Aujourd'hui, nous sommes tous témoins d'une compétition des installations en pays différents pour étudier les régions inconnues de noyaux riches en neutrons. Beaucoup d'efforts sont consacrés à comprendre le rôle de l'excès de neutrons et son influence sur les noyaux dans les environs de coquilles de neutrons fermées. Un des moyens pour étudier la structure nucléaire est via la désintégration bêta. Une fois un noyau est prouvé d'exister, ses propriétés de désintégration bêta, comme T1/2 et Pn (probabilité de l'émission de neutrons de bêta-retardés), qui sont relativement faciles à mesurer, peuvent fournir les premiers indices sur la structure nucléaire. Sur le site de processus-r des «points d'attente» (noyaux sur des coquilles de neutrons fermés) ont des effets importants sur la dynamique processus-r ainsi que sur la distribution de l'abondance des éléments. Les conditions astrophysiques exactes en vertu de desquelles la synthèse nucléaire a lieu ne sont pas connus avec certitude. Parce que les noyaux participant en processus-r sont difficiles à synthétiser même aujourd'hui et à étudier expérimentalement, les paramètres nécessaires pour les calculs du processus-r sont principalement dérivés de modèles théoriques. Comme on l'a vu récemment, la plupart des théories n'ont pas réussi à reproduire des ensembles de données nouvellement mesurées près de fermetures de couche. Avec de nouvelles données expérimentales déjà (ou bientôt) disponibles les approches théoriques peuvent être ajustées. Comme émission de neutrons retardée bêta devient plus importante voie le canal dominant en désintégration des noyaux loin d'un stabilité, l'utilisation d'un détecteur de neutrons approprié afin d'étudier leurs propriétés est indispensable. C'est pour mener la recherche appropriée que dans le cadre de la thèse, en étroite collaboration avec le JINR (Dubna) un nouveau système de détection a été construit. Il se compose de 80 compteurs de ³He, un détecteur 4π de bêta et un HPGe afin de mesurer simultanément l'activité de gamma, bêta et neutrons. Le développement d'un tel système de détection, actuellement installé sur ALTO, a été le premier objectif de la thèse. Puis, au cours de deux campagnes expérimentales menées pour examiner les propriétés de désintégration bêta de noyaux riches en neutrons dans le proximité de N = 50, N = 82 la capacité de travail du système de détection produit a été prouvée. Dans le région de ⁷⁸Ni : le temps de vie et de la probabilité de l'émission de neutrons bêta retardés pour ⁸º,⁸²,⁸³,⁸⁴Ga ont été mesurés. Nous sommes les premiers à observer la structure de ⁸¹,⁸² Ge via spectroscopie gamma spectre conditionnée par bêta et par neutron. Grâce à la détection des neutrons les intensités absolues de la désintégration bêta ont été proposées pour la première fois. Dans le région de ¹³²Sn les temps de vie de ¹²³Ag, ¹²⁴Ag, ¹²⁵Ag et ¹²⁷In, ¹²⁸In ont été mesurées. Pour la première fois l'émission de neutrons retardés bêta a été observée pour le cas de ¹²⁶Cd, sa valeur Pn également mesurée. Sur la base des données obtenues, nous arrivons à la conclusion que, pour déterminer la contribution relative de désintégrations permises et interdites les efforts théoriques doivent être faites en traversant la couche N = 50. Alors que dans le région de N = 82 plus de données expérimentales sont nécessaires. / Nowadays we are all witnesses of a competition of facilities at different countries to study unknown regions of neutron rich nuclei. Much efforts are devoted to understand the role of neutron excess and its influence on nuclei in vicinity of closed neutron shells. One of the means to investigate nuclear structure is in beta-decay. Once a nucleus is proven to exist, its beta-decay properties, such as T1/2 and Pn (probability of beta-delayed neutron emission), which are relatively easy to measure, can provide the first hints on the nuclear structure. On the r-process site, "waiting points"(nuclei on closed neutron shells) has significant effects on the r-process dynamics and the abundance distribution. The actual side and the astrophysical conditions under which the nuclear synthesis takes place are still not certainly known - since r-process nuclei are difficult to produce and to study experimentally, input parameters for r-process calculations are mostly derived from theoretical models. As it has been seen lately, most of the theories have failed to reproduce newly measured data sets near shell closures. With new experimental data already (or shortly) available theoretical approaches can be adjusted. Since a beta-delayed neutron emission becomes strong if not dominating decaying channel for nuclei far stability, a proper neutron detector to study their properties is indispensable. To conduct the appropriate investigations, in the frame of the present thesis, in close collaboration with JINR (Dubna) a new detection system was constructed. It consists of 80 ³He-filled counters, 4π beta detector and a HPGe in order to measure simultaneously beta, gamma, neutron activity. The development of such a detection system system, currently installed at ALTO ISOL facility, was the first objective of the thesis. Then, during two experimental campaigns conducted to investigate beta decay properties of neutron rich nuclei in the neighborhood of N=50, N=82 the workability of the newly produced detection system was proven. In the vicinity of ⁷⁸Ni: half- lives and probability of beta-delayed neutron emission for ⁸º,⁸²,⁸³,⁸⁴Ga were measured. We were the first to observe the structure of ⁸¹,⁸² Ge via beta neutron gated gamma spectra. Thanks to the neutron detection channel the absolute intensities of beta decay were proposed for the first time. In the vicinity of ¹³²Sn the half lives of ¹²³Ag, ¹²⁴Ag, ¹²⁵Ag and ¹²⁷In, ¹²⁸In was measured. For the first time the beta delayed neutron emission was observed for ¹²⁶Cd, its Pn value also measured. Based on the data obtained we come to the conclusion that to figure out the relative contribution of allowed and forbidden decays more theoretical efforts should be done crossing the N=50 shell. Whereas in the vicinity of N=82 shell more experimental challenge are required.

Es wurde eine Elektron-Zyklotron-Resonanz-Ionenquelle mit einer Mikrowellenfrequenz von2,45 GHz für die Produktion intensiver Ströme einfach geladener Metallionen entwickelt. Deren Beladung mit Metalldampf erfolgt über ein integriertes zylindrisches Sputtermagnetron, welches speziell für diese Aufgabe entworfen wurde. Die entstandene MECRIS, engl. Magnetron Electron Cyclotron Resonance Ion Source, vereinigt die ECR-Ionenquellentechnologie mit der Magnetron-Sputtertechnologie auf bisher einzigartige Weise und verkörpert so ein neues Metallionen-Quellenkonzept. Unter Verwendung eines Al-Sputtertargets konnte die Funktionsfähigkeit der MECRIS an dem Beispiel der Al+-Ionenerzeugung erfolgreich demonstriert werden. Der extrahierbare Al+-Ionenstrom wurde über einen neuartigen, im Rahmen der Arbeit entwickelten, Hochstrom-Faraday-Cup gemessen. Auf Basis numerischer Berechnungen wurde das Gesamtmagnetfeld so ausgelegt, dass die Permanentmagnete des Magnetrons und die Spulen der ECR-Quelle eine Minimum-B-Struktur erzeugen, welche einen effektiven Elektroneneinschluss nach dem magnetischen Spiegelprinzip ermöglicht. Gleichzeitig wird durch eine geschlossene ECR-Fläche, mit der magnetischen Resonanzflussdichte von 87,5 mT, eine optimale Heizung der Plasmaelektronen realisiert. Die mithilfe einer Doppel-Langmuir-Sonde gemessene Elektronentemperatur steigt in Richtung Quellenmitte an und beträgt maximal 11 eV. Geheizte Elektronen erlauben die effiziente Stoßionisation der Al-Atome, welche mit einer Rate von über 1E18 Al-Atome/s eingespeist werden und eine höchstmögliche Dichte von 2E10 1/cm³ aufweisen. Die MECRIS erzeugt hauptsächlich einfach geladene Ionen des gesputterten Materials (Al+) und des Prozessgases (Ar+). Der Al+-Ionenextraktionsstrom ist über die Erhöhung der Prozessparameter Sputterleistung, Mikrowellenleistung, Spulenstrom und Extraktionsspannung um eine Größenordnung bis auf maximal 135 μA steigerbar, was einer Stromdichte von 270 μA/cm² über die Extraktionsfläche von rund 0,5 cm² entspricht. Dies steht im Einklang mit der Prozessparameterabhängigkeit der anhand der Sonde bestimmten Plasmadichte, welche einen größtmöglichen Wert von etwa 6E11 1/cm³ annimmt. Das Verhältnis von extrahiertem Al+- zu Ar+-Ionenstrom kann durch Optimierung der Prozessparameter von 0,3 auf maximal 2 angehoben werden. Sondenmessungen des entsprechenden Ionendichteverhältnisses bestätigen diesen Sachverhalt. Um möglichst große Extraktionsströme und Al+/Ar+-Verhältnisse zu generieren, muss die ECR-Fläche demnach in dem Bereich der höchsten Al-Atomdichte in der Targetebene lokalisiert sein. Gegenüber dem alleinigen Magnetronplasma (ohne Mikrowelleneinspeisung) können mit dem MECRIS-Plasma um bis zu 140 % höhere Al+-Ionenströme produziert werden. Aus Sondenuntersuchungen geht hervor, dass dies eine Folge der um etwa eine Größenordnung gesteigerten Plasmadichte und der um rund 7 eV größeren Elektronentemperatur des MECRIS-Plasmas ist. Das MECRIS-Plasma wurde außerdem mittels optischer Emissionsspektroskopie charakterisiert und durch ein globales sowie ein zweidimensionales Modell simuliert. Die gewonnenen Prozessparameterabhängigkeiten der Plasmadichte, Elektronentemperatur sowie Al+- und Ar+-Ionendichte stimmen mit den Sondenergebnissen überein. Teilweise treten jedoch Absolutwertunterschiede von bis zu zwei Größenordnungen auf. Die Erhöhung der Sputterleistung und Extraktionsspannung über die derzeitigen Grenzen von 10 kW bzw. 30 kV sowie die Optimierung der Extraktionseinheit hinsichtlich minimaler Elektrodenblindströme bietet das Potential, den Al+-Ionenstrom bis in den mA-Bereich zu steigern. / An electron cyclotron resonance ion source working at a microwave frequency of 2.45 GHz has been developed in order to generate an intense current of singly charged metal ions. It is loaded with metal vapor by an integrated cylindrical sputter magnetron, which was especially designed for this purpose. The MECRIS (Magnetron Electron Cyclotron Resonance Ion Source) merges ECR ion source technology with sputter magnetron technology in a unique manner representing a new metal ion source concept. By using an Al