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9 results on '"RADIAÇÃO DE FUNDO"'

1. Radiação natural e células tronco de tumores mamários em população residente no município de Poços de Caldas-MG

Author

Merola, Yula Lima, 1971, Schenka, André Almeida, 1976, Castilho, Roger Frigério, Granjeiro, Paulo Afonso, Otero, Ubirani Barros, Matos, Patricia Sabino de, Universidade Estadual de Campinas. Faculdade de Ciências Médicas, Programa de Pós-Graduação em Fisiopatologia Médica, and UNIVERSIDADE ESTADUAL DE CAMPINAS

Subjects
Radônio, Radon, Neoplastic stem cells, Background radiation, Células-tronco neoplásicas, Neoplasias da mama, Radiação de fundo, Breast neoplasms
Abstract

Orientador: Andre Almeida Schenka Tese (doutorado) - Universidade Estadual de Campinas, Faculdade de Ciências Médicas Resumo: Introdução: O câncer de mama é uma doença multifatorial pela combinação de fatores genéticos e ambientai. Recentemente estudos sugeriram que haveria subpopulações de células neoplásicas no câncer de mama, as células tronco tumorais (CTTs) que estariam associadas com o desenvolvimento tumoral, resistência as drogas, recorrências e metástase. Diversos fatores ambientais estão relacionados ao aumento do risco de desenvolver a doença, entre eles a exposição à radiação ionizante. Uma possível associação entre a exposição à radiação natural e efeitos a saúde, principalmente incidência e mortalidade por câncer, tem sido investigadas em várias regiões de radioatividade natural A radiação ionizante pode ser origem em natural e artificial. A radiação ionizante natural está presente no mundo e todas as pessoas estão expostas a uma exposição crônica de baixas doses ao longo da vida. Objetivo: O estudo teve como objetivo avaliar a radiação natural e células-tronco de tumores mamários no município de Poços de Caldas-MG. O Planalto Poços de Caldas é mundialmente conhecido pela sua radioatividade elevada e a ocorrência de minério nuclear.Material e Métodos: Dados clínicos-patológicos foram obtidos de 35 casos de câncer de mama no período de 2003 a 2011. Foram testados em cortes de TMA,obtidos a partir dos blocos de parafina originais contendo os tumores mamários, os seguintes anticorpos: CD34, SOX-2, Oct 3/4, p63, CD24, CD44, CD133 e ESA/EPCAM e medições de radiação gama terrestre e radônio foram quantificadas. Resultados: A maioria das pacientes tinha mais de 50 anos (94,28%) e histórico familiar de câncer de mama (28,57%). Apenas 28,57% declararam o uso de terapia de reposição hormonal, enquanto 40% confirmaram ter usado contraceptivos orais. Os marcadores de células tronco tumorais foram detectados em menos de 30% das amostras e em níveis baixos, sendo os marcadores mais frequentes o CD44+/CD24- (40%) e ALDH-1 (25,71%). Em relação a radiação gama terrestre a média foi de 0,91mSv/ano, acima do valor de referência da UNSCEAR de 0,5mSv/ano e a média geométrica da concentração do radônio foi de 50 Bq/m3 abaixo do valor de referência da OMS de 100 Bq/m3. Ao contrário da hipótese inicial, a frequência de células positivas de ALDH-1 e CD44+/CD24- e o número de CTTs foram associados negativamente com a radiação gama terrestre (coeficiente de Rho de Spearman de -0,405 e -0,393, respectivamente p

Published
2021
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2. DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM

Author

Muir, J., Baxter, E., Miranda, V, Doux, C., Ferte, A., Leonard, C. D., Huterer, D., Jain, B., Lemos, P., Raveri, M., Nadathur, S., Campos, A. [UNESP], Chen, A., Dodelson, S., Elvin-Poole, J., Lee, S., Secco, L. F., Troxel, M. A., Weaverdyck, N., Zuntz, J., Brout, D., Choi, A., Crocce, M., Davis, T. M., Gruen, D., Krause, E., Lidman, C., MacCrann, N., Moller, A., Prat, J., Ross, A. J., Sako, M., Samuroff, S., Sanchez, C., Scolnic, D., Zhang, B., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bertin, E., Bhargava, S., Bridle, S. L., Brooks, D., Burke, D. L., Carnero Rosell, A., Kind, M. Carrasco, Carretero, J., Cawthon, R., Costanzi, M., Costa, L. N. da, Pereira, M. E. S., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Estrada, J., Everett, S., Evrard, A. E., Ferrero, I, Flaugher, B., Frieman, J., Garcia-Bellido, J., Giannantonio, T., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., Menanteau, F., Miquel, R., Morgan, R., Myles, J., Palmese, A., Paz-Chinchon, F., Plazas, A. A., Romer, A. K., Roodman, A., Sanchez, E., Scarpine, V, Serrano, S., Sevilla-Noarbe, I, Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Tucker, D. L., Varga, T. N., Weller, J., Wilkinson, R. D., DES Collaboration, Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), DES, National Science Foundation (US), Ministerio de Ciencia, Innovación y Universidades (España), European Commission, Generalitat de Catalunya, Instituto Nacional de Ciência e Tecnologia (Brasil), Stanford University, University of Hawaii, University of Arizona, University of Pennsylvania, California Institute of Technology, Newcastle University, University of Michigan, University College London, University of Chicago, University of Portsmouth, Carnegie Mellon University, Universidade Estadual Paulista (UNESP), Ohio State University, Duke University, University of Edinburgh, Harvard and Smithsonian, Institut d'Estudis Espacials de Catalunya (IEEC), Institute of Space Sciences (ICE-CSIC, University of Queensland, 382 Via Pueblo Mall, SLAC National Accelerator Laboratory, Australian National University, LPC, NSF's National Optical-Infrared Astronomy Research Laboratory, Universidade de São Paulo (USP), Laboratório Interinstitucional de E-Astronomia-LIneA, Fermi National Accelerator Laboratory, Universidad Autonoma de Madrid, Institut d'Astrophysique de Paris, University of Sussex, University of Manchester, Instituto de Astrofisica de Canarias, Universidad de la Laguna, University of Illinois at Urbana-Champaign, National Center for Supercomputing Applications, Barcelona Institute of Science and Technology, University of Wisconsin-Madison, INAF-Osservatorio Astronomico di Trieste, Institute for Fundamental Physics of the Universe, Observatório Nacional, IIT Hyderabad, Ludwig-Maximilians-Universität, Santa Cruz Institute for Particle Physics, University of Oslo, University of Cambridge, Max Planck Institute for Extraterrestrial Physics, Ludwig-Maximilians Universität München, Center for Astrophysics | Harvard and Smithsonian, Macquarie University, Lowell Observatory, Institució Catalana de Recerca i Estudis Avançats, Peyton Hall, Medioambientales y Tecnológicas (CIEMAT), University of Southampton, Oak Ridge National Laboratory, Stanford Univ, Univ Hawaii, Univ Arizona, Univ Penn, CALTECH, Newcastle Univ, Univ Michigan, UCL, Univ Chicago, Univ Portsmouth, Carnegie Mellon Univ, Universidade Estadual Paulista (Unesp), Ohio State Univ, Duke Univ, Univ Edinburgh, Harvard & Smithsonian, Inst Estudis Espacials Catalunya IEEC, CSIC, Univ Queensland, SLAC Natl Accelerator Lab, Australian Natl Univ, Univ Clermont Auvergne, Cerro Tololo Interamer Observ, Lab Interinst E Astron LIneA, Fermilab Natl Accelerator Lab, Univ Autonoma Madrid, Inst Astrophys Paris, Sorbonne Univ, Univ Sussex, Univ Manchester, Inst Astrofis Canarias, Univ La Laguna, Univ Illinois, Natl Ctr Supercomp Applicat, Barcelona Inst Sci & Technol, Univ Wisconsin, INAF Osservatorio Astron Trieste, Inst Fundamental Phys Universe, Observ Nacl, Ludwig Maximilians Univ Munchen, Santa Cruz Inst Particle Phys, Univ Oslo, Univ Cambridge, Max Planck Inst Extraterr Phys, Macquarie Univ, Lowell Observ, Inst Catalana Recerca & Estudis Avancats, Princeton Univ, Ctr Invest Energet Medioambientales & Tecnol CIEM, Univ Southampton, Oak Ridge Natl Lab, UAM. Departamento de Física Teórica, Muir, J., Baxter, E., Miranda, V., Doux, C., Ferte, A., Leonard, C. D., Huterer, D., Jain, B., Lemos, P., Raveri, M., Nadathur, S., Campos, A., Chen, A., Dodelson, S., Elvin-Poole, J., Lee, S., Secco, L. F., Troxel, M. A., Weaverdyck, N., Zuntz, J., Brout, D., Choi, A., Crocce, M., Davis, T. M., Gruen, D., Krause, E., Lidman, C., Maccrann, N., Moller, A., Prat, J., Ross, A. J., Sako, M., Samuroff, S., Sanchez, C., Scolnic, D., Zhang, B., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bertin, E., Bhargava, S., Bridle, S. L., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cawthon, R., Costanzi, M., Da Costa, L. N., Pereira, M. E. S., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Estrada, J., Everett, S., Evrard, A. E., Ferrero, I., Flaugher, B., Frieman, J., Garcia-Bellido, J., Giannantonio, T., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., Menanteau, F., Miquel, R., Morgan, R., Myles, J., Palmese, A., Paz-Chinchon, F., Plazas, A. A., Romer, A. K., Roodman, A., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Tucker, D. L., Varga, T. N., Weller, J., and Wilkinson, R. D.

Subjects
General relativity, Cosmological parameters, Geometry, Astrophysics::Cosmology and Extragalactic Astrophysics, Lambda, Sky surveys, 01 natural sciences, Omega, Evolution of the Universe, Cosmology, Cosmic microwave background, Cosmologial constant, symbols.namesake, 0103 physical sciences, Dark energy, RADIAÇÃO DE FUNDO, Astrophysical studies of gravity, Weak, Large-scale structure of the Universe, Planck, 010306 general physics, Weak gravitational lensing, Gravitational Lensing, Physics, 010308 nuclear & particles physics, Física, symbols, Neutrino, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Muir, J., et al. (DES Collaboration), We analyze Dark Energy Survey (DES) data to constrain a cosmological model where a subset of parameters - focusing on ωm - are split into versions associated with structure growth (e.g., ωmgrow) and expansion history (e.g., ωmgeo). Once the parameters have been specified for the ΛCDM cosmological model, which includes general relativity as a theory of gravity, it uniquely predicts the evolution of both geometry (distances) and the growth of structure over cosmic time. Any inconsistency between measurements of geometry and growth could therefore indicate a breakdown of that model. Our growth-geometry split approach therefore serves both as a (largely) model-independent test for beyond-ΛCDM physics, and as a means to characterize how DES observables provide cosmological information. We analyze the same multiprobe DES data as [Phys. Rev. Lett. 122, 171301 (2019)PRLTAO0031-900710.1103/PhysRevLett.122.171301]: DES Year 1 (Y1) galaxy clustering and weak lensing, which are sensitive to both growth and geometry, as well as Y1 BAO and Y3 supernovae, which probe geometry. We additionally include external geometric information from BOSS DR12 BAO and a compressed Planck 2015 likelihood, and external growth information from BOSS DR12 RSD. We find no significant disagreement with ωmgrow=ωmgeo. When DES and external data are analyzed separately, degeneracies with neutrino mass and intrinsic alignments limit our ability to measure ωmgrow, but combining DES with external data allows us to constrain both growth and geometric quantities. We also consider a parametrization where we split both ωm and w, but find that even our most constraining data combination is unable to separately constrain ωmgrow and wgrow. Relative to ΛCDM, splitting growth and geometry weakens bounds on σ8 but does not alter constraints on h., The DES data management system is supported by the National Science Foundation under Grants No. AST-1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under Grants No. ESP2017-89838, No. PGC2018-094773, No. PGC2018-102021, No. SEV-2016-0588, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds from the European Union. I. F. A. E. is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC grant agreements No. 240672, No. 291329, and No. 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq Grant No. 465376/2014-2).

Published
2021
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3. Aplicação de uma metodologia de screening para avaliar a mortalidade por câncer em municípios selecionados do Estado de Minas Gerais, Brasil Screening methodology application to evaluate cancer mortality in selected cities in the State of Minas Gerais, Brazil

Author

Ubirani B. Otero, Berenice N. Antoniazzi, Lene H. S. Veiga, Silvana R. Turci, and Gulnar Azevedo e Silva Mendonça

Subjects
Coeficiente de Mortalidade, Neoplasias, Radiação de Fundo, Mortality Rate, Neoplasms, Background Radiation, Medicine, Public aspects of medicine, RA1-1270
Abstract

Iniciou-se uma investigação epidemiológica em municípios do sul de Minas Gerais, Brasil, considerando a possibilidade de aumento na incidência de câncer devido a maior exposição à radiação natural em alguns deles. Buscou-se, preliminarmente, conhecer o padrão de mortalidade por câncer, avaliar se existe excesso de óbitos e discutir os possíveis fatores de risco associados a esse aumento. Propõe-se uma metodologia de screening com base na razão de mortalidade padronizada (RMP) para classificar os municípios prioritários em estudos futuros. Os municípios considerados de altíssima prioridade para investigação foram: Andradas - câncer de pulmão em homens [RMP = 208 (106-310)] e fígado em mulheres [RMP = 403 (104-701)]; Poços de Caldas - leucemia em homens e mulheres (RMP = 284 (156-412) e RMP = 211 (111-312), respectivamente); Pouso Alegre - leucemia em homens [RMP = 333 (127-540)] e cânceres hematológicos em mulheres [RMP = 257 (188-396)].Estudos epidemiológicos devem ser conduzidos para avaliar a contribuição da radiação e outros fatores de riscos relacionados ao câncer e assim subsidiar futuras medidas de prevenção e controle.An epidemiological investigation was launched in several cities in southern Minas Gerais State, Brazil, considering the possibility of increased cancer incidence due to high exposure to natural radiation. First, the cancer mortality patterns were assessed to determine whether there was an increase in cancer deaths and to discuss the possible risk factors related to such an increase. The study proposed the use of a screening methodology based on standardized mortality ratio (SMR) in order to classify priority areas for future studies. Cities considered high priority for further investigation were: Andradas, for lung cancer in men (SMR = 208 (106-310)) and liver cancer in women (SMR = 403 (104-701)); Poços de Caldas, leukemia in men and women (SMR = 284 (156-412)) and SMR = 211 (111-312), respectively); Pouso Alegre, leukemia in men (SMR = 333 (127-540)) and hematological cancers in women (SMR = 257 (188-396)). Epidemiological studies are necessary to evaluate the role of radiation and other risk factors in these cancers and thus to support future preventive and control measures.

Published
2007
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4. Aplicação de uma metodologia de screening para avaliar a mortalidade por câncer em municípios selecionados do Estado de Minas Gerais, Brasil.

Author

Otero, Ubirani B., Antoniazzi, Berenice N., Veiga, Lene H. S., Turci, Silvana R., and e Silva Mendonça, Gulnar Azevedo

Abstract

Copyright of Cadernos de Saude Publica is the property of Escola Nacional de Saude Publica Sergio Arouca and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)

Published
2007
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5. Planck 2018 results: I. Overview and the cosmological legacy of Planck

Author

Planck Collaboration, Aghanim, N., Akrami, Y., Arroja, F., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Battye, R., Benabed, K., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bock, J. J., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bucher, M., BURIGANA, CARLO, Butler, R. C., Calabrese, E., Cardoso, J. -F., Carron, J., Casaponsa, B., Challinor, A., Chiang, H. C., Colombo, L. P. L., Combet, C., Contreras, D., Crill, B. P., CUTTAIA, FRANCESCO, de Bernardis, P., de Zotti, G., Delabrouille, J., Delouis, J. -M., Désert, F. -X., Di Valentino, E., Dickinson, C., Diego, J. M., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Falgarone, E., Fantaye, Y., Fergusson, J., Fernandez-Cobos, R., FINELLI, FABIO, Forastieri, F., FRAILIS, Marco, FRANCESCHI, ENRICO, Frolov, A., GALEOTTA, Samuele, Galli, S., Ganga, K., Génova-Santos, R. T., Gerbino, M., Ghosh, T., González-Nuevo, J., Górski, K. M., Gratton, S., GRUPPUSO, ALESSANDRO, Gudmundsson, J. E., Hamann, J., Handley, W., Hansen, F. K., Helou, G., Herranz, D., Hildebrandt, S. R., Hivon, E., Huang, Z., Jaffe, A. H., Jones, W. C., Karakci, A., Keihänen, E., Keskitalo, R., Kiiveri, K., Kim, J., Kisner, T. S., Knox, L., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Langer, M., Lasenby, A., LATTANZI, Mario Gilberto, Lawrence, C. R., Le Jeune, M., Leahy, J. P., Lesgourgues, J., Levrier, F., Lewis, A., Liguori, M., Lilje, P. B., Lilley, M., Lindholm, V., López-Caniego, M., Lubin, P. M., Ma, Y. -Z., Macías-Pérez, J. F., MAGGIO, Gianmarco, Maino, D., Mandolesi, N., Mangilli, A., Marcos-Caballero, A., MARIS, Michele, Martin, P. G., Martinelli, M., Martínez-González, E., Matarrese, S., Mauri, N., McEwen, J. D., Meerburg, P. D., Meinhold, P. R., Melchiorri, A., Mennella, A., Migliaccio, M., Millea, M., Mitra, S., Miville-Deschênes, M. -A., Molinari, D., Moneti, A., Montier, L., MORGANTE, GIANLUCA, Moss, A., Mottet, S., Münchmeyer, M., Natoli, P., Nørgaard-Nielsen, H. U., Oxborrow, C. A., Pagano, L., PAOLETTI, DANIELA, Partridge, B., Patanchon, G., Pearson, T. J., Peel, M., Peiris, H. V., PERROTTA, Francesca, Pettorino, V., Piacentini, F., Polastri, L., Polenta, G., Puget, J. -L., Rachen, J. P., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Rocha, G., Rosset, C., Roudier, G., Rubiño-Martín, J. A., Ruiz-Granados, B., SALVATI, LAURA, SANDRI, MAURA, Savelainen, M., Scott, D., Shellard, E. P. S., Shiraishi, M., Sirignano, C., Sirri, G., Spencer, L. D., Sunyaev, R., Suur-Uski, A. -S., Tauber, J. A., TAVAGNACCO , DANIELE, Tenti, M., TERENZI, LUCA, Toffolatti, L., Tomasi, M., Trombetti, T., Valiviita, J., Van Tent, B., Vibert, L., Vielva, P., VILLA, FABRIZIO, Vittorio, N., Wandelt, B. D., Wehus, I. K., White, M., White, S. D. M., ZACCHEI, Andrea, Zonca, A., Universidad de Cantabria, Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA (UMR_8112)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Institut Lagrange de Paris, Sorbonne Universités, Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire de Physique Théorique d'Orsay [Orsay] (LPT), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Planck, Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS), Sorbonne Université (SU)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2020-....] (UGA [2020-....])-Institut polytechnique de Grenoble - Grenoble Institute of Technology [2020-....] (Grenoble INP [2020-....]), Université Grenoble Alpes [2020-....] (UGA [2020-....]), Institut de Planétologie et d'Astrophysique de Grenoble [2020-....] (IPAG [2020-....]), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble [2020-....] (OSUG [2020-....]), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes [2020-....] (UGA [2020-....])-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes [2020-....] (UGA [2020-....]), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Astrophysique, Laboratoire de physique de l'ENS - ENS Paris (LPENS), Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Sorbonne Université (SU)-École normale supérieure - 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Galilei', Universita degli Studi di Padova, University of Cambridge [UK] (CAM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), University College of London [London] (UCL), University of Manchester [Manchester], Venetian Institute Molecular Medicine (VIMM), University of British Columbia (UBC), Laboratoire de neurobiologie cellulaire et moléculaire (NBCM), Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), USDA-ARS : Agricultural Research Service, Planck Collaboration, Department of Physics, Helsinki Institute of Physics, European Commission, Ministerio de Ciencia e Innovación (España), Consejo Superior de Investigaciones Científicas (España), European Research Council, European Space Agency, Aghanim N., Akrami Y., Arroja F., Ashdown M., Aumont J., Baccigalupi C., Ballardini M., Banday A.J., Barreiro R.B., Bartolo N., Basak S., Battye R., Benabed K., Bernard J.-P., Bersanelli M., Bielewicz P., Bock J.J., Bond J.R., Borrill J., Bouchet F.R., Boulanger F., Bucher M., Burigana C., Butler R.C., Calabrese E., Cardoso J.-F., Carron J., Casaponsa B., Challinor A., Chiang H.C., Colombo L.P.L., Combet C., Contreras D., Crill B.P., Cuttaia F., De Bernardis P., De Zotti G., Delabrouille J., Delouis J.-M., Desert F.-X., Di Valentino E., Dickinson C., Diego J.M., Donzelli S., Dore O., Douspis M., Ducout A., Dupac X., Efstathiou G., Elsner F., Ensslin T.A., Eriksen H.K., Falgarone E., Fantaye Y., Fergusson J., Fernandez-Cobos R., Finelli F., Forastieri F., Frailis M., Franceschi E., Frolov A., Galeotta S., Galli S., Ganga K., Genova-Santos R.T., Gerbino M., Ghosh T., Gonzalez-Nuevo J., Gorski K.M., Gratton S., Gruppuso A., Gudmundsson J.E., Hamann J., Handley W., Hansen F.K., Helou G., Herranz D., Hildebrandt S.R., Hivon E., Huang Z., Jaffe A.H., Jones W.C., Karakci A., Keihanen E., Keskitalo R., Kiiveri K., Kim J., Kisner T.S., Knox L., Krachmalnicoff N., Kunz M., Kurki-Suonio H., Lagache G., Lamarre J.-M., Langer M., Lasenby A., Lattanzi M., Lawrence C.R., Le Jeune M., Leahy J.P., Lesgourgues J., Levrier F., Lewis A., Liguori M., Lilje P.B., Lilley M., Lindholm V., Lopez-Caniego M., Lubin P.M., Ma Y.-Z., Macias-Perez J.F., Maggio G., Maino D., Mandolesi N., Mangilli A., Marcos-Caballero A., Maris M., Martin P.G., Martinelli M., Martinez-Gonzalez E., Matarrese S., Mauri N., McEwen J.D., Meerburg P.D., Meinhold P.R., Melchiorri A., Mennella A., Migliaccio M., Millea M., Mitra S., Miville-Deschenes M.-A., Molinari D., Moneti A., Montier L., Morgante G., Moss A., Mottet S., Munchmeyer M., Natoli P., Norgaard-Nielsen H.U., Oxborrow C.A., Pagano L., Paoletti D., Partridge B., Patanchon G., Pearson T.J., Peel M., Peiris H.V., Perrotta F., Pettorino V., Piacentini F., Polastri L., Polenta G., Puget J.-L., Rachen J.P., Reinecke M., Remazeilles M., Renault C., Renzi A., Rocha G., Rosset C., Roudier G., Rubino-Martin J.A., Ruiz-Granados B., Salvati L., Sandri M., Savelainen M., Scott D., Shellard E.P.S., Shiraishi M., Sirignano C., Sirri G., Spencer L.D., Sunyaev R., Suur-Uski A.-S., Tauber J.A., Tavagnacco D., Tenti M., Terenzi L., Toffolatti L., Tomasi M., Trombetti T., Valiviita J., Van Tent B., Vibert L., Vielva P., Villa F., Vittorio N., Wandelt B.D., Wehus I.K., White M., White S.D.M., Zacchei A., Zonca A., Van Swinderen Institute for Particle Physics and G, High-Energy Frontier, Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Département de Physique de l'ENS-PSL, École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Département de Physique de l'ENS-PSL, Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - 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CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Università degli Studi di Padova = University of Padua (Unipd), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique de l'ENS - ENS Paris (LPENS (UMR_8023)), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Challinor, Anthony [0000-0003-3479-7823], Fergusson, James [0000-0003-4820-171X], Handley, William [0000-0002-5866-0445], Lasenby, Anthony [0000-0002-8208-6332], and Apollo - University of Cambridge Repository

