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Made available in DSpace on 2014-10-09T12:53:57Z (GMT). No. of bitstreams: 0 / Made available in DSpace on 2014-10-09T14:09:29Z (GMT). No. of bitstreams: 0 / No presente trabalho foi desenvolvida uma técnica radiográfica para a inspeção de amostras finas, que emprega feixes de partículas - ? como radiação penetrante e, detectores de traços nucleares de estado sólido para o registro da imagem. O feixe é gerado em uma tela de boro natural quando irradiada com nêutrons térmicos e o detector utilizado foi o CR-39. A interação das partículas - ? com o detector geram danos, os quais sob a ação de uma solução química adequada transformam-se em traços, as unidades básicas formadoras da imagem. Foi desenvolvido um sistema digital próprio para a aquisição, análise e processamento dos dados e das imagens registradas nos detectores. As condições ótimas de irradiação e de revelação para a obtenção de uma radiografia são 1,3 horas e 25 minutos a 70°C, respectivamente. Nestas condições a técnica é capaz de analisar amostras com até 10?m de espessura, com uma resolução espacial de 32?m. O emprego do sistema digital permitiu uma redução significativa no tempo despendido para a aquisição e análise de dados e, uma melhoria na visualização das imagens radiográficas registradas. Além disto permitiu acesso a novos dados referentes aos traços registrados, o que abriu novas perspectivas de pesquisa pois, tem-se acesso aos parâmetros fundamentais que norteiam a teoria da formação da imagem em detectores de traços nucleares utilizada neste trabalho. São apresentadas algumas radiografias que demonstram a potencialidade da técnica desenvolvida. Quando comparada com as outras técnicas radiográficas usuais, empregadas para inspecionar amostras finas, a desenvolvida no presente trabalho permite um menor tempo para a obtenção da imagem, não é necessário a manipulação de materiais radioativos líquidos e, o filme empregado é praticamente insensível às radiações ?, ?, raios - X e luz visível. / Tese (Doutoramento) / IPEN/T / Instituto de Pesquisas Energéticas e Nucleares - IPEN-CNEN/SP

Les observations astronomiques et cosmologiques suggèrent fortement la présence d’une matière exotique, non-relativiste et non-baryonique qui représenterait 26% du contenu de masse-énergie de l’Univers actuel. Cette matière dite sombre et froide serait compo- sée de particules neutres, massives et interagissant faiblement avec la matière ordinaire (WIMP : Weakly Interactive Massive Particles). Le projet PICASSO (Projet d’Identification des CAndidats Supersymétriques de la matière SOmbre) est une des expériences installées dans le site souterrain de SNOLAB à Sudbury en Ontario, qui tente de détecter directement un des candidats de la matière sombre, proposé dans le cadre des extensions supersymétriques du modèle standard : le neutralino. Pour cela, PICASSO utilise des détecteurs à gouttelettes surchauffées de C4F10, basés sur le principe de la chambre à bulles. Les transitions de phase dans les liquides surchauffés peuvent être déclenchées par le recul du 19 F, causé par une collision élastique avec les neutralinos. La nucléation de la gouttelette génère une onde sonore enregistrée par des senseurs piézo-électriques. Cette thèse présentera les récents progrès de l’expérience PICASSO qui ont conduit à une augmentation substantielle de sa sensibilité dans la recherche du neutralino. En effet, de nouvelles procédures de fabrication et de purification ont permis de réduire à un facteur de 10, la contamination majeure des détecteurs, causée par les émetteurs alpha. L’étude de cette contamination dans les détecteurs a permis de localiser la source de ces émetteurs. Les efforts effectués dans le cadre de l’analyse des données, ont permis d’améliorer l’effet de discrimination entre des évènements engendrés par les particules alpha et par les reculs nucléaires. De nouveaux outils d’analyse ont également été implémentés dans le but de discriminer les évènements générés par des particules de ceux générés par des bruits de fond électroniques ou acoustiques. De plus, un mécanisme important de suppression de bruit de fond indésirable à haute température, a permis à l’expérience PICASSO d’être maintenant sensible aux WIMPs de faibles masses. / Astronomical and cosmological observations strongly suggest the presence of an exotic form of non-relativistic, non-baryonic matter that would represent 26% of the actual energy-matter content of the Universe. This so-called cold dark matter would be composed of Weakly Interactive Massive Particles (WIMP). PICASSO (Project In CAnada to Search for Supersymmetric Objects) aims to detect directly one of the dark matter candidates proposed in the framework of supersymmetric extensions of the standard model : the neutralino. The experiment is installed in the SNOLAB underground laboratory at Sudbury (Ontario) and uses superheated C4F10 droplets detectors, a variant of bubble chamber technique. Phase transitions in the superheated liquids are triggered by 19 F recoils caused by the elastic collision with neutralinos and create an acoustic signal which is recorded by piezoelectric sensors. This thesis presents recent progress in PICASSO leading to a substantially increased sensitivity in the search of neutralinos. New fabrication and purification procedures allowed a background reduction of about a factor 10 of the major detectors contamination caused by alpha emitters. Detailed studies allowed to localize these emitters in the detectors. In addition, data analysis efforts were able to improve substantially the discrimination between alpha particle induced events and those created by nuclear recoils. New analysis tools were also developed in order to discriminate between particle induced and non-particle induced events, such as electronic backgrounds and acoustic noise signals. An important new background suppression mechanism at higher temperatures led to the present improved sensitivity of PICASSO at low WIMP masses.

Energy resolution characteristics of silicon surface barrier detector signals amplified by different preamplifiers and spectroscopic amplifiers have been studied. The characterization has been done using alpha particles from an 241Am source and spontaneous fission fragments from two Cf sources. The alpha and spontaneous fission activities of the sources have been measured and the isotopic compositions, ages, and initial activities of the two Cf sources have been calculated using the results from the activity measurements. 82.3% and 82.5% of the spontaneous fission activity of the two sources is found to originate from 252Cf. Heavy ion detection properties of two Si detector setups have been determined by measuring spontaneous fission fragments from one of the Cf sources in coincidence. The mass distribution of fission fragments is derived from the pulse spectra of the coincidence measurements. The conditions for future time resolution measurements have been established. Inquiries on commercially available ultra-thin Si detectors have been made. The purpose is to upgrade detector telescopes to lower the energy threshold of ΔE-ΔE-E identification of particles from neutroninduced nuclear reactions. Three manufacturers of Si detectors with thickness 20-25 µm and active area around 450 mm2 have been listed together with properties of the three offered detectors.

This thesis concerns heating and current drive in tokamak plasmas using the fast magnetosonic wave in the ion cyclotron range of frequencies. Fast wave heating is a versatile heating method for thermonuclear fusion plasmas and can provide both ion and electron heating and non-inductive current drive. Predicting and interpreting realistic heating scenarios is however difficult due to the coupled evolution of the cyclotron resonant ion velocity distributions and the wave field. The SELFO code, which solves the coupled wave equation and Fokker-Planck equation for cyclotron resonant ion species in a self-consistent manner, has been upgraded to allow the study of more advanced fast wave heating and current drive scenarios in present day experiments and in preparation for the ITER tokamak. Theoretical and experimental studies related to fast wave heating and current drive with emphasis on fast ion effects are presented. Analysis of minority ion cyclotron current drive in ITER indicates that the use of a hydrogen minority rather than the proposed helium-3 minority results in substantially more efficient current drive. The parasitic losses of power to fusion born alpha particles and beam injected ions are concluded to be acceptably low. Experiments performed at the JET tokamak on polychromatic ion cyclotron resonance heating and on fast wave electron current drive are presented and analysed. Polychromatic heating is demonstrated to increase the bulk plasma ion to electron heating ratio, in line with theoretical expectations, but the fast wave electron current drive is found to be severely degraded by parasitic power losses outside of the plasma. A theoretical analysis of parasitic power losses at radio frequency antennas indicates that the losses can be significantly increased in scenarios with low wave damping and with narrow antenna spectra, such as in electron current drive scenarios. / QC 20100506

