Estimativa de risco devido à ingestão de isótopos de urânio em fontes de águas minerais

OBJETIVOS: Complementar dados de investigação anterior sobre o risco de indução de câncer devido à ingestão de 226Ra, 228Ra e 222Rn em fontes de águas minerais de uma região de altos níveis de radioatividade natural, do Brasil. Desta forma, foi realizada a estimativa de indução de câncer devido à ingestão de 238U e 234U nessas mesmas águas. MÉTODO: O coeficiente de risco para os isótopos naturais de urânio foi considerado como sendo o mesmo daquele utilizado para a indução de sarcoma ósseo pelo 226Ra e que a quantidade depositada no osso corresponde a 25 vezes a ingestão diária de 226Ra e a 11 vezes a ingestão diária dos isótopos de urânio de meia-vida longa. Amostras de água das fontes ultilizadas pela população de Água da Prata, Estado de São Paulo, foram coletadas, num período de um ano, de forma a abranger todas as estações. RESULTADOS: Foram encontradas concentrações variando de 2,0 a 28,4 mBq/L e de 4,7 a 143m Bq/L para 238U e 234U, respectivamente. Baseando-se nessas concentrações foi estimado o risco devido à ingestão dos isótopos de urânio: um total de 0,3 casos de câncer por 10(6) indivíduos expostos. Este dado indica que a ingestão crônica de urânio nas concentrações observadas nas fontes analisadas resultará em um acréscimo no número de casos de câncer fatais de 0,1 %. CONCLUSÕES: Se as incertezas na estimativa dos efeitos carcinogênicos forem levadas em consideração, pode-se concluir que praticamente nenhum caso de câncer ocorrerá devido à ingestão de urânio presente nas águas minerais analisadas.OBJETIVOS: Complementar dados de investigação anterior sobre o risco de indução de câncer devido à ingestão de 226Ra, 228Ra e 222Rn em fontes de águas minerais de uma região de altos níveis de radioatividade natural, do Brasil. Desta forma, foi realizada a estimativa de indução de câncer devido à ingestão de 238U e 234U nessas mesmas águas. MÉTODO: O coeficiente de risco para os isótopos naturais de urânio foi considerado como sendo o mesmo daquele utilizado para a indução de sarcoma ósseo pelo 226Ra e que a quantidade depositada no osso corresponde a 25 vezes a ingestão diária de 226Ra e a 11 vezes a ingestão diária dos isótopos de urânio de meia-vida longa. Amostras de água das fontes ultilizadas pela população de Água da Prata, Estado de São Paulo, foram coletadas, num período de um ano, de forma a abranger todas as estações. RESULTADOS: Foram encontradas concentrações variando de 2,0 a 28,4 mBq/L e de 4,7 a 143m Bq/L para 238U e 234U, respectivamente. Baseando-se nessas concentrações foi estimado o risco devido à ingestão dos isótopos de urânio: um total de 0,3 casos de câncer por 10(6) indivíduos expostos. Este dado indica que a ingestão crônica de urânio nas concentrações observadas nas fontes analisadas resultará em um acréscimo no número de casos de câncer fatais de 0,1 %. CONCLUSÕES: Se as incertezas na estimativa dos efeitos carcinogênicos forem levadas em consideração, pode-se concluir que praticamente nenhum caso de câncer ocorrerá devido à ingestão de urânio presente nas águas minerais analisadas

Análise da dicotomia sofrimento e prazer na função gerencial feminina

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Chemical and radiological characterization of meals served by the COSEAS (USP-SP)

O presente estudo apresenta resultados de análise química de refeições (almoço) oferecidas pelo restaurante do COSEAS (USP), por cinco dias não consecutivos. Essas refeições foram coletadas em triplicata, da mesma forma como oferecida para os usuários, sendo, a seguir, liofilizadas para as análises posteriores. No total, 15 amostras foram coletadas. A análise química de composição centesimal foi realizada segundo as técnicas padronizadas pela AOAC. O conteúdo de alguns elementos minerais (Ca, Fe, K, Na, Se e Zn) foi determinado por análise por ativação neutrônica instrumental. A validação da metodologia foi feita por meio da análise dos materiais de referência. A partir dos dados de concentração, calcularam-se os valores de ingestão de cada nutriente correspondente a esta refeição (40% da ingestão diária total), que foram avaliadas segundo as novas recomendações de nutrientes (Dietary Reference Intakes - DRIs) do National Research Council (USA), considerando a população de mulheres no estágio de vida de 19 a 30 anos. Comparando-se os valores médios encontrados com os valores recomendados, concluiu-se que: para os macronutrientes e os micronutrientes, Fe, Se e Zn, as recomendações foram atingidas; para Ca e K foram deficientes; e para Na excedeu o valor recomendado. Os radionuclídeos 40K, 60Co, 137Cs e 131I foram determinados, nas amostras de dieta, por espectrometria gama; 90Sr por cintilação em meio líquido; e 210Po, 234U, 232Th, 238U, 235U, 228Th, 230Th e 232Th por espectrometria alfa. Verificou-se, a partir dos resultados obtidos, que todos os radionuclídeos analisados se encontram muito abaixo dos limites estabelecidos pela FAO.This study presents the results obtained for the chemical and radiological analyses of lunch meals served in the cafeteria at the University of São Paulo-USP (COSEAS restaurant) in Brazil, on 5 non-consecutive days. On each of the five days, the meals were collected in triplicate and then freeze-dried for analysis totalizing 15 samples. The determination of the proximate composition complied with the AOAC standardized methodologies. The content of Ca, Fe, K, Na, Se, and Zn was determined by instrumental neutron activation analysis and the method validation was performed by certified reference materials analyses. Based on the concentration data, the daily intake of each mineral was calculated (corresponding to 40% of the total daily intake) and compared to the new recommendations set by the National Research Council (USA) considering the 19-30 year-old women range group. Comparing the average values obtained in this study with the recommended values, it was possible to verify that for macronutrients and the micronutrients Fe, Se, and Zn the recommendations were followed; for Ca and K they were deficient and exceeded the recommendation value for Na. The radionuclides 40K, 60Co, 137Cs, and 131I were determined by gamma spectrometry; 90Sr by liquid cintilation and 210Po, 234U, 232Th, 238U, 235U, 228Th, 230Th, and 232Th by alfa spectrometry. All radionuclides are present in concentrations below the limits set by the Food and Agriculture Organization (FAO)

Optimization and validation of a LC-HRMS method for aflatoxins determination in urine samples

Mycotoxins’ exposure by inhalation and/or dermal contact can occur in different branches of industry especially where heavily dusty settings are present and the handling of dusty commodities is performed. This study aims to explore the possible contribution of the occupational exposure to aflatoxins by analysing urine samples for the presence of aflatoxins B1 and M1 and aflatoxin B1-N7-guanine adduct. The study was conducted in 2017 on two groups of volunteers, the workers group, composed by personnel employed in an Italian feed plant (n = 32), and a control group (n = 29), composed by the administrative employees of the same feed plant; a total of 120 urine samples were collected and analysed. A screening method and a quantitative method with high-resolution mass spectrometry determination were developed and fully validated. Limits of detections were 0.8 and 1.5 pg/mLurine for aflatoxin B1 and M1, respectively. No quantitative determination was possible for the adduct aflatoxin B1-N7-guanine. Aflatoxin B1 and its adduct were not detected in the analysed samples, and aflatoxin M1, instead, was found in 14 samples (12%) within the range 1.9–10.5 pg/mLurine. Only one sample showed a value above the limit of quantification (10.5 pg/mLurine). The absence of a statistical difference between the mean values for workers and the control group which were compared suggests that in this specific setting, no professional exposure occurs. Furthermore, considering the very low level of aflatoxin M1 in the collected urine samples, the contribution from the diet to the overall exposure is to be considered negligible

Biomonitoring data for assessing aflatoxins and ochratoxin a exposure by italian feedstuffs workers

Mycotoxins exposure by inhalation and/or dermal contact is possible in different branches of industry especially where heavily dusty settings are present and the handling of dusty commodities is performed. This study aims to explore the validity of the biomonitoring as a tool to investigate the intake of mycotoxins in a population of workers operating in an Italian feed plant. Serum samples were collected for the determination of aflatoxins B1 (AFB1), AFB1-Lysine adduct and ochratoxin A (OTA). A method based on liquid-liquid extraction coupled with high resolution mass spectrometry determination was developed and fully validated. For AFB1, a high number of non-detected samples (90%) was found and no statistical difference was observed comparing workers and control group. None of the analyzed samples showed the presence of AFB1-Lysine adduct. For OTA, the 100% of the analyzed samples was positive with a 33% of the samples showing a concentration higher than the limit of quantification (LOQ), but no statistical difference was highlighted between the average levels of exposed and control groups. In conclusion, the presence of AFB1 and OTA in serum cannot be attributable to occupational exposure

Determination of Natural Radionuclides (Ra-226, Po-210, Ra-228 and K-40) and Cs-137 in Fish Consumed in the City of São Paulo

The aim of the study was to determine the activity concentration of the natural radionuclides (226Ra, 210Po, 228Ra and 40K) and artificial radionuclide 137Cs in the muscle of the marine fish species most consumed in the city of São Paulo and to evaluate the annual effective dose due to the consumption of the fish. Samples were collected in the supermarket chain Extra and Carrefour and in the distribution center CEAGESP. Six fish species were selected among the most available and consumed in São Paulo city: anchovy, tuna, dogfish, croaker, hake and sardine. After the sample preparation procedures, the determination of 226Ra, 228Ra, 40K and 137Cs was carried out by gamma spectrometry and the determination of 210Po by alpha spectrometry. The results obtained for all the species studied are below the limits adopted by the Brazilian Standards for 137Cs and, therefore, their consumption offers no risk due to the ingestion of this radionuclide. The concentration obtained for the radionuclides 226Ra, 210Po, 228Ra and 137Cs in the fish samples analized are low and of the same order of magnitude as data from literature. The results obtained for the doses, for all the species studied, showed that their consumption offers no risk of exposure due to the ingestion of the analyzed radionuclides

Production of He-4 and (4) in Pb-Pb collisions at root(NN)-N-S=2.76 TeV at the LHC

Results on the production of He-4 and (4) nuclei in Pb-Pb collisions at root(NN)-N-S = 2.76 TeV in the rapidity range vertical bar y vertical bar <1, using the ALICE detector, are presented in this paper. The rapidity densities corresponding to 0-10% central events are found to be dN/dy4(He) = (0.8 +/- 0.4 (stat) +/- 0.3 (syst)) x 10(-6) and dN/dy4 = (1.1 +/- 0.4 (stat) +/- 0.2 (syst)) x 10(-6), respectively. This is in agreement with the statistical thermal model expectation assuming the same chemical freeze-out temperature (T-chem = 156 MeV) as for light hadrons. The measured ratio of (4)/He-4 is 1.4 +/- 0.8 (stat) +/- 0.5 (syst). (C) 2018 Published by Elsevier B.V.Peer reviewe

Mechanisms of star formation quenching in local galaxies

Les données astronomiques deviennent de plus en plus précises et permettent d’affiner notre compréhension des processus qui régissent l’évolution des galaxies, mais nous ne disposons toujours pas d’un paradigme global pour expliquer certains mécanismes physiques. En particulier, le déclenchement et la régulation de l’extinction de la formation stellaire ne sont pas compris en détail étant donné les nombreux processus dont elle peut résulter et les différentes échelles de temps qui sont impliquées.Le but de ce projet de thèse est d’étudier le contenu en gaz, l’activité de formation d’étoiles et l’extinction des étoiles dans les galaxies en utilisant les données spectroscopiques du relevé SDSS-IV MaNGA, ainsi que des observations de gaz moléculaire et atomique.Tout d’abord, je décris l’échantillon de galaxies proches sur lequel j’ai décidé de me concentrer. Il s’agit de 29 galaxies proches qui présentent des caractéristiques cinématiques complexes dans leurs spectres dans le domaine visible. Dans la deuxième partie, je présente une analyse de cet échantillon en termes de paramètres structurels des galaxies et d’activité de formation d’étoiles. Je conclus que ces objets nous permettent d’échantillonner différentes phases de l’évolution des galaxies, qui résultent d’événements de fusions mineures. Dans la troisième partie, je détaille les résultats que j’ai obtenus en appliquant une procédure d’ajustement de spectres innovante aux données d’une galaxie MaNGA particulière. Cette approche permet de mettre en évidence une fusion mineure en décomposant les caractéristiques spectrales optiques, à la fois dans les raies d’émission du gaz et dans le continuum stellaire. Dans la quatrième partie, je me concentre sur l’analyse du contenu en gaz froid à travers des observations de gaz moléculaire et atomique. Je déduis les masses de gaz moléculaire ainsi qu’une relation de Kennicutt-Schmidt afin d’estimer l’efficacité de la formation d’étoiles des galaxies étudiées.Astronomical data become more and more precise and help the refining of our understanding of the processes that drive galaxy evolution, but we still do not have a global paradigm to explain some physical mechanisms. Especially, the triggering and regulation of star formation quenching are not understood in detail given the numerous processes that it can be resulting from and the different timescales that are involved.The aim of this thesis project is to study the gas content, star formation activity and quenching within galaxies using integral field spectroscopic data from the SDSS-IV MaNGA survey, as well as single-dish observations of molecular and atomic gas.Firsly, I describe the sample of nearby galaxies that I decided to focus on. It consists of 29 nearby galaxies that show complex kinematic features in their optical spectra. It is drawn from the cross-identification between the MaNGA data release DR15 and a catalogue comprising massive, isolated, bulge-dominated galaxies exhibiting a central excess of star formation.In the second part, I present an analysis of this sample in terms of galaxy structural parameters and star formation activity. I conclude that these objects enable us to sample different phases of galaxy evolution, that result from minor-merger events.In the third part, I detail the results that I obtained by applying an innovative fitting procedure to the data from one peculiar MaNGA galaxy. This approach helps reveal a minor-merger event by disentangling the optical spectral features, both in gas and stellar components.In the fourth part, I focus on the analysis of the cold gas content through molecular and atomic gas observations. I infer the molecular and atomic gas masses as well as a Kennicutt-Schmidt relation so as to estimate the star formation efficiency of the studied galaxies