Subjects
Cosmic background radiation, Cosmology: observations, Cosmology: theory, Surveys, cosmological model, Cosmic background radiation, Cosmology: observations, Cosmology: theory, Surveys, Astronomy, Cosmic microwave background, cosmic background radiation: polarization, Astrophysics, 01 natural sciences, 7. Clean energy, Cosmology: observation, redshift: low, RADIAÇÃO DE FUNDO, LENSING TOMOGRAPHY, observations [Cosmology], 010303 astronomy & astrophysics, media_common, Physics, Polarization (waves), MULTIBAND IMAGING PHOTOMETER, symbols, astro-ph.CO, power spectrum: angular dependence, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics and Astronomy, Structure formation, Cosmology and Nongalactic Astrophysics (astro-ph.CO), COMPONENT SEPARATION, satellite: Planck, ANGULAR POWER SPECTRUM, PARAMETER CONSTRAINTS, media_common.quotation_subject, FOS: Physical sciences, Lambda-CDM model, MAIN GALAXY SAMPLE, Astrophysics::Cosmology and Extragalactic Astrophysics, Radio spectrum, microwaves, NO, symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, theory [Cosmology], 0103 physical sciences, detector: pixel, Planck, 010308 nuclear & particles physics, Astronomy and Astrophysics, 115 Astronomy, Space science, Redshift, cosmic background radiation: temperature, Space and Planetary Science, Sky, PROBE WMAP OBSERVATIONS, DARK ENERGY, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], MICROWAVE BACKGROUND POLARIZATION, BARYON ACOUSTIC-OSCILLATIONS
Abstract

Planck Collaboration: et al., arXiv:1807.06205v2, The European Space Agency’s Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857 GHz. This paper presents the cosmological legacy of Planck, which currently provides our strongest constraints on the parameters of the standard cosmological model and some of the tightest limits available on deviations from that model. The 6-parameter ΛCDM model continues to provide an excellent fit to the cosmic microwave background data at high and low redshift, describing the cosmological information in over a billion map pixels with just six parameters. With 18 peaks in the temperature and polarization angular power spectra constrained well, Planck measures five of the six parameters to better than 1% (simultaneously), with the best-determined parameter (θ*) now known to 0.03%. We describe the multi-component sky as seen by Planck, the success of the ΛCDM model, and the connection to lower-redshift probes of structure formation. We also give a comprehensive summary of the major changes introduced in this 2018 release. The Planck data, alone and in combination with other probes, provide stringent constraints on our models of the early Universe and the large-scale structure within which all astrophysical objects form and evolve. We discuss some lessons learned from the Planck mission, and highlight areas ripe for further experimental advances., The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA, and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU).

Published
2020
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6. Avaliação da concentração de radônio-222 no ar de postos de trabalho de Curitiba/PR

Author

Del Claro, Flávia and Paschuk, Sergei Anatolyevich

Subjects
Materiais de construção - Contaminação, Ambiente de trabalho - Curitiba (PR), Soils - Contamination, Radiação ionizante - Efeito fisiológico, Radiation dosimetry, Building materials - Contamination, Radon, Ionizing radiation - Physiological effect, Radiation, Background, Radiação - Dosimetria, Solos - Contaminação, Radiação de fundo, Work environment - Curitiba (PR)
Abstract

Comissão Nacional de Energia Nuclear (CNEN) O ser humano está exposto diariamente a várias fontes de radiação natural sendo que a principal delas é o gás nobre 222Rn, pertencente à cadeia radioativa do 238U. A grande importância do estudo do 222Rn se deve ao fato do mesmo ser responsável, juntamente com seus produtos de decaimento, por cerca da metade da dose efetiva proveniente das fontes de radiações ionizantes naturais que é recebida pela população mundial. Além disso, o gás 222Rn ao ser inalado produz isótopos que passam por oito decaimentos radioativos (metade por emissão de partículas alfa e metade por emissão de partículas beta) para chegar ao isótopo estável de chumbo. Essa radiação interage com as células dos tecidos biológicos apresentando alta probabilidade de induzir o desenvolvimento de tumores pulmonares. O objetivo desta dissertação é avaliar os valores de concentração de 222Rn em ambientes de trabalho da região de Curitiba – Paraná, assim como, mensurar os níveis de 222Rn provenientes do solo e de materiais de construção que permeiam os postos de trabalho avaliados. Para o estudo dos níveis de 222Rn indoor foram utilizados detectores de estado sólido CR-39, submetidos à revelação química e leitura manual em microscópio óptico. Os cálculos das concentrações de 222Rn nos postos de trabalho foram obtidos a partir de metodologia de calibração desenvolvida pelo Centro de Desenvolvimento da Tecnologia Nuclear (CDTN) em conjunto com o Laboratório de Radiações Ionizantes da Universidade Tecnológica Federal do Paraná (UTFPR). O detector ativo AlphaGUARD (SaphymoGmbH) foi utilizado para análise das concentrações médias de 222Rn do solo e dos materiais de construção que também foram submetidos ao método de espectrometria gama para avaliação qualitativa e quantitativa dos radionuclídeos presentes nas amostras de areia, argamassa, brita azul, brita vermelha, concreto e tijolo vermelho. A metodologia utilizada para as medidas de solo permitiu encontrar as concentrações médias de 222Rn (radônio) e 220Rn (torônio) presentes no solo. Os resultados das concentrações médias de 222Rn obtidos nas medidas indoor dos postos de trabalho encontram-se entre 36 ± 49 Bq/m³ e 164 ± 51 Bq/m³. Valores esses considerados dentro do limite de referência de 200 Bq/m³ estabelecido por agências internacionais como United Nations Scientific Committee on the Effects of Atomic Radiation (UNSCEAR) e o International Commission on Radiological Protection (ICRP), mas um pouco acima do limite de 148 Bq/m³ preconizado pela United States Environmental Protection Agency (EPA). Em relação aos materiais de construção, os valores de concentração de 222Rn encontrados estão em uma faixa de 427 ± 310 Bq/m³ a 2053 ± 700 Bq/m³. As concentrações de 222Rn no solo variaram de 31 ± 2 kBq/m³ a 35 ± 4 kBq/m³ e os valores médios encontrados de 220Rn estão em um intervalo de 41 ± 6 kBq/m³ e 25 ± 11 kBq/m³, os quais constatam que as concentrações do gás radônio do solo estão abaixo do critério sueco que determina que valores inferiores a 50 kBq/m³ não caracterizam uma situação de alto risco. In every day life people are exposed to various types of radiation arising from different artificial and natural sources and among all of them the main role belongs to the isotope of noble gas 222Rn that makes part of the 238U radioactive chain. The isotope 222Rn is responsible for approximately half of the effective annual dose received by the world population. Being inhaled, the radon isotopes have to undergo 8 radioactive decay events (one half by emitting alpha particles and another half by emitting betas) to get to a stable isotope of lead. This radiation interacting with the cells of biological tissue have very high probability to induce the lung cancer. The goal of present research is to evaluate the activity concentration of 222Rn in the air of workplaces at Curitiba – Paraná State. Simultaneously there were performed the measurements of 222Rn emanation from soil and building materials occurred at evaluated workplaces. Indoor measurements of 222Rn activity were performed using Polycarbonate track etched detectors CR-39 that after the exposition in air were submitted to chemical etching and manual reading using the optical microscope.The calculations of the activity concentration of 222Rn in the air of workplaces were completed using the results of calibration performed by the Center of Nuclear Technology Development (CDTN) in cooperation with the Laboratory of Applied Nuclear Physics of the Federal University of Technology - Paraná (UTFPR).The instant radon detector AlphaGUARD (Saphymo GmbH) was used in the measurements of the average concentrations of 222Rn in soil gas and building materials. Building materials were also submitted to gamma spectrometry analysis for qualitative and quantitative evaluation of the radionuclides present in samples of sand, mortar, blue crushed stone, red crushed stone, concrete and red bricks. The method used for the measurements of radon activity in soil gas allowed to find the average concentrations of two isotopes 222Rn and 220Rn. The average concentration of indoor 222Rn obtained in the measurements in air of workplaces vary between 36 ± 49 Bq/m³ and 164 ± 51 Bq/m³. These values are considered within the reference limit of 200 Bq/m³ established by international agencies such as the United Nations Scientific Committee on the Effects of Atomic Radiation (UNSCEAR) and the International Commission on Radiological Protection (ICRP), but slightly above the limit of 148 Bq/m³ established by the United States Environmental Protection Agency (USEPA). The measurements involving building materials presented the concentration values of 222Rn in a range from 427 ± 310 Bq/m³ to 2053 ± 700 Bq/m³. The 222Rn concentrations in soil ranged from 31 ± 2 kBq/m³ to 35 ± 4 kBq/m³ and the average values of 220Rn are found in a range of 41 ± 6 kBq/m³ and 25 ± 11 kBq/m³, thus the concentrations of radon gas soil are below the Swedish criterion of 50 kBq/m³ that represent the minimum value for high-risk situation.

Published
2013

7. Probing the cosmic distance-duality relation with the Sunyaev-Zel’dovich effect, X-ray observations and supernovae Ia

Author

R. F. L. Holanda, J. A. S. Lima, and Marcelo B. Ribeiro

Subjects
Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Order (ring theory), Astronomy and Astrophysics, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Redshift, Luminosity, Supernova, Space and Planetary Science, Angular diameter, Cluster (physics), RADIAÇÃO DE FUNDO, Surface brightness, Galaxy cluster, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The angular diameter distances toward galaxy clusters can be determined with measurements of the Sunyaev-Zel'dovich effect and X-ray surface brightness combined with the validity of the distance-duality relation, $D_L(z) (1 + z)^{2}/D_{A}(z) = 1$, where $D_L(z)$ and $D_A(z)$ are, respectively, the luminosity and angular diameter distances. This combination enables us to probe galaxy cluster physics or even to test the validity of the distance-duality relation itself. We explore these possibilities based on two different, but complementary approaches. Firstly, in order to constrain the possible galaxy cluster morphologies, the validity of the distance-duality relation (DD relation) is assumed in the $\Lambda$CDM framework (WMAP7). Secondly, by adopting a cosmological-model-independent test, we directly confront the angular diameters from galaxy clusters with two supernovae Ia (SNe Ia) subsamples (carefully chosen to coincide with the cluster positions). The influence of the different SNe Ia light-curve fitters in the previous analysis are also discussed. We assumed that $\eta$ is a function of the redshift parametrized by two different relations: $\eta(z) = 1 + \eta_{0}z$, and $\eta(z)=1 + \eta_{0}z/(1+z)$, where $\eta_0$ is a constant parameter quantifying the possible departure from the strict validity of the DD relation. The statistical analysis presented here provides new evidence that the true geometry of clusters is elliptical. We find that the two-light curve fitters (SALT2 and MLCS2K2) present a statistically significant conflict, and a joint analysis involving the different approaches suggests that clusters are endowed with an elliptical geometry as previously assumed., Comment: 33 pages, 15 figures, some typos corrected, accepted for publication in the Astronomy \& Astrophysics

