die resonante Laserionisation hat sich als ein universales Verfahren für eine Vielzahl von Anwendungen etabliert, die eine selektive Ionisation bei hoher Effizienz erfordern. Hierzu wurden zwei Lasersysteme mit unterschiedlichen Zielsetzungen und Schwerpunkten entwickelt und in dieser Arbeit angewendet. Im ersten Teil der Arbeit wird die Entwicklung der hochauflösenden Resonanzionisations-Massenspektrometrie zum Ultraspurennachweis von 41Ca vorgestellt. Hierzu wurden drei kontinuierliche Diodenlaser mit einem Quadrupolmassenspektrometer kombiniert. Bei einer Nachweiseffizienz von 1 × 10^−5 konnte eine Nachweisgrenze von 2 × 10^-13 41Ca/totCa erreicht werden. Das in den Routinebetrieb überführte Meßverfahren ermöglichte die Teilnahme an einem interdisziplinären Netzwerk zur Osteoporose-Forschung. In Vergleichsmessungen der Resonanzionisations-Massenspektrometrie mit allen derzeit existierenden Meßverfahren zum 41Ca-Ultraspurennachweis konnte eine sehr gute Übereinstimmung erzielt werden. Der zweite Teil der Arbeit beinhaltet die Adaption eines durchstimmbaren, hochrepetierenden Titan:Saphir-Lasersystem für den Einsatz an Laserionenquellen zur selektiven Erzeugung radioaktiver Ionenstrahlen. Das entwickelte Lasersystem ermöglicht eine effiziente, resonante Anregung des Großteils der Elemente im Periodensystem. Hierzu wurde eine kombinierte Frequenzverdopplungs- und Frequenzverdreifachungseinheit zur Erzeugung höherer Harmonischer aufgebaut. Die Anwendbarkeit eines solchen reinen Festkörper-Lasersystems wurde in zahlreichen off-line Testmessungen sowohl in Mainz als auch an den ISOL Einrichtungen am TRIUMF und ORNL gezeigt und führte zum ersten on-line Einsatz am TRIUMF.

Design and implementation of a novel multi-constellation FPGA-based dual frequency GNSS receiver for space applications

The PhD activity described in the document is part of the Microsatellite and Microsystem Laboratory of the II Faculty of Engineering, University of Bologna. The main objective is the design and development of a GNSS receiver for the orbit determination of microsatellites in low earth orbit. The development starts from the electronic design and goes up to the implementation of the navigation algorithms, covering all the aspects that are involved in this type of applications. The use of GPS receivers for orbit determination is a consolidated application used in many space missions, but the development of the new GNSS system within few years, such as the European Galileo, the Chinese COMPASS and the Russian modernized GLONASS, proposes new challenges and offers new opportunities to increase the orbit determination performances. The evaluation of improvements coming from the new systems together with the implementation of a receiver that is compatible with at least one of the new systems, are the main activities of the PhD. The activities can be divided in three section: receiver requirements definition and prototype implementation, design and analysis of the GNSS signal tracking algorithms, and design and analysis of the navigation algorithms. The receiver prototype is based on a Virtex FPGA by Xilinx, and includes a PowerPC processor. The architecture follows the software defined radio paradigm, so most of signal processing is performed in software while only what is strictly necessary is done in hardware. The tracking algorithms are implemented as a combination of Phase Locked Loop and Frequency Locked Loop for the carrier, and Delay Locked Loop with variable bandwidth for the code. The navigation algorithm is based on the extended Kalman filter and includes an accurate LEO orbit model.

Sampling methods for low-frequency electromagnetic imaging

For the detection of hidden objects by low-frequency electromagnetic imaging the Linear Sampling Method works remarkably well despite the fact that the rigorous mathematical justification is still incomplete. In this work, we give an explanation for this good performance by showing that in the low-frequency limit the measurement operator fulfills the assumptions for the fully justified variant of the Linear Sampling Method, the so-called Factorization Method. We also show how the method has to be modified in the physically relevant case of electromagnetic imaging with divergence-free currents. We present numerical results to illustrate our findings, and to show that similar performance can be expected for the case of conducting objects and layered backgrounds.

Measurement of the oscillation frequency of B s mesons in the hadronic decay mode B s pi D s (phi pi) X with the D0 detector at the Fermilab Tevatron collider

The standard model (SM) of particle physics is a theory, describing three out of four fundamental forces. In this model the Cabibbo-Kobayashi-Maskawa (CKM) matrix describes the transformation between the mass and weak eigenstates of quarks. The matrix properties can be visualized as triangles in the complex plane. A precise measurement of all triangle parameters can be used to verify the validity of the SM. The least precisely measured parameter of the triangle is related to the CKM element |Vtd|, accessible through the mixing frequency (oscillation) of neutral B mesons, where mixing is the transition of a neutral meson into its anti-particle and vice versa. It is possible to calculate the CKM element |Vtd| and a related element |Vts| by measuring the mass differences Dmd (Dms ) between neutral Bd and bar{Bd} (Bs and bar{Bs}) meson mass eigenstates. This measurement is accomplished by tagging the initial and final state of decaying B mesons and determining their lifetime. Currently the Fermilab Tevatron Collider (providing pbar{p} collisions at sqrt{s}=1.96 TeV) is the only place, where Bs oscillations can be studied. The first selection of the "golden", fully hadronic decay mode Bs->Ds pi(phi pi)X at DØ is presented in this thesis. All data, taken between April 2002 and August 2007 with the DØ detector, corresponding to an integrated luminosity of int{L}dt=2.8/fb is used. The oscillation frequency Dms and the ratio |Vtd|/|Vts| are determined as Dms = (16.6 +0.5-0.4(stat) +0.4-0.3(sys)) 1/ps, |Vtd|/|Vts| = 0.213 +0.004-0.003(exp)pm 0.008(theor). These results are consistent with the standard model expectations and no evidence for new physics is observable.