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>Magister Scientiae - MSc / It is well known, that there is a severe lack of information available pertaining to neutron rich nuclei, specifically of those nuclei with mass numbers ≥ 60. These neutron rich nuclei are not easy to access in current experimental facilities or be produced with sufficient yield to allow for it to be studied. In order to expand our understanding of nuclear physics by studying the properties and characteristics of these nuclei, the development of new facilities producing Radioactive-ion Beams (RIBs) is required. The applications for RIBs are wide, allowing for deeper investigations into the properties of nuclei, their interactions and the manner in which they were formed in the early universe. Additionally, there are various interdisciplinary fields such as medicine, biology and material science in which RIBs can be utilized as a driving mechanism for new research and technological innovation. The iThemba Laboratory for Accelerator Based Sciences (iThemba LABS), South Africa, has proposed a new facility for the production and acceleration of radioactive-ion beams (RIBs). The RIB Project is to be developed in sequential phases and would produce a range of neutron-rich isotopes for low-energy materials science and nuclear physics research. Of specific interest, is the production of the Helium-6 isotope (6He), for its potential applications in various areas of nuclear physics research. The aim of this research work was to design, model and optimise a RIB production target capable of producing high intensity 6He beams, guided by the characteristics of the primary proton beam available for use at iThemba LABS. This research work/design study is however limited, due to the absence of experimentally measured and verified 6He cross section data for proton induced reactions on the proposed target materials (Graphite and Boron Carbide). However, best-estimate approaches were adopted through the use of validated computer codes. Additionally, all 6He yield results are presented as in-target yields, as this study did not cover the diffusion (isotope release) efficiency of the target systems in question. Three RIB production targets types were investigated using Graphite, Boron Carbide and Beryllium Oxide as potential target materials. Following numerous optimisation processes, a Boron Carbide RIB target was converged upon, proving to be suitable for the production of high intensity 6He beams at iThemba LABS, by meeting the material thermal and mechanical limiting criteria for operation. This target system was found to produce an in-target 6He yield rate of 2 ~ 3 x 1011 6He/s, considered sufficient for experimental application at iThemba LABS.

A possible mechanism to explain the origin of around 35 neutron–deficient stable isotopes with mass A≥75 between 74 Se and 196 Hg, known as the p–nuclei is the nucleosynthesis in the proton–rich neutrino–driven winds of core–collapse supernovae via the νp–process. However this production scenario is very sensitive to the underlying supernova dynamics and the nuclear physics input. As far as nuclear uncertainties are concerned, the breakout reaction from the pp-chains, 7Be(α, γ)11C, has been identified as an important link which can influence the nuclear flow and therefore the efficiency of the νp–process. However its reaction rate is not well known over the relevant energy range (T9 = 1.5–3). In this thesis we report on the direct first measurement of two resonances of the 7Be(α, γ)11 C reaction with previously unknown strengths using an intense radioactive 7Be beam from ISAC and the DRAGON recoil separator in inverse kinematics. Since resonance strength measurements with low mass beams using recoil separators depend strongly on the recoil angular distribution, which can exceed the acceptance of the separator, we first performed a proof–of–principle test by measuring a known resonance of the 6Li(α, γ)10B reaction, which also presents a similar challenge. Our results from the 6Li(α, γ)10B reaction are in agreement with literature, showing that DRAGON can measure resonance strengths of reactions for which the maximum momentum cone of the recoils exceeds its acceptance. From the newly measured 7Be(α, γ)11C resonance strengths we calculated the new reaction rate which is lower than the current recommended by 10–50% and constrained to 5–10% in the relevant temperature region. Using this new rate, we performed detailed nucleosynthesis calculations which suggest that there is no effect the production of light p–nuclei, but a production increase for CNO elements of up to an order of magnitude is observed. / Dissertation / Doctor of Philosophy (PhD)

Dans les milieux astrophysiques explosifs tels que les novae ou les sursauts X, la densité d'hydrogène et la température sont suffisamment grandes pour que le temps entre deux réactions impliquant un proton soit plus court que le temps de vie de certains ions radioactifs. La connaissance de la section efficace des réactions de capture d’un proton par un ion radioactif est un des ingrédients important permettant la modélisation de tels milieux. Dans ce travail, un nouveau dispositif expérimental permettant d'étudier la force de résonance de réactions (p,gamma) en cinématique inverse est présenté. Ce dispositif, baptisé ARES (Astrophysical REcoil Separator), a été d’abord caractérisé à l'aide de l'étude de la réaction 19F(p,gamma)20Ne et plus particulièrement de la mesure de la force de la résonance bien connue à 635 keV au dessus du seuil 19F+p. De plus, la simulation de cette expérience est en accord avec les mesures effectuées. Une première mesure de force de résonance d'une réaction impliquant un faisceau d'ions radioactifs est ensuite présentée. Il s'agit de la réaction 19Ne(p,gamma)20Na et plus particulièrement de la résonance à 448 keV au dessus du seuil 19Ne+p. Une limite supérieure de 15.2 meV avec un niveau de confiance de 90% est obtenue. Cette limite supérieure améliore légèrement les résultats de mesures antérieures. / In explosive astrophysical environments such as novae or X-ray bursts, the temperature and the hydrogen density are so large that the time between two reactions involving protons is smaller than the live time of radioactive ions. The cross section of such reactions is an important ingredient of the modeling of such environments. In this work, a new experimental device, allowing the study of resonance strength of (p,gamma) reactions, is presented. This setup, called ARES (Astrophysical REcoil Separator), is first characterized using the study of the well known reaction, 19F(p,gamma)20Ne and more precisely the measurement of the resonance strength of the 635 keV level above the 19F+p threshold. The simulation of this experiment is found in good agreement with the measurement. Then the first resonance strength measurement of a reaction involving radioactive ions beams is presented, i.e. the resonance strength of the 448 keV level above the 19Ne+p threshold in the 19Ne(p,gamma)20Na reaction. An upper limit of 15.2 meV with a confidence level of 90% is obtained. This upper limit improves slightly the results of previous measurements.

Une extension de la surface de masses atomiques dans la région A ≈ 100 est présentée par l’intermédiaire des mesures de masse des isotopes 100-102Sr et 100-102Rb. Les mesures ont été effectuées avec le spectromètre de masse ISOLTRAP constitué de différents pièges à ions. Les premières mesures directes des masses des 100-102Sr et du 100-102Rb sont rapportées ici. Ces mesures confirment la continuité de la région de déformation nucléaire avec l’augmentation du nombre de neutrons jusqu’à N = 65.De sorte à interpréter la déformation dans la chaine isotopique du strontium et à déterminer si une déformation peut apparaitre pour des isotopes de krypton plus lourds, une comparaison est faite entre les données expérimentales et des résultats de calculs théoriques disponibles dans la littérature. Pour compléter ces comparaisons, des calculs Hartree-Fock-Bogoliubov pour des isotopes pairs et impairs sont aussi présentés, illustrant la compétition entre formes nucléaires dans la région.Le développement d’une source d’ions à ionisation par électro nébuliseur est présenté. Cette source peut produire un large panel de masses isobariques destinées à la calibration. La première mise en service de la source est présentée, incluant les résultats des premiers balayages en masse détectés derrière le spectromètre de masse quadripolaire. Une résolution de quelques unités de masses atomiques a été atteinte. / An extension of the atomic mass surface in the region A ≈ 100 is performed via massmeasurements of the 100-102Sr and 100-102Rb isotopes with the ion-trap mass spectrometer ISOLTRAPat CERN-ISOLDE. The first direct mass measurements of 102Sr and 101;102Rb are reported here. Thesemeasurements confirm the continuation of the region of nuclear deformation with the increase of neutronnumber, at least as far as N = 65.In order to interpret the deformation in the strontium isotopic chain and to determine whether an onsetof deformation is present in heavier krypton isotopes, a comparison is made between experimentalvalues and theoretical calculations available in the literature. To complete this comparison, Hartree-Fock-Bogoliubov calculations for even and odd isotopes are also presented, illustrating the competitionof nuclear shapes in the region.The development of an electrospray ionization ion source is presented. This source can delivera large range of isobaric masses for calibration purposes. The early commissioning of the sourceis discussed, including the results from the first mass scans detected behind the quadrupole massspectrometer. A resolution of a few atomic mass units is reached.

Thesis (Ph.D.); Submitted to the UNIVERSITY OF CALIFORNIA, BERKELEY, CA (US); 9 Dec 2004. / Published through the Information Bridge: DOE Scientific and Technical Information. "LBNL--56744" Guo, Fanqing. USDOE Director. Office of Science. Office of Nuclear Physics (US) 12/09/2004. Report is also available in paper and microfiche from NTIS.