Les observations astronomiques et cosmologiques suggèrent fortement la présence d’une matière exotique, non-relativiste et non-baryonique qui représenterait 26% du contenu de masse-énergie de l’Univers actuel. Cette matière dite sombre et froide serait compo- sée de particules neutres, massives et interagissant faiblement avec la matière ordinaire (WIMP : Weakly Interactive Massive Particles). Le projet PICASSO (Projet d’Identification des CAndidats Supersymétriques de la matière SOmbre) est une des expériences installées dans le site souterrain de SNOLAB à Sudbury en Ontario, qui tente de détecter directement un des candidats de la matière sombre, proposé dans le cadre des extensions supersymétriques du modèle standard : le neutralino. Pour cela, PICASSO utilise des détecteurs à gouttelettes surchauffées de C4F10, basés sur le principe de la chambre à bulles. Les transitions de phase dans les liquides surchauffés peuvent être déclenchées par le recul du 19 F, causé par une collision élastique avec les neutralinos. La nucléation de la gouttelette génère une onde sonore enregistrée par des senseurs piézo-électriques. Cette thèse présentera les récents progrès de l’expérience PICASSO qui ont conduit à une augmentation substantielle de sa sensibilité dans la recherche du neutralino. En effet, de nouvelles procédures de fabrication et de purification ont permis de réduire à un facteur de 10, la contamination majeure des détecteurs, causée par les émetteurs alpha. L’étude de cette contamination dans les détecteurs a permis de localiser la source de ces émetteurs. Les efforts effectués dans le cadre de l’analyse des données, ont permis d’améliorer l’effet de discrimination entre des évènements engendrés par les particules alpha et par les reculs nucléaires. De nouveaux outils d’analyse ont également été implémentés dans le but de discriminer les évènements générés par des particules de ceux générés par des bruits de fond électroniques ou acoustiques. De plus, un mécanisme important de suppression de bruit de fond indésirable à haute température, a permis à l’expérience PICASSO d’être maintenant sensible aux WIMPs de faibles masses. / Astronomical and cosmological observations strongly suggest the presence of an exotic form of non-relativistic, non-baryonic matter that would represent 26% of the actual energy-matter content of the Universe. This so-called cold dark matter would be composed of Weakly Interactive Massive Particles (WIMP). PICASSO (Project In CAnada to Search for Supersymmetric Objects) aims to detect directly one of the dark matter candidates proposed in the framework of supersymmetric extensions of the standard model : the neutralino. The experiment is installed in the SNOLAB underground laboratory at Sudbury (Ontario) and uses superheated C4F10 droplets detectors, a variant of bubble chamber technique. Phase transitions in the superheated liquids are triggered by 19 F recoils caused by the elastic collision with neutralinos and create an acoustic signal which is recorded by piezoelectric sensors. This thesis presents recent progress in PICASSO leading to a substantially increased sensitivity in the search of neutralinos. New fabrication and purification procedures allowed a background reduction of about a factor 10 of the major detectors contamination caused by alpha emitters. Detailed studies allowed to localize these emitters in the detectors. In addition, data analysis efforts were able to improve substantially the discrimination between alpha particle induced events and those created by nuclear recoils. New analysis tools were also developed in order to discriminate between particle induced and non-particle induced events, such as electronic backgrounds and acoustic noise signals. An important new background suppression mechanism at higher temperatures led to the present improved sensitivity of PICASSO at low WIMP masses.

De nombreuses études ont montré que l'exposition de cultures cellulaires à des particules α conduit à des changements biologiques importants autant dans les cellules irradiées que dans les cellules bystander non-irradiées. L'étude des réponses biologiques non-ciblées dans des cultures cellulaires exposées à de faibles fluences d’ions lourds permet d’estimer les risques pour la santé du rayonnement spatial et de la radiothérapie. Nous avons caractérisé les mécanismes sous-jacents de l'induction d'effets stressants dans des cultures confluentes de fibroblastes normaux humains exposés à de faibles fluences d’ions fer de 1000 MeV/u (transfert d'énergie linéique (TEL) ~151 keV/µm), d’ions silicium de 600 MeV/u (TEL ~50 keV/µm) ou d’ions carbone de 290 MeV/u (TEL ~13 keV/µm). Nous avons comparé ces résultats avec ceux obtenus dans des cultures cellulaires exposées, en parallèle, à de faibles fluences de particules α de 0,92 MeV/u (TEL ~109 keV/µm). L'induction de dommages à l'ADN, les changements dans l'expression des gènes, la carbonylation des protéines et la peroxydation lipidique durant les 24 h suivant l'exposition de cultures confluentes à de faibles doses (0,2 cGy et plus) d’ions fer ou d'ions silicium ont très largement contribué à la propagation d’effets stressants des cellules irradiées aux cellules bystander non-irradiées. Pour une dose moyenne de 0,2 cGy, seules ~1 et 3 % des cellules seraient irradiées dans le noyau par un ion, respectivement, fer ou silicium. Les immunoblots ont révélés des augmentations significatives des niveaux de phospho-TP53 (sérine 15), p21Waf1 (CDKN1A), HDM2, phospho-ERK1/2, de carbonylation des protéines et de peroxydation lipidique dans les 24 h suivant l’exposition. L'ampleur de ces réponses suggère la participation de cellules non ciblées dans les effets observés. De plus, lorsque les populations cellulaires irradiées ont été ré-ensemencées dans un milieu de culture frais peu après l'irradiation, les niveaux de ces marqueurs ont aussi augmentés durant 24 h. Ensemble, ces résultats montrent un effet rapidement propagé et persistant. Des analyses in situ réalisées dans des cultures cellulaires confluentes ont montré que la formation de foyers de la protéine 53BP1, marqueur de dommages à l'ADN, touchait un nombre de cellules plus important que celui auguré par la fraction de cellules traversées dans le noyau par un ion fer ou silicium. Cet effet est exprimé dès 15 min suivant l'exposition, atteint son maximum 1 h après l’exposition puis diminue jusqu’à 24 h. Une tendance similaire s'est produite après exposition à une dose moyenne absorbée de 0,2 cGy de particules α de 3,7 MeV, mais non après 0,2 cGy d’ions carbone de 290 MeV/u.Des analyses utilisant des puits de cultures intégrant une fine épaisseur de CR-39, détecteur solide de traces nucléaires, et permettant ainsi l’identification des cellules irradiées aux ions fer ou silicium, confirment la participation de cellules bystander dans la réponse au stress. Des études mécanistiques ont, de plus, indiqué que les jonctions gap permettant la communication intercellulaire, certaines voies de la réparation de l’ADN, ainsi que le métabolisme oxydatif participent à la propagation des effets non ciblés induit par des radiations de haut TEL. Nous avons également examiné la contribution possible des particules secondaires produites le long des traces d’ions primaires dans les réponses biologiques. Les simulations réalisées avec le code de transport de particules FLUKA ont révélé que la dose due aux produits de fragmentation, autres que les électrons, est inférieure à 1 % de la dose absorbée dans les cultures cellulaires exposées à des ions lourds. De plus, la dose radiale des ions lourds secondaires est limitée à ~10-20 µm autour de l’ion primaire. Ainsi, ces derniers sont peu susceptibles de contribuer de manière significative à la réponse biologique observée dans des cellules non ciblées par des ions lourds primaires / Widespread evidence indicates that exposure of cell cultures to α particles results in significant biological changes in both the irradiated and non-irradiated bystander cells in the population. The induction of non-targeted biological responses in cell cultures exposed to low fluences of high charge (Z) and high energy (E) particles is relevant to estimates of the health risks of space radiation and to radiotherapy. Here, we investigated the mechanisms underlying the induction of stressful effects in confluent normal human fibroblast cultures exposed to low fluences of 1000 MeV/u iron ions (linear energy transfer (LET) ~151 keV/µm), 600 MeV/u silicon ions (LET ~50 keV/µm) or 290 MeV/u carbon ions (LET ~13 keV/µm). We compared the results with those obtained in cell cultures exposed, in parallel, to low fluences of 0.92 MeV/u α particles (LET ~109 keV/µm).Induction of DNA damage, changes in gene expression, protein carbonylation and lipid peroxidation during 24 h after exposure of confluent cultures to mean doses as low as 0.2 cGy of iron or silicon ions strongly supported the propagation of stressful effects from irradiated to bystander cells. At a mean dose of 0.2 cGy, only ~1 and 3 % of the cells would be targeted through the nucleus by an iron or silicon ion, respectively. Within 24 h post-irradiation, immunoblot analyses revealed significant increases in the levels of phospho-TP53 (serine 15), p21Waf1 (also known as CDKN1A), HDM2, phospho-ERK1/2, protein carbonylation and lipid peroxidation. The magnitude of the responses suggested participation of non-targeted cells in the response. Furthermore, when the irradiated cell populations were subcultured in fresh medium shortly after irradiation, greater than expected increases in the levels of these markers were also observed during 24 h. Together, the results imply a rapidly propagated and persistent bystander effect. In situ analyses in confluent cultures showed 53BP1 foci formation, a marker of DNA damage, in more cells than expected based on the fraction of cells traversed through the nucleus by an iron or silicon ion. The effect was expressed as early as 15 min after exposure, peaked at 1 h and decreased by 24 h. A similar tendency occurred after exposure to a mean absorbed dose of 0.2 cGy of 3.7 MeV α particles, but not after 0.2 cGy of 290 MeV/u carbon ions.Analyses in dishes that incorporate a CR-39 solid state nuclear track detector bottom identified the cells irradiated with iron or silicon ions and further supported the participation of bystander cells in the stress response. Mechanistic studies indicated that gap junction intercellular communication, DNA repair, and oxidative metabolism participate in the propagation of the induced effects.We also considered the possible contribution of secondary particles produced along the primary particle tracks to the biological responses. Simulations with the FLUKA multi-particle transport code revealed that fragmentation products, other than electrons, in cells cultures exposed to HZE particles comprise <1 % of the absorbed dose. Further, the radial spread of dose due to secondary heavy ion fragments is confined to approximately 10-20 µm Thus, the latter are unlikely to significantly contribute to the stressful effects in cells not targeted by primary HZE particles.

Parallel-plate avalanche counters, PPACs, are commonly used to detect fission fragments. The PPAC detects them and mark (very accurately) the time of detection. Such measurements can be used to measure the neutron energy (via time-of-flight) to study neutron-induced fission.This project report provides a method that, together with the discussed improvements, allows the fabrication of good quality PPAC detectors. Several PPACs are manufactured and the electrodes are built from 0.9 µm thick mylar foils which are evaporated with a 40-80 nm thin layer of aluminum.The developed PPACs are characterized with well known radioactive Cf and Am sources (the source characterization also found in this report), and compared against each other. Additionally, the PPAC signal amplitude spectrum are found to follow theoretical expectations with regards to angular dependence, gas pressure and an applied electrode voltage.At a specific applied electrode voltage and range of gas pressures (3-9 mbar), the measured time resolutions are 2.24-1.38 ns. A trend is observed for finer time resolutions at higher gas pressures. / Parallel-plate avalanche counters, PPACs, används ofta för att detektera fissionsfragment. PPAC:en detekterar fragmenten med väldigt god tidsupplösning och således kan PPAC detektorer användas till att mäta neutron energier (mha. flygtidsmetoden), vilka uppmätts för att studera neutroninducerad fission.Det här projektet och den här rapporten beskriver en metod, med föreslagna förbättringar, som möjliggör tillverkning av PPAC detektorer av bra kvalitet. Under projektet har flera PPACs byggts med elektroder gjorda av 0.9 µm tunn mylar förångade med 40-80 nm aluminium. De tillverkade PPAC detektorerna är karaktäriserade med väl kända radioaktiva Cf- och Am-källor (dessa karaktäriseras även i den här rapporten). Detektorerna är sedan jämförda mot varandra och är funna att följa teoretiska förväntningar med avseende på vinkel-, gastryck- och pålagd elektrodspänningsberoende.Resultaten av projektet, som besvarar flera tidigare frågeställningar och bekräftar vissa antaganden, flyttar utsikten och förståelsen framåt för hur PPACs fungerar och vad forskarna kan uppnå med dem.