Published
2012

8. Aplicação de uma metodologia de screening para avaliar a mortalidade por câncer em municípios selecionados do Estado de Minas Gerais, Brasil

Author

Gulnar Azevedo e Silva Mendonça, Ubirani Otero, Berenice N. Antoniazzi, Silvana Rubano Barretto Turci, and Lene H. S. Veiga

Subjects
Cancer mortality, medicine.medical_specialty, Future studies, business.industry, Public Health, Environmental and Occupational Health, Cancer, medicine.disease, Neoplasias, Standardized mortality ratio, Cancer incidence, Environmental health, Epidemiology, medicine, Radiação de Fundo, Coeficiente de Mortalidade, Liver cancer, Lung cancer, business
Abstract

Iniciou-se uma investigação epidemiológica em municípios do sul de Minas Gerais, Brasil, considerando a possibilidade de aumento na incidência de câncer devido a maior exposição à radiação natural em alguns deles. Buscou-se, preliminarmente, conhecer o padrão de mortalidade por câncer, avaliar se existe excesso de óbitos e discutir os possíveis fatores de risco associados a esse aumento. Propõe-se uma metodologia de screening com base na razão de mortalidade padronizada (RMP) para classificar os municípios prioritários em estudos futuros. Os municípios considerados de altíssima prioridade para investigação foram: Andradas - câncer de pulmão em homens [RMP = 208 (106-310)] e fígado em mulheres [RMP = 403 (104-701)]; Poços de Caldas - leucemia em homens e mulheres (RMP = 284 (156-412) e RMP = 211 (111-312), respectivamente); Pouso Alegre - leucemia em homens [RMP = 333 (127-540)] e cânceres hematológicos em mulheres [RMP = 257 (188-396)].Estudos epidemiológicos devem ser conduzidos para avaliar a contribuição da radiação e outros fatores de riscos relacionados ao câncer e assim subsidiar futuras medidas de prevenção e controle.

Published
2007

9. Perturbações das equações de Einstein-Boltzmann e suas aplicações à radiação cósmica de fundo

Author

Barros, Gustavo de, Alcaniz, Jaílson Souza de, Waga, Ioav, and Calvão, Maurício Ortiz

Subjects
Cosmologia, Equações de Einstein-Boltzmann, Radiação de fundo, CIENCIAS EXATAS E DA TERRA::ASTRONOMIA::ASTROFISICA EXTRAGALACTICA::COSMOLOGIA [CNPQ]
Abstract

Submitted by André Araújo (leoaraujo@eba.ufrj.br) on 2019-01-09T13:22:59Z No. of bitstreams: 1 DSilva.pdf: 1122559 bytes, checksum: 66d41423da535191ebfb2ba84822814c (MD5) Made available in DSpace on 2019-01-09T13:22:59Z (GMT). No. of bitstreams: 1 DSilva.pdf: 1122559 bytes, checksum: 66d41423da535191ebfb2ba84822814c (MD5) Previous issue date: 2018 Estudo introdutório e didático dessa nova e crescente área da Cosmologia, que é a radiação cósmica de fundo (RCF). Apresentamos os conceitos, princípios e resultados básicos ligados a esse problema. Como a física que governa as equações a ele relacionadas vem essencialmente das perturbações das equações de Einstein-Boltzmann, grande parte desse trabalho direciona-se ao entendimento das perturbações lineares dessas equações, no “gauge” (calibre) newtoniano conforme, com tricurvatura nula e considerando apenas perturbações escalares. As condições iniciais desse sistema de equações também são exploradas. Outra parte principal é consagrada à aplicação desse sistema para a compreensão do espectro de potência das anisotropias em temperatura da RCF. Study aimed at understanding the basics of the new and growing topic of cosmic microwave background (CMB) physics. We present the fundamental concepts, principles and results related with this problem. Since the relevant equations are essentially the Einstein-Boltzmann perturbed equations, a great part of this work is dedicated to these linearized equations, in the conformal Newtonian gauge, with vanishing tri-curvature, for scalar perturbations only. The initial conditions are also touched on. Another part of paramount importance is the application to the description of the power spectrum of temperature anisotropies.

Published
2006

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