Nuclear charge radius determination of 7,10 Be and the one-neutron halo nucleus 11 Be

The only nuclear model independent method for the determination of nuclear charge radii of short-lived radioactive isotopes is the measurement of the isotope shift. For light elements (Z < 10) extremely high accuracy in experiment and theory is required and was only reached for He and Li so far. The nuclear charge radii of the lightest elements are of great interest because they have isotopes which exhibit so-called halo nuclei. Those nuclei are characterized by a a very exotic nuclear structure: They have a compact core and an area of less dense nuclear matter that extends far from this core. Examples for halo nuclei are 6^He, 8^He, 11^Li and 11^Be that is investigated in this thesis. Furthermore these isotopes are of interest because up to now only for such systems with a few nucleons the nuclear structure can be calculated ab-initio. In the Institut für Kernchemie at the Johannes Gutenberg-Universität Mainz two approaches with different accuracy were developed. The goal of these approaches was the measurement of the isotope shifts between (7,10,11)^Be^+ and 9^Be^+ in the D1 line. The …first approach is laser spectroscopy on laser cooled Be^+ ions that are trapped in a linear Paul trap. The accessible accuracy should be in the order of some 100 kHz. In this thesis two types of linear Paul traps were developed for this purpose. Moreover, the peripheral experimental setup was simulated and constructed. It allows the efficient deceleration of fast ions with an initial energy of 60 keV down to some eV and an effcient transport into the ion trap. For one of the Paul traps the ion trapping could already be demonstrated, while the optical detection of captured 9^Be^+ ions could not be completed, because the development work was delayed by the second approach. The second approach uses the technique of collinear laser spectroscopy that was already applied in the last 30 years for measuring isotope shifts of plenty of heavier isotopes. For light elements (Z < 10), it was so far not possible to reach the accuracy that is required to extract information about nuclear charge radii. The combination of collinear laser spectroscopy with the most modern methods of frequency metrology …finally permitted the …first-time determination of the nuclear charge radii of (7,10)^Be and the one neutron halo nucleus 11^Be at the COLLAPS experiment at ISOLDE/ CERN. In the course of the work reported in this thesis it was possible to measure the absolute transition frequencies and the isotope shifts in the D1 line for the Be isotopes mentioned above with an accuracy of better than 2 MHz. Combination with the most recent calculations of the mass effect allowed the extraction of the nuclear charge radii of (7,10,11)^Be with an relative accuracy better than 1%. The nuclear charge radius decreases from 7^Be continuously to 10^Be and increases again for 11^Be. This result is compared with predictions of ab-initio nuclear models which reproduce the observed trend. Particularly the "Greens Function Monte Carlo" and the "Fermionic Molecular Dynamic" model show very good agreement.

Ein Experiment zur Bestimmung des g-Faktors des gebundenen Elektrons in wasserstoff- und lithiumähnlichen mittelschweren Ionen

In dieser Arbeit werden der experimentelle Aufbau und erste Messungen für die Bestimmung des g-Faktors des Elektrons gebunden in wasserstoff- und lithiumähnlichen mittelschweren Ionen beschrieben. Mit dem hochpräzisenWert des g-Faktors können theoretische Berechnungen der Quantenelektrodynamik gebundener Zustände überprüft werden. Die Messungen werden in einem Dreifach-Penningfallen-System durchgeführt. Dort wurden im Rahmen dieser Arbeit auch erstmals hochgeladene Ionen bis 28Si13+ in einer hierfür entwickelten Elektronenstrahl-Ionenquelle/-falle erzeugt. Für die Bestimmung des g-Faktors werden die freie Zyklotronfrequenz und die Larmorfrequenz benötigt. Erstere wird aus den drei Eigenfrequenzen des in der Präzisionsfalle gespeicherten Ions berechnet. Um das Ion bei den Messungen nicht zu verlieren, werden die Eigenfrequenzen des Ions durch Kopplung an einen radiofrequenten Nachweisschwingkreis nicht-destruktiv nachgewiesen. Die freie Zyklotronfrequenz konnte dabei mit einer relativen Genauigkeit von wenigen 10E−9 bestimmt werden. Zur Bestimmung der Larmorfrequenz ist die genaue Kenntnis der Spinrichtung des Elektrons im Magnetfeld notwendig. Diese wird durch den kontinuierlichen Stern-Gerlach-Effekt in der sogenannten Analysefalle bestimmt. Hierzu muss eine hohe Stabilität der axialen Frequenz des Ions erreicht werden. Um dies sowie die Hochpräzisionsmessungen in der Präzisionsfalle zu erreichen, wurden in dieser Arbeit beide Fallen hinsichtlich ihrer elektrischen und magnetischen Eigenschaften charakterisiert.

Diodenlaserbasierte Resonanzionisations-Massenspektrometrie zur Spektroskopie und Ultraspurenanalyse an Uranisotopen

In dieser Arbeit wird die Erweiterung und Optimierung eines Diodenlasersystems zur hochauflösenden Resonanzionisationsmassenspektrometrie beschrieben. Ein doppelinterferometrisches Frequenzkontrollsystem, welches Absolutstabilisierung auf ca. 1 MHz sowie sekundenschnelle Frequenzverstimmungen um mehrere GHz für bis zu drei Laser parallel ermöglicht, wurde optimiert. Dieses Lasersystem dient zwei wesentlichen Anwendungen. Ein Aspekt waren umfangreiche spektroskopische Untersuchungen an Uranisotopen mit dem Ziel der präzisen und eindeutigen Bestimmung von Energielagen, Gesamtdrehimpulsen, Hyperfeinkonstanten und Isotopieverschiebungen sowie die Entwicklung eines effizienten, mit kommerziellen Diodenlasern betreibbaren Anregungsschemas. Mit diesen Erkenntnissen wurde die Leistungsfähigkeit des Lasermassenspektrometers für die Ultraspurenanalyse des Isotops 236U, welches als Neutronendosimeter und Tracer für radioaktive anthropogene Kontaminationen in der Umwelt verwendet wird, optimiert und charakterisiert. Anhand von synthetischen Proben wurde eine Isotopenselektivität von 236U/238U=4,5(1,5)∙10-9 demonstriert.

Measurement of the 1s-2s energy interval in muonium

The 1s-2s interval has been measured in the muonium (;mgr;(+)e(-)) atom by Doppler-free two-photon pulsed laser spectroscopy. The frequency separation of the states was determined to be 2 455 528 941.0(9.8) MHz, in good agreement with quantum electrodynamics. The result may be interpreted as a measurement of the muon-electron charge ratio as -1-1.1(2.1)x10(-9). We expect significantly higher accuracy at future high flux muon sources and from cw laser technology.

Oxygen and hydrogen isotopes measured in the Northeast Atlantic

Only a few studies have examined the variation of oxygen and hydrogen isotopes of seawater in NE Atlantic water masses, and data are especially sparse for intermediate and deep-water masses. The current study greatly expands this record with 527 d18O values from 47 stations located throughout the mid- to low-latitude NE Atlantic. In addition, dD was analyzed in the 192 samples collected along the GEOTRACES North Atlantic Transect GA03 (GA03_e=KN199-4) and the 115 Iberia-Forams cruise samples from the western and southern Iberian margin. An intercomparison study between the two stable isotope measurement techniques (cavity ring-down laser spectroscopy and magnetic-sector isotope ratio mass spectrometry) used to analyze GA03_e samples reveals relatively good agreement for both hydrogen and oxygen isotope ratios. The surface (0-100 m) and central (100-500 m) water isotope data show the typical, evaporation related trend of increasing values equatorward with the exception for the zonal transect off Cape Blanc, NW Africa. Off Cape Blanc, surface water isotope signatures are modified by the upwelling of fresher Antarctic Intermediate Water (AAIW) that generally has isotopic values of 0.0 to 0.5 per mil for d18O and 0 to 2 per mil for dD. Along the Iberian margin the Mediterranean Outflow Water (MOW) is clearly distinguished by its high d18O (0.5-1.1 per mil) and dD (3-6 per mil) values that can be traced into the open Atlantic. Isotopic values in the NE Atlantic Deep Water (NEADW) are relatively low (d18O: -0.1 to 0.5 per mil; dD: -1 to 4 per mil) and show a broader range than observed previously in the northern and southern convection areas. The NEADW is best observed at GA03_e Stations 5 and 7 in the central NE Atlantic basin. Antarctic Bottom Water isotope values are relatively high indicating modification of the original Antarctic source water along the flow path. The reconstructed d18O-salinity relationship for the complete data set has a slope of 0.51, i.e., slightly steeper than the 0.46 described previously by Pierre et al. (1994, J. Mar. Syst. 5 (2), 159-170.) for the tropical to subtropical Northeast Atlantic. This slope decreases to 0.46 for the subtropical North Atlantic Central Water (NACW) and the MOW and to 0.32 for the surface waters of the upper 50 m. The dD-salinity mixing lines have estimated slopes of 3.01 for the complete data, 1.26 for the MOW, 3.47 for the NACW, and 2.63 for the surface waters. The slopes of the d18O-dD relationship are significantly lower than the one for the Global Meteoric Water Line with 5.6 for the complete data set, 2.30 for the MOW, 4.79 for the NACW, and 3.99 for the surface waters. The lower slopes in all the relationships clearly reflect the impact of the evaporation surplus in the subtropics.

Intrakavitäts-Absorptionsspektroskopie von Spurengasen mit hoher Sensitivität und Selektivität auf Basis konkurrierender Moden eines Halbleiterlasers

Die Validität des Sensorkonzeptes aus dem Patent von Prof. H. Hillmer wird unter Verwendung einer gasförmigen Testsubstanz gezeigt. Zu diesem Zweck wird ein bestehender Messaufbau durch zahlreiche Verbesserungen optimiert. Die optischen Eigenschaften der verwendeten Komponenten und der resultierenden modifizierten Aufbauten werden dargelegt. Die bisherigen faserbasierter Messaufbauten werden zu einem symmetrischen Messaufbau mit verbesserter spektraler Auflösung und vereinfachter Handhabung erweitert. Die Vorlaufzeiten, die zuvor ein maßgebliches Problem darstellte, wurde deutlich reduziert. Die spektralen Eigenschaften des überarbeiteten Lasersystems werden detailliert erfasst und dargestellt. Der asymmetrische Messaufbau erreicht minimale Halbwertsbreiten von 0,04 ± 0,02 nm, bei einem Seitenmodenunterdrückungsverhältnis von 26,9 ± 0,9 dB und weist einen Schwellstrom von 361,55 mA auf. Der symmetrische Aufbau erreicht Halbwertsbreiten von 0,04 ± 0,02 nm, ein Seitenmodenunterdrückungsverhältnis von 49,45 ± 0,05 nm und weist einen Schwellstrom von 261,25 mA auf. Durch die Erweiterung des Systems zum symmetrischen Messaufbau wird es möglich, die Positionen der Wellenlängen frei zu wählen, wohingegen im asymmetrischen Messaufbau die Wellenlänge der äußeren Kavität immer näher am Maximum der Verstärkungskurve des SOA gewählt werden muss. Mit beiden System werden Messungen mit unterschiedlichen Stoffmengen von Acetylen mit unterschiedlichen Abständen zwischen den Laserlinien durchgeführt. Obwohl eine vergleichsweise schwache Absorptionslinie von Acetylen für die Messungen gewählt wurde, zeigen beide Systeme eine instantane Änderung der Intensitäten der Laserlinien bei einer Änderung der Stoffmenge im Resonator. Die Laserlinie, die von der Absorption von Acetylen betroffen ist, nimmt ab, wohingegen die Intensität der zweiten Laserlinie zunimmt. Es wird erstmals gezeigt, dass eine Leistungsübertragung zwischen den Laserlinien stattfindet. Die Reaktion beider Systeme ist stark vom Abstand der Laserlinien zueinander abhängig, wodurch eine genaue Bestimmung der Sensitivität nicht durchgeführt wird.