Microstructure changes in uranium and uranium/metal alloys due to radiation damage are of great interest in nuclear science and engineering. Titanium has attracted attention because of its similarity to Zr. It has been proposed for use in the second generation of fusion reactors due to its resistance to radiation-induced swelling. Aluminum can be regarded as a standard absorbing material or backing material for irradiation targets. Initial study of thin aluminum films irradiation by �������Cf fission fragments and alpha particles from source has been conducted in the Radiation Center, Oregon State University. Initial study of thin aluminum films irradiation by �������Cf fission fragments and alpha particles from source has been conducted in the Radiation Center, Oregon State University. Aluminum can be regarded as a standard absorbing material or backing material for irradiation targets. The AFM investigation of microstructure damages of thin aluminum surfaces revealed that the voids, dislocation loops and dislocation lines, formed in the thin aluminum films after bombardment by �������Cf fission fragments and alpha particles, depends on the irradiation dose. The void swelling and diameter and depth of voids increase linearly with the fluence of particles and dose; however, the areal density of voids decreased when formation of dislocation loops began. Study of deposition of uranium on titanium backing material by molecular plating and characterization of produced U/Ti film has been performed. The U/Ti film has smooth and uniform surfaces but the composition of the deposits is complex and does not include water molecules which probably involve the presence of U (VI). A possible structure for the deposits has been suggested. X-ray diffraction pattern of U/Ti films showed that The U/Ti film has an amorphous structure. Uranium films (0.500 mg/cm��) and stack of titanium foils (thickness 0.904 mg/cm��) were used to study the microstructural damage of the uranium film and its backing material. Irradiation of U/Ti film and Ti foils with 1 MeV/u (136 MeV) �������Xe�������� ions in was performed in the Positive Ion Injector (PII) unit at the Argonne Tandem Linear Accelerator System (ATLAS) Facility at Argonne National Laboratory, IL. Pre- and post- irradiation of samples was analyzed by X-ray diffraction, Scanning Electron Microscopy/Energy Dispersive Spectroscopy (SEM/EDS) and Atomic Force Microscopy (AFM). The irradiation of U/Ti films results in the formation of a crystalline U���O��� phase and polycrystalline Ti phase. Annealing of the thin uranium deposit on a titanium backing at 800��C in the air atmosphere condition for an hour produced a mixture of UO���, U���O���, Ti, TiO and TiO��� (rutile) phases; meanwhile, annealing at 800oC for an hour in the argon environment produced a mixture of ��-U���O���, Ti and TiO��� (rutile) phases. These phenomena indicate that the damage during irradiation was not due to foil heating. Microstructural damage of irradiated uranium film was dominated by void and bubble formation. The microstructure of irradiated titanium foils is characterized by hillocks, voids, polygonal ridge networks, dislocation lines and dislocation networks. Theory predicts that titanium undergoes an allotropic phase transformation at 882.5 ��C, changing from a closed-packed hexagonal crystal structure (��-phase) into a body-centered cubic crystal structure (��- phase). When the titanium foils were irradiated with 136MeV �������Xe�������� at beam intensity of 3 pnA corresponding to 966��C, it was expected that its structure can change from hexagonal-close packed (hcp) to body-centered cubic (bcc). However, in contrast to the theory, transformation from ��-Ti (hcp) phase to fcc-Ti phase was observed. This phenomenon indicates that during irradiation with high energy and elevated temperature, the fcc-Ti phase more stable than the hcp-Ti Phase. / Graduation date: 2012