sputter target, the efficiency of the MECRIS was demonstrated successfully for the example of Al+ ion production. The extractable ion current was measured by a newly developed high-current Faraday cup. On the basis of numerical modeling, the total magnetic field was set in a way that the permanent magnets of the magnetron and the coils of the ECR source are forming a minimum-B-structure, providing an effective electron trap by the magnetic mirror principle. Simultaneously, optimal electron heating is achieved by a closed ECR-surface at resonant magnetic flux density of 87.5 mT. Electron temperature increases towards the center of the source to a maximum of about 11 eV and was measured by a double Langmuir probe. Due to the heated electron population, efficient electron impact ionization of the Al atoms is accomplished. Al atoms are injected with a rate of more than 1E18 Al-atoms/s resulting in a maximum Al atom density of 2E10 1/cm³. The MECRIS produces mainly singly charged ions of the sputtered material (Al+) and the process gas (Ar+). The Al+ ion extraction current is elevated by one order of magnitude to a maximum of 135 μA by increasing the process parameters sputter magnetron power, microwave power, coil current, and acceleration voltage. Related to the extraction area of about 0.5 cm², the highest possible Al+ ion current density is 270 μA/cm². A corresponding process parameter dependency was found for the plasma density showing a peak value of about 6E11 1/cm³, which was deduced from probe measurements. The ratio of the extracted Al+ ion current to the Ar+ ion current can be enhanced from 0.3 to a maximum of 2 by optimization of the process parameters. This was confirmed by probe investigations of the appropriate ion density ratio. In conclusion, the ECR-surface needs to be located in the area of the highest Al atom density in the target plane in order to improve the extraction current and Al+/Ar+ ratio. The MECRIS plasma produces an Al+ ion current, which is up to 140 % higher compared to that of the sole sputter magnetron plasma (without microwave injection). As revealed by probe measurements, this effect is due to the higher plasma density and electron temperature of the MECRIS plasma, leading to a difference of one order of magnitude and 7 eV, respectively. Additionally, the MECRIS plasma has been characterized by optical emission spectroscopy and simulated by a global and a two-dimensional model. Retrieved process parameter dependencies of plasma density, electron temperature, Al+ ion density, and Ar+ ion density coincide with probe findings. Although a discrepancy of the absolute values of partly up to two orders of magnitude is evident. Potentially, the Al+ ion current can be enhanced to the mA-region by optimizing the ion extraction system for minimal idle electrode currents and by rising sputter magnetron power as well as acceleration voltage above the actual limits of 10 kW and 30 kV, respectively.

In the thesis the development of two equipment for preparation of ultrathin films under ultrahign vacuum conditions (UHV) is discussed. Here, additionally to a brief description of theoretical principles, more details on the design of these units are given. In the first part the design of a thermal source of oxygen or hydrogen atomic beams is discussed. Further, a design and construction of an ion–atomic beam source for ion-beam assisted deposition of thin films is detailed. The source combines the principles of an efusion cell and electron-impact ion beam source generating ions of (30 – 100) eV energy. The source has been successfully applied for the growth of GaN on the Si(111) 7x7 substrate under room temperature.

Diploma thesis describes the design of an switched mode power supply with switching at zero voltage for driving the anode of Anode-layer type ion source. First aim of thesis is ion sources and specialy Anode-layer type of ion source in detail. Main aim of thesis are important aspects of the design of switching mode power supply, which comes later the detailed construction of an switched mode power supply with output voltage 2800 V at output power 2800 W.

