Deflagrations in hybrid CONe white dwarfs: a route to explain the faint Type Iax supernova 2008ha

Stellar evolution models predict the existence of hybrid white dwarfs (WDs) with a carbon-oxygen core surrounded by an oxygen-neon mantle. Being born with masses similar to 1.1 M-aS (TM), hybrid WDs in a binary system may easily approach the Chandrasekhar mass (M-Ch) by accretion and give rise to a thermonuclear explosion. Here, we investigate an off-centre deflagration in a near-M-Ch hybrid WD under the assumption that nuclear burning only occurs in carbon-rich material. Performing hydrodynamics simulations of the explosion and detailed nucleosynthesis post-processing calculations, we find that only 0.014 M-aS (TM) of material is ejected while the remainder of the mass stays bound. The ejecta consist predominantly of iron-group elements, O, C, Si and S. We also calculate synthetic observables for our model and find reasonable agreement with the faint Type Iax SN 2008ha. This shows for the first time that deflagrations in near-M-Ch WDs can in principle explain the observed diversity of Type Iax supernovae. Leaving behind a near-M-Ch bound remnant opens the possibility for recurrent explosions or a subsequent accretion-induced collapse in faint Type Iax SNe, if further accretion episodes occur. From binary population synthesis calculations, we find the rate of hybrid WDs approaching M-Ch to be of the order of 1 per cent of the Galactic SN Ia rate.

Polarization spectral synthesis for Type Ia supernova explosion models

We present a Monte Carlo radiative transfer technique for calculating synthetic spectropolarimetry for multidimensional supernova explosion models. The approach utilizes 'virtual-packets' that are generated during the propagation of the Monte Carlo quanta and used to compute synthetic observables for specific observer orientations. Compared to extracting synthetic observables by direct binning of emergent Monte Carlo quanta, this virtual-packet approach leads to a substantial reduction in the Monte Carlo noise. This is not only vital for calculating synthetic spectropolarimetry (since the degree of polarization is typically very small) but also useful for calculations of light curves and spectra. We first validate our approach via application of an idealized test code to simple geometries. We then describe its implementation in the Monte Carlo radiative transfer code ARTIS and present test calculations for simple models for Type Ia supernovae. Specifically, we use the well-known one-dimensional W7 model to verify that our scheme can accurately recover zero polarization from a spherical model, and to demonstrate the reduction in Monte Carlo noise compared to a simple packet-binning approach. To investigate the impact of aspherical ejecta on the polarization spectra, we then use ARTIS to calculate synthetic observables for prolate and oblate ellipsoidal models with Type Ia supernova compositions.

Fragilidades dos mecanismos de controle das organizações sociais de saúde no município do Rio de Janeiro

Nosso problema de pesquisa neste trabalho é a avaliação do funcionamento dos principais mecanismos de controle das organizações sociais de saúde, no caso específico do Município do Rio de Janeiro. As reiteradas denúncias de irregularidades e ilegalidades pelo Tribunal de Contas do Município do Rio de Janeiro e pelo Ministério Público do Estado do Rio de Janeiro levantaram dúvidas acerca da adequação dos processos de monitoramento, fiscalização e controle dessas entidades. Disto decorre nosso objetivo central de pesquisa, que é identificar as fragilidades do novo modelo de gestão por organizações sociais de saúde, no caso da cidade do Rio de Janeiro. Para isso, foram analisados: o arcabouço jurídico-normativo do modelo local, a partir de análise comparativa da legislação municipal que regulamenta seu funcionamento (Lei 5.026/09) e sua contraparte federal (Lei 9.637/98); indicadores de saúde que mensurassem o desempenho das OSS; todas as inspeções realizadas pelo TCM-RJ até o fim de 2015; e o conjunto de recomendações enviado pelo MP-ERJ para a Prefeitura após deflagração da Operação Ilha Fiscal, que acarretou a desqualificação da OS BIOTECH e a prisão de seus dirigentes, acusados de desviar mais de R$48 milhões em recursos públicos. Ao final, constatouse que as fragilidades da legislação municipal e dos decretos executivos que regulamentam a atuação das OSS no MRJ não permitem o exercício efetivo do comando da parceria, em afronta, portanto, ao dispositivo constitucional que determina que a atuação de entidades privadas no âmbito do SUS pode se dar apenas de modo complementar. Ademais, verificou-se total inadequação da estrutura de controle pela Prefeitura, cuja principal consequência foi tornar o modelo de reforma gerencialista em um modelo que incentiva o comportamento patrimonialista no âmbito da saúde pública, uma vez que o controle de meios é absolutamente negligenciado.

Type Ia Supernovae : Homogeneity and Diversity

The use of type Ia supernovae as distance estimators has shown that about 75% of the energy content of the universe has a negative equation of state parameter and thus, drives the acceleration of the universe. Constraining the exact nature of this energy is one of the main goals in cosmology. As the statistics of observed high-redshift supernovae increases, systematic effects become the limiting factor to pursue such investigations, thus deeper understanding of the physical properties of SNe is of great importance. In this thesis we investigate spectral homogeneity and diversity of local and high redshift supernovae. Special emphasis has been given to the analysis of optical spectra of local peculiar supernovae 1999aa and 1999ac. The study of the spectra of SN 1999aa pointed out that this SN could be a link between the extreme peculiar SN 1991T and normal SNe. Moreover, the identification of a high velocity component of Ca II and possibly of a low velocity component of C III suggests some degree of asphericity in the ejecta of this supernova. Evidence for a deflagration of a C+O white dwarf was found in the early spectra of SN 1999ac. The spectral proprieties of a vast sample of local SNe are also studied by means of newly introduced spectral indicators. These were used to possibly improve the intrinsic spread of SN peak magnitudes to 0.15 mag, independently of light curve parameters. The first quantitative comparison between local and high redshift supernova is carried out. No evidence for extreme peculiar sub-luminous SNe was found in our data set including 13 SNe with redshift range z=0.279-0.912. Furthermore, SN2002fd (z=0.279) was found to show spectral characteristics similar to SN 1991T/SN 1999aa-like supernovae. We also present a feasibility study of the Hubble diagram in rest frame I-band up to z~0.5, and show the possibility to probe the presence of intergalactic dust, which could possibly mimic the effect of dark energy in the Hubble diagram.

L'anno che non fu? L'anno dell'Europa e la crisi nelle relazioni transatlantiche, 1973/74

The 1970s are in the limelight of a growing historiographic attention, partly due to the recent opening of new archival resources. 1973, in particular, has a special interest in the historian’s eyes, as many are the events that happened that year: to name but a few, the Chilean coup, the October War, the ensuing oil crisis, the Vietnamese peace treaty. So it is may be not entirely surprising that not much attention has been paid to the Year of Europe, a nebulous American initiative destined to sum up to nothing practical - as Kissinger himself put it, it was destined to be the Year that never Was.1 It is my opinion, however, that its failure should not conceal its historical interest. Even though transatlantic relations have sometimes been seen as an uninterrupted history of crisis,2 in 1973 they reached what could then be considered as their unprecedented nadir. I believe that a thorough analysis of the events that during that year found the US increasingly at odds with the countries of Western Europe is worth carrying out not only to cast a new light on the dynamics of transatlantic relations but also to deepen our comprehension of the internal dynamics of the actors involved, mainly the Nixon administration and a unifying Europe. The Nixon administration had not carefully planned what the initiative actually should have amounted to, and its official announcement appears to have been one of Kissinger’s coups de theatre. Yet the Year of Europe responded to the vital priority of revitalising the relations with Western Europe, crucial ally, for too long neglected. But 1973 did not end with the solemn renewal of the Atlantic Declaration that Kissinger had sought. On the contrary, it saw, for the first time, the countries of the newly enlarged EC engaged in a real, if short-lived, solidarity on foreign policy, which highlighted the Nixon administration’s contradictions regarding European integration. Those, in addition to the numerous tensions that already strained transatlantic relations, gave birth to a downward spiral of incomprehensions and misperceptions, which the unexpected deflagration of the October war seriously worsened. However, even though the tensions did not disappear, the European front soon started to disintegrate, mainly under the strains imposed by the oil crisis. Significant changes in the leadership of the main European countries helped to get the tones back to normal. During the course of 1974-5, the substantial failure of the Euro-Arab dialogue, the Gymlich compromise, frequent and serene bilateral meetings bear witness that the worst was over.

Fatal contact shot to the chest caused by the gas jet from a muzzle-loading pistol discharging only black powder and no bullet: case study and experimental simulation of the wounding effect.

In modern medico-legal literature, only a small number of publications deal with fatal injuries from black powder guns. Most of them focus on the morphological features such as intense soot soiling, blast tattooing and burn effects in close-range shots or describe the wound ballistics of spherical lead bullets. Another kind of "unusual" and potentially lethal weapons are handguns destined for firing only blank cartridges such as starter and alarm pistols. The dangerousness of these guns is restricted to very close and contact range shots and results from the gas jet produced by the deflagration of the propellant. The present paper reports on a suicide committed with a muzzle-loading percussion pistol cal. 45. An unusually large stellate entrance wound was located in the precordial region, accompanied by an imprint mark from the ramrod and a faint greenish discoloration (apparently due to the formation of sulfhemoglobin). Autopsy revealed an oversized powder cavity, multiple fractures of the anterior thoracic wall as well as ruptures of the heart, the aorta, the left hepatic lobe and the diaphragm. In total, the zone of mechanical destruction had a diameter of approx. 15 cm. As there was no exit wound and no bullet lodged in the body, the injury was caused exclusively by the inrushing combustion gases of the propellant (black powder) comparable with the gas jet of a blank cartridge gun. In contact shots to ballistic gelatine using the suicide's pistol loaded with black powder but no projectile, the formation of a nearly spherical cavity could be demonstrated by means of a high-speed camera. The extent of the temporary cavity after firing with 5 g of black powder roughly corresponded to the zone of destruction found in the suicide's body.

Dynamics of thermal ignition of spray flames in mixing layers

Conditions are identified under which analyses of laminar mixing layers can shed light on aspects of turbulