Precision measurements of superallowed Fermi β-decay allow for stringent tests of the magnitude of isospin-symmetry-breaking effects in nuclei, the validity of the conserved vector current hypothesis, and the unitarity of the Cabibbo-Kobayashi-Maskawa (CKM) quark-mixing matrix. A high-precision measurement of the branching ratio for the superallowed β+ decay of 74Rb has been performed at the Isotope Separator and ACcelerator (ISAC) facility at TRIUMF. The 8π spectrometer, an array of 20 HPGe detectors, was used to detect γ-rays emitted following the Gamow-Teller and non-analogue Fermi β-decays of 74Rb. PACES, an array of 5 Si(Li) detectors, was used to detect emitted conversion electrons, while half of SCEPTAR, a close-packed array of 10 plastic scintillators, was used to detect emitted β particles. In this experiment, 23 excited states were identified in 74Kr which were populated following the β-decay of 74Rb. A total of 58 γ-rays were identified following the 8.241(4)x108 detected β-particles. An observed non-superallowed branching ratio of 0.396(7)% was determined from the intensity of the identified γ-rays, while the unobserved non-superallowed intensity was calculated to be 0.05(5)%, leading to a superallowed branching ratio of 99.55(5)%. The superallowed branching ratio is now the most precise experimental quantity in the determination of the superallowed ft-value of 74Rb. Combining the half-life and Q-value with the superallowed branching ratio measured in this work leads to a superallowed ft-value of 3082.6(66) s. Finally, comparisons between the superallowed ft-value, the world average Ft-value, and the non-analogue Fermi branching ratio are made to provide future guidance in the refinement of the theoretical models required to describe the crucial isospin-symmetry-breaking term in superallowed β-decay.

This work presents a study of the electronic structure of four transition metal oxides (TMOs) using spectroscopic data and a variety of theoretical models. TMOs are a class of materials made from d-block metals in the periodic table, and one or more oxygen atoms. The nature of d-electrons is examined and theoretical models used to treat d-electron systems are tested against experimental data. Background theory of condensed matter physics is outlined. An overview of density functional theory (DFT) as a theoretical model for calculating the electronic structure of materials is presented. A variety of exchange-correlation (XC) functionals used within the DFT framework are outlined and tested for their applicability to the TMO systems in question. X-ray spectroscopy is briefly outlined and used to test the validity of the different XC functionals. All four compounds, AgO, Ag2O, CuO, and Cu2O require a Hubbard U term in the XC functional to most accurately reproduce experimental results. The effects of varying the value of U is examined in depth. The oxygen K-edge X-ray emission spectra (XES) exhibits a“two peak” structure for all compounds; the effect of varying the U value is to change the intensity ratio of the two peaks. The ratio of the two peaks as a function of U shows a linear trend in all compounds. A simple line is fit to the peak ratio vs. U curve. A common line between all compounds would provide an important metric with which to predict the appropriate U value needed in similar materials based on simple experimental data. However, the parameters of the fitted line were not common between the four compounds and any metric derived from this method would be system-dependent and not widely applicable to other systems. There are, however, interesting trends in the data when the U value is varied that provide subjects for future research. A number of fundamental quantities are determined both from experiment and theoretical calculations. Calculated bandgap values are shown to be lower than the experimental values for most functionals tested. This is not unexpected as DFT methods are known to predict much smaller bandgaps than expected. The Heyd-Scuseria-Ernzerhof (HSE) functional used for Ag2O and Cu2O does predict the bandgaps very accurately. The core-hole effect is estimated and proven to be negligible in these systems. Charge transfer and on-site Coulomb repulsion energies, important quantities in the electronic behaviour of TMOs, are determined and compared to previously reported values.

Le travail présenté dans ce manuscrit regroupe quatre études par spectroscopie gamma de quatre noyaux produits par une réaction de fission induite par protons de 25 MeV, sur une cible épaisse d'238U. Cette expérience a été menée au JYFL à Jyväskylä auprès du multidétecteur JUROGAM II. Dans ce manuscrit l'étude spectroscopique détaillée des noyaux : 84Se, 86Se, 83As et 98Y a été menée. Les trois premiers noyaux sont des noyaux sphériques se situant au voisinage de la couche magique N = 50. Leurs études peuvent permettre de mieux aborder l'évolution du gap de cette couche, mais aussi d'améliorer les interactions utilisées dans les calculs de modèle en couches permettant de reproduire leurs comportements. Huit nouvelles transitions ont pu être assignées à ces noyaux, ces résultats expérimentaux sont relativement bien en accord avec les calculs de modèle en couches effectués. Le noyau 98Y est un noyau possédant une coexistence de formes nucléaires. Alors que les états d'énergies inférieures à 500keV ont une configuration sphérique, les états situés au dessus sont déformés. Cinq nouvelles transitions ont été déterminées et ajoutées au schéma de niveaux existants, et deux calculs utilisant deux modèles collectifs ont été réalisés. Le premier utilisant le modèle GICM reproduit le comportement des états au dessous de 500keV et le deuxième QPRM reproduit les états prolate déformés permettant l'assignation d'un comportement sphérique à l'isomère (10-). / The work presented in this thesis includes four gamma-ray spectroscopy studies of four nuclei produced by fission induced by 25 MeV protons, on a thick target of 238U. This experiment was realized at JYFL in Jyväskylä with the multi-detector JUROGAM II. In this manuscript a detailed spectroscopic study of nuclei : 84Se, 86 Se, 83 As and 98Y was performed. The first three nuclei are spherical and they are on or adjacent to the N =50 shell closure. Their studies provide a better understanding of the possible decrease in energy of this shell closure, and also of the interactions used in shell-model calculations. Eight new transitions have been assigned to these nuclei and these experimental results are in a relatively good agreement with the shell-model calculations. In the nucleus 98Y a coexistence of nuclear shapes is observed. While the low-energy states below 500keV have a spherical configuration, higher lying states are deformed. Five new transitions were discovered and added to the existing levels scheme, and two calculations using two collective models have been made. The first set of calculations has used the GICM model to reproduce the behavior of states below 500keV and the second set of calculations has used QPRM to reproduce the prolate deformed states, and permitted the assignment of a spherical shape to the isomer (10-).

Made available in DSpace on 2014-10-09T12:49:50Z (GMT). No. of bitstreams: 0 / Made available in DSpace on 2014-10-09T14:02:57Z (GMT). No. of bitstreams: 0 / Tese (Doutoramento) / IPEN/T / Instituto de Pesquisas Energeticas e Nucleares - IPEN/CNEN-SP

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Made available in DSpace on 2014-10-09T12:41:06Z (GMT). No. of bitstreams: 0 / Made available in DSpace on 2014-10-09T14:09:09Z (GMT). No. of bitstreams: 1 04673.pdf: 4338286 bytes, checksum: 9b40b59ddc2764691461410ae0194329 (MD5) / Dissertacao (Mestrado) / IPEN/D / Instituto de Pesquisas Energeticas e Nucleares - IPEN/CNEN-SP

Submitted by Claudinei Pracidelli (cpracide@ipen.br) on 2014-11-10T12:24:02Z No. of bitstreams: 0 / Made available in DSpace on 2014-11-10T12:24:02Z (GMT). No. of bitstreams: 0 / Tese (Doutorado em Tecnologia Nuclear) / IPEN/T / Instituto de Pesquisas Energeticas e Nucleares - IPEN-CNEN/SP

Alvos naturais de Mg, Al, Si, Cr, Ti, Ni e Zr foram irradiados com prótons e as seções de choque para várias reações nucleares foram determinadas a energias inferiores a 30 MeV. As irradiações foram efetuadas nos ciclotrons CV-28 e CYCLONE 30 do IPEN, que possuem energia nominal de 24 e 30 MeV, respectivamente. O feixe de prótons foi monitorado por meio de lâminas de Cu ou a partir da formação de nuclídeos na própria amostra com seção de choque conhecida para as energias utilizadas. Especial interesse foi dedicado às reações raras di tipo (p, 2alfa) e (p, ANTPOT.3 H) das quais existem, em geral, poucos dados publicados, principalmente para energias próximas do limiar. A determinação da seção de choque foi realizada a partir da medida da atividade residual dos produtos pelo método de espectroscopia gama simples. Um detector HPG com resolução menor que 2 keV foi utilizado. Devido ao valor reduzido da seção de choque das reações de interesse no intervalo de energia considerado, uma análise estatística cuidadosa dos dado foi necessária. Em áreas reduzidas dos picos detectados precisaram da quantificação, em alguns casos, da contribuição de nuclídeos formados na própria amostra por outras reações, a partir de impurezas ou provenientes do fundo radioativo. Entre os produtos obtidos encontram-se os nuclídeos ANTPOT.22 Na, ANTPOT.26 Al, ANTPOT.44 Ti, e ANTPOT.54 Mn. A detecção de ANTPOT.26 Al nas amostras de Al e Si, permitiu estimar os limites do método proposto para o estudo de reações raras de interesse astrofísico. No total, são apresentados neste trabalho 72 valores de seção de choque. Desse total, 21 dados são apresentados pela primeira vez ou foram obtidos pela primeira vez pelo método proposto ou às energias estudadas. Os resultados mais importantes referem-se às reações ANTPOT.29 Si(p, 2alfa)ANTPOT.22 Na,ANTPOT.53 Cr(p, 2alfa)ANTPOT.46 Sc, ANTPOT.46 Ti(p, ANTPOT.3 H)ANTPOT.44 Ti, )ANTPOT.58 Ni(p, ANTPOT.3 H)ANTPOT.56 Ni e ANTPOT.90 Zr(p, ANTPOT.3 H)ANTPOT.88 Zr. Os resultados foram comparados com valores publicados na literatura e com o resultado do cálculo realizado a partir de modelos teóricos conhecidos, permitindo a obtenção de conclusões relativas ao método experimental, assim como aos mecanismos da reação envolvidos. / Natural targets of Mg, Al, Si, Cr, Ti, Ni and Zr were irradiated with protons and the cross section for several reactions were determined for incident energies up to 30 MeV. The irradiations were performed at the CV-28 and CYCLONE 30 cyclotrons from the IPEN, which have nominal energies of 24 and 30 MeV, respectively. The protons beams were monitored by copper foils or by the nuclide formation in the irradiated targets with known cross sections for the used energy. Special interest was dedicated to rare reactions of the (p, 2alfa) and (p, ANTPOT.3 H) kind, from which we have a few published data, mainly for energies near the threshold. The cross section determination was accomplished by the residual actives measurement of the reaction products by the simple gamma spectroscopy method using an HPGe detector with resolution better than 2 keV. Due to the low value of the cross section for the considered reaction, a careful statistical analysis of the obtained data was needed. The small areas of the detected peaks required the quantification of the contributions of nuclides produced by others reactions, from contaminants or from the radioactive background. Among others, the ANTPOT.22 Na, ANTPOT.26 Al, ANTPOT.44 Ti and ANTPOT.54 Mn products have been detected. The detection of ANTPOT.26 Al in the Al and Si targets allow the estimation of the limits of the proposed method for the study of astrophysical interest reaction. In total, 72 cross section values are being presented. Out of this amount, 21 are being presented for the first time or have been obtained for the first time by the method or for the studied energies. The most important results refer to the ANTPOT.29 Si(p, 2gamma)²²Na, ANTPOT.53 Cr(p, 2gamma)ANTPOT.46 Sc, ANTPOT.46 Ti(p, ANTPOT.3 H)ANTPOT.44 Ti, ANTPOT.58 Ni(p, ANTPOT.3 H)ANTPOT.56 Ni and ANTPOT.90 Zr(p, ANTPOT.3 H)ANTPOT.88 Zr reactions. The results have been compared to published vales and calculations using known theoretical models, allowing the achievement of conclusions related to the experimental method, as well as the reaction mechanism involved.

Made available in DSpace on 2014-10-09T12:49:50Z (GMT). No. of bitstreams: 0 / Made available in DSpace on 2014-10-09T14:02:57Z (GMT). No. of bitstreams: 0 / Tese (Doutoramento) / IPEN/T / Instituto de Pesquisas Energeticas e Nucleares - IPEN/CNEN-SP

Made available in DSpace on 2014-10-09T12:26:44Z (GMT). No. of bitstreams: 0 / Made available in DSpace on 2014-10-09T14:06:15Z (GMT). No. of bitstreams: 0 / O hidrogênio vem sendo muito utilizado como agente pulverizador de ligas à base de terras raras e metais de transição devido à sua taxa de difusão ser extremamente alta mesmo em baixas temperaturas. Tais materiais são utilizados em dispositivos de estocagem de hidrogênio, geração de eletricidade ou de campos magnéticos, que são produzidos através de um processo cuja primeira etapa é a transformação das ligas em um pó fino através de moagem. Além destas, o hidrogênio também está sendo utilizado para a obtenção de ligas à base de titânio nióbio zircônio para sua pulverização. Para a fabricação destas ligas a metalurgia do pó é utilizada, pois com ela é possível obter como resultado peças com superfície porosa, requisito para sua aplicação como biomateriais. Outras vantagens da utilização da metalurgia do pó na fabricação dessas ligas são melhor acabamento superficial e melhor homogeneidade microestrutural. Neste trabalho foram preparadas amostras na composição Ti-13Nb-13Zr. A hidrogenação foi realizada a 700°C, 600°C e a 500°C para o titânio, nióbio e zircônio, respectivamente. Após a hidrogenação, foram realizadas moagens em moinho do tipo planetário de alta energia utilizando velocidade de 200rpm durante 90 minutos, e moinho convencional de bolas durante 30h. As amostras foram prensadas em prensa uniaxial e em seguida em prensa isostática e então sinterizadas a 1150°C com tempo de patamar de 7 a 13h. As amostras foram caracterizadas microestruturalmente por microscopia eletrônica de varredura (MEV), espectroscopia de energia dispersiva (EDS) e difração de raios X. As propriedades estruturais e mecânicas determinadas foram de densidade, microdureza e módulo de elasticidade. A amostra sinterizada a 1150°C por 7h, hidrogenada com pressão de 10.000 mbar e produzida por moagem em moinho planetário de alta energia apresentou melhores propriedades mecânicas e boa homogeneidade microestrutural, obtendo a composição final da liga Ti-13Nb- 13Zr. / Dissertacao (Mestrado) / IPEN/D / Instituto de Pesquisas Energeticas e Nucleares - IPEN-CNEN/SP