A radio frequency (rf) quadrupole instrument, currently known as an Isobar Separator for Anions (ISA), has been integrated into an Accelerator Mass Spectrometry (AMS) system to facilitate anion–gas reactions before the tandem accelerator. An AMS Cs+ sputter source provided > 15 keV ions that were decelerated in the prototype ISA to < 20 eV for reaction in a single collision cell and re-accelerated for AMS analysis. Reaction based isobar suppression capabilities were assessed for smaller AMS systems and a new technique for gas–phase reaction studies was developed. Isobar suppression of 36S– and 12C3– for 36Cl analysis, and YF3– and ZrF3– for 90Sr analysis were studied in NO2 with deceleration to < 12 eV. Observed attenuation cross sections, σ [x 10^–15 cm^2], were σ(S– + NO2) = 6.6, σ(C3– + NO2) = 4.2, σ(YF3– + NO2) = 7.6, σ(ZrF3– + NO2) = 19. With 8 mTorr NO2, relative attenuations of S–/Cl– ~ 10^–6, C3–/Cl– ~ 10^–7, YF3–/SrF3– ~ 5 x 10^–5 and ZrF3–/SrF3– ~ 4 x 10^–6 were observed with Cl– ~ 30% and SrF3– > 90% transmission. Current isobar attenuation limits with < 1.75 MV accelerator terminal voltage and ppm impurity levels were calculated to be 36S–/Cl– ~ 4 x 10^–16, 12C3–/Cl– ~ 1.2 x 10^–16, 90YF3–/SrF3– ~ 10^–15 and 90ZrF3–/SrF3– ~ 10^–16. Using 1.75 MV, four 36Cl reference standards in the range 4 x 10^–13 < 36Cl/Cl < 4 x 10^–11 were analyzed with 8 mTorr NO2. The measured 36Cl/Cl ratios plotted very well against the accepted values. A sample impurity content S/Cl < 6 x 10^–5 was measured and a background level of 36S–/Cl < 9 x 10^–15 was determined. Useful currents of a wide variety of anions are produced in AMS sputter sources and molecules can be identified relatively unambiguously by stripping fragments from tandem accelerators. Reactions involving YF3–, ZrF3–, S– and SO– + NO2 in the ISA analyzed by AMS are described, and some interesting reactants are identified.

A radio frequency (rf) quadrupole instrument, currently known as an Isobar Separator for Anions (ISA), has been integrated into an Accelerator Mass Spectrometry (AMS) system to facilitate anion–gas reactions before the tandem accelerator. An AMS Cs+ sputter source provided > 15 keV ions that were decelerated in the prototype ISA to < 20 eV for reaction in a single collision cell and re-accelerated for AMS analysis. Reaction based isobar suppression capabilities were assessed for smaller AMS systems and a new technique for gas–phase reaction studies was developed. Isobar suppression of 36S– and 12C3– for 36Cl analysis, and YF3– and ZrF3– for 90Sr analysis were studied in NO2 with deceleration to < 12 eV. Observed attenuation cross sections, σ [x 10^–15 cm^2], were σ(S– + NO2) = 6.6, σ(C3– + NO2) = 4.2, σ(YF3– + NO2) = 7.6, σ(ZrF3– + NO2) = 19. With 8 mTorr NO2, relative attenuations of S–/Cl– ~ 10^–6, C3–/Cl– ~ 10^–7, YF3–/SrF3– ~ 5 x 10^–5 and ZrF3–/SrF3– ~ 4 x 10^–6 were observed with Cl– ~ 30% and SrF3– > 90% transmission. Current isobar attenuation limits with < 1.75 MV accelerator terminal voltage and ppm impurity levels were calculated to be 36S–/Cl– ~ 4 x 10^–16, 12C3–/Cl– ~ 1.2 x 10^–16, 90YF3–/SrF3– ~ 10^–15 and 90ZrF3–/SrF3– ~ 10^–16. Using 1.75 MV, four 36Cl reference standards in the range 4 x 10^–13 < 36Cl/Cl < 4 x 10^–11 were analyzed with 8 mTorr NO2. The measured 36Cl/Cl ratios plotted very well against the accepted values. A sample impurity content S/Cl < 6 x 10^–5 was measured and a background level of 36S–/Cl < 9 x 10^–15 was determined. Useful currents of a wide variety of anions are produced in AMS sputter sources and molecules can be identified relatively unambiguously by stripping fragments from tandem accelerators. Reactions involving YF3–, ZrF3–, S– and SO– + NO2 in the ISA analyzed by AMS are described, and some interesting reactants are identified.