Development of the gas chromatograph – mass spectrometer to investigate volatile species in the lunar soil for the Luna-Resurs mission

Since the analysis of the lunar rocks and soil samples, brought to Earth by the Apollo missions, it is believed that the Moon has a waterless nature and also other volatile species are strongly depleted. Advancement in analysis techniques helped to identify water and other volatile species in lunar volcanic glasses. Additionally, recent lunar space missions detected water and volatile organic compounds in the region of the lunar poles where permanently shadowed craters are existing. All known lunar soil samples available on Earth come from the lunar near side, close to the equator. To verify the most recent measurement results and to enhance the knowledge of the geological history of the Moon it is of high interest to perform in situ measurements on the lunar poles. For this reason the Russian space agency, Roskosmos, developed aprogram for the scientific exploration of the lunar poles. The Gas Analysis Package (GAP) is part of the selected scientific payload aboard the Luna-Resurs Lander. This instrument uses pyrolytic cells and will apply laser spectroscopy, gas chromatography and mass spectrometry to detect and analyze volatile components trapped in the lunar soil. An existing ion optical design of a compact reflectron type time-of-flight mass spectrometer, originally built for the MEAP/P-BACE balloon mission, was chosen as a part of the GAP instrument. The scope of this thesis is the development of the interface between gas chromatography (GC) and this Neutral Gas Mass Spectrometer (NGMS) to perform coupled GC-MS measurements. In the first part of this thesis the interfacing concept was developed and verified by coupling the NGMS prototype to gas chromatography. The second part of this thesis is devoted to the development of the NGMS flight version.

Grazing incidence pumped Zr x-ray laser for spectroscopy on Li-like ions

X-ray laser fluorescence spectroscopy of the 2s-2p transition in Li-like ions is promising to become a widely applicable tool to provide information on the nuclear charge radii of stable and radioactive isotopes. For performing such experiments at the Experimental Storage Ring ESR, and the future NESR within the FAIR Project, a grazing incidence pumped (GRIP) x-ray laser (XRL) was set up at GSI Darmstadt using PHELIX (Petawatt High Energy Laser for heavy Ions eXperiments). The experiments demonstrated that lasing using the GRIP geometry could be achieved with relatively low pump energy, a prerequisite for higher repetition rate. In the first chapter the need of a plasma XRL is motivated and a short history of the plasma XRL is presented. The distinctive characteristic of the GRIP method is the controlled deposition of the pump laser energy into the desired plasma density region. While up to now the analysis performed were mostly concerned with the plasma density at the turning point of the main pump pulse, in this thesis it is demonstrated that also the energy deposition is significantly modified for the GRIP method, being sensitive in different ways to a large number of parameters. In the second chapter, the theoretical description of the plasma evolution, active medium and XRL emission properties are reviewed. In addition an innovative analysis of the laser absorption in plasma which includes an inverse Bremsstrahlung (IB) correction factor is presented. The third chapter gives an overview of the experimental set-up and diagnostics, providing an analytical formula for the average and instantaneous traveling wave speed generated with a tilted, on-axis spherical mirror, the only focusing system used up to now in GRIP XRL. The fourth chapter describes the experimental optimization and results. The emphasis is on the effect of the incidence angle of the main pump pulse on the absorption in plasma and on output and gain in different lasing lines. This is compared to the theoretical results for two different incidence angles. Significant corrections for the temperature evolution during the main pump pulse due to the incidence angle are demonstrated in comparison to a simple analytical model which does not take into account the pumping geometry. A much better agreement is reached by the model developed in this thesis. An interesting result is also the appearance of a central dip in the spatially resolved keV emission which was observed in the XRL experiments for the first time and correlates well with previous near field imaging and plasma density profile measurements. In the conclusion also an outlook to the generation of shorter wavelength XRL’s is given.