A next-to-leading order calculation of the impact of primordial magnetic fields into cosmological observables

In this thesis, we perform a next-to-leading order calculation of the impact of primordial magnetic fields (PMF) into the evolution of scalar cosmological perturbations and the cosmic microwave background (CMB) anisotropy. Magnetic fields are everywhere in the Universe at all scales probed so far, but their origin is still under debate. The current standard picture is that they originate from the amplification of initial seed fields, which could have been generated as PMFs in the early Universe. The most robust way to test their presence and constrain their features is to study how they impact on key cosmological observables, in particular the CMB anisotropies. The standard way to model a PMF is to consider its contribution (quadratic in the magnetic field) at the same footing of first order perturbations, under the assumptions of ideal magneto-hydrodynamics and compensated initial conditions. In the perspectives of ever increasing precision of CMB anisotropies measurements and of possible uncounted non-linear effects, in this thesis we study effects which go beyond the standard assumptions. We study the impact of PMFs on cosmological perturbations and CMB anisotropies with adiabatic initial conditions, the effect of Alfvén waves on the speed of sound of perturbations and possible non-linear behavior of baryon overdensity for PMFs with a blue spectral index, by modifying and improving the publicly available Einstein-Boltzmann code SONG, which has been written in order to take into account all second-order contributions in cosmological perturbation theory. One of the objectives of this thesis is to set the basis to verify by an independent fully numerical analysis the possibility to affect recombination and the Hubble constant.

Caso Danrley: luto [exercício]

Palavras cruzadas sobre o conteúdo Luto

Morte e luto

Backup moodle do módulo "Morte e luto" do curso de Especialização em Saúde da Pessoa Idosa produzido pela UNA-SUS/UFMA. Neste módulo são apresentados os princípios do cuidado paliativo em geriatria, o processo de morte e morrer no envelhecimento, além da humanização e controle de sintomas com abordagem interdisciplinar.

A morte e o luto: cuidado paliativo em Geriatria

Texto que compõe a unidade 1 do módulo “Morte e Luto” do curso de Especialização em Saúde da Pessoa Idoso produzido pela UNA-SUS/UFMA. Aborda, dentro do processo de envelhecimento, os princípios do Cuidado Paliativo, o processo de morte e o morrer, o luto e suas implicações frente ao indivíduo e aos seus familiares e por fim, apresenta como comunicar más notícias considerando as possibilidades do contexto de vida do indivíduo.

A morte e o luto: humanização e alívio de sintomas

Texto que compõe a unidade 2 do módulo “Morte e Luto” do curso de Especialização em Saúde da Pessoa Idoso produzido pela UNA-SUS/UFMA. Apresenta a abordagem multidisciplinar humanizada frente ao alívio de sintomas e a morte no domicílio.

Processo de morte e luto

O material é componente do Curso de Especialização em Saúde da Pessoa Idosa (unidade 2, módulo 13) da UNA-SUS/UFMA. Trata-se de um infográfico que apresenta algumas informações que permitem a melhor compreensão da morte e do luto.

Homozygous Inactivating Mutation In Nanos3 In Two Sisters With Primary Ovarian Insufficiency.

Despite the increasing understanding of female reproduction, the molecular diagnosis of primary ovarian insufficiency (POI) is seldom obtained. The RNA-binding protein NANOS3 poses as an interesting candidate gene for POI since members of the Nanos family have an evolutionarily conserved function in germ cell development and maintenance by repressing apoptosis. We performed mutational analysis of NANOS3 in a cohort of 85 Brazilian women with familial or isolated POI, presenting with primary or secondary amenorrhea, and in ethnically-matched control women. A homozygous p.Glu120Lys mutation in NANOS3 was identified in two sisters with primary amenorrhea. The substituted amino acid is located within the second C2HC motif in the conserved zinc finger domain of NANOS3 and in silico molecular modelling suggests destabilization of protein-RNA interaction. In vitro analyses of apoptosis through flow cytometry and confocal microscopy show that NANOS3 capacity to prevent apoptosis was impaired by this mutation. The identification of an inactivating missense mutation in NANOS3 suggests a mechanism for POI involving increased primordial germ cells (PGCs) apoptosis during embryonic cell migration and highlights the importance of NANOS proteins in human ovarian biology.

Atividade fisica e saude : estudo do conhecimento de professores de educação fisica do ensino fundamental atraves da educação a distancia

Universidade Estadual de Campinas . Faculdade de Educação Física

As interfaces entre imagem corporal e a representação simbolica de Carl Gustav Jung

Universidade Estadual de Campinas . Faculdade de Educação Física

Desenvolvimento morfológico dos ovários em fetos eqüinos sem raça definida

O objetivo deste trabalho foi caracterizar histologicamente o desenvolvimento ovariano pré-natal em fetos eqüinos sem raça definida (SRD) nos trópicos, ressaltando surgimento e quantificação de ovogônias e folículos. Foram obtidos 131 fetos em frigorífico, os quais foram mensurados quanto ao comprimento (cm) equivalente à distância cefalococcígea (CR), seguido de corte das gônadas e fixação das amostras em Bouin por 24 horas. As idades foram estimadas por regressão. Foram preparados cortes histológicos ovarianos de 7µm de espessura, os quais foram corados com hematoxilina-eosina. O surgimento de ovogônias, folículos primordiais, em crescimento e antrais foi verificado, respectivamente, em fetos com CR entre 4,1 e 6,5cm (40 a 49 dias de gestação (DG)); 9,1 e 12,0cm (60 a 69 DG); 23,1 e 29,0cm (116 a 135 DG) e 50,1 e 65,0cm (201 a 245 DG). A quantidade máxima de ovogônias, folículos primordiais, em crescimento e antrais foi observada em fetos com CR entre, 4,1 e 6,0cm (40 a 49 DG); 16,1 e 23,0cm (90 a 115 DG); 29,1 e 36,0cm (136 a 155 DG) e 50,1 e 97,0cm (201 a 320 DG), respectivamente. Os resultados sugerem que o desenvolvimento morfológico dos ovários fetais de eqüinos SRD nos trópicos é mais precoce que o observado nos relatos de literatura referentes a estudos de eqüinos de diversas raças em regiões temperadas.

Desenvolvimento da Tanatologia: estudos sobre a morte e o morrer

Este artigo discute os principais temas e pesquisas na área da Tanatologia, estudos sobre a morte e o morrer. São apresentados os autores pioneiros que escreveram as primeiras obras de sistematização da Tanatologia entre os quais: Herman Feifel, Robert Kastenbaum e Elizabeth Kübler-Ross, e os principais temas de estudo: luto, violência e guerra, a morte e a TV, cuidados a pacientes gravemente enfermos, além da formação de profissionais da área de saúde e educação para lidar com pessoas vivendo situações de perdas e morte. São feitas propostas de estudos para o futuro desenvolvimento da Tanatologia em nosso país.

Abundance variations in the globular cluster M71 (NGC 6838)

Context. Abundance variations in moderately metal-rich globular clusters can give clues about the formation and chemical enrichment of globular clusters. Aims. CN, CH, Na, Mg and Al indices in spectra of 89 stars of the template metal-rich globular cluster M71 are measured and implications on internal mixing are discussed. Methods. Stars from the turn-off up to the Red Giant Branch (0.87 < log g < 4.65) observed with the GMOS multi-object spectrograph at the Gemini-North telescope are analyzed. Radial velocities, colours, effective temperatures, gravities and spectral indices are determined for the sample. Results. Previous findings related to the CN bimodality and CN-CH anticorrelation in stars of M71 are confirmed. We also find a CN-Na correlation, and Al-Na, as well as an Mg(2)-Al anticorrelation. Conclusions. A combination of convective mixing and a primordial pollution by AGB or massive stars in the early stages of globular cluster formation is required to explain the observations.

Large change in the predicted number of small halos due to a small amplitude oscillating inflaton potential

A smooth inflaton potential is generally assumed when calculating the primordial power spectrum, implicitly assuming that a very small oscillation in the inflaton potential creates a negligible change in the predicted halo mass function. We show that this is not true. We find that a small oscillating perturbation in the inflaton potential in the slow-roll regime can alter significantly the predicted number of small halos. A class of models derived from supergravity theories gives rise to inflaton potentials with a large number of steps and many trans-Planckian effects may generate oscillations in the primordial power spectrum. The potentials we study are the simple quadratic (chaotic inflation) potential with superimposed small oscillations for small field values. Without leaving the slow-roll regime, we find that for a wide choice of parameters, the predicted number of halos change appreciably. For the oscillations beginning in the 10(7)-10(8) M(circle dot) range, for example, we find that only a 5% change in the amplitude of the chaotic potential causes a 50% suppression of the number of halos for masses between 10(7)-10(8) M(circle dot) and an increase in the number of halos for masses <10(6) M(circle dot) by factors similar to 15-50. We suggest that this might be a solution to the problem of the lack of observed dwarf galaxies in the range 10(7)-10(8) M(circle dot). This might also be a solution to the reionization problem where a very large number of Population III stars in low mass halos are required.

Origin of magnetic fields in galaxies

Microgauss magnetic fields are observed in all galaxies at low and high redshifts. The origin of these intense magnetic fields is a challenging question in astrophysics. We show here that the natural plasma fluctuations in the primordial Universe (assumed to be random), predicted by the fluctuation - dissipation theorem, predicts similar to 0.034 mu G fields over similar to 0.3 kpc regions in galaxies. If the dipole magnetic fields predicted by the fluctuation- dissipation theorem are not completely random, microgauss fields over regions greater than or similar to 0.34 kpc are easily obtained. The model is thus a strong candidate for resolving the problem of the origin of magnetic fields in less than or similar to 10(9) years in high redshift galaxies.

Populations III.1 and III.2 gamma-ray bursts: constraints on the event rate for future radio and X-ray surveys

Aims. We calculate the theoretical event rate of gamma-ray bursts (GRBs) from the collapse of massive first-generation (Population III; Pop III) stars. The Pop III GRBs could be super-energetic with the isotropic energy up to E(iso) greater than or similar to 10(55-57) erg, providing a unique probe of the high-redshift Universe. Methods. We consider both the so-called Pop III.1 stars (primordial) and Pop III.2 stars (primordial but affected by radiation from other stars). We employ a semi-analytical approach that considers inhomogeneous hydrogen reionization and chemical evolution of the intergalactic medium. Results. We show that Pop III.2 GRBs occur more than 100 times more frequently than Pop III.1 GRBs, and thus should be suitable targets for future GRB missions. Interestingly, our optimistic model predicts an event rate that is already constrained by the current radio transient searches. We expect similar to 10-10(4) radio afterglows above similar to 0.3 mJy on the sky with similar to 1 year variability and mostly without GRBs (orphans), which are detectable by ALMA, EVLA, LOFAR, and SKA, while we expect to observe maximum of N < 20 GRBs per year integrated over at z > 6 for Pop III.2 and N < 0.08 per year integrated over at z > 10 for Pop III.1 with EXIST, and N < 0.2 for Pop III.2 GRBs per year integrated over at z > 6 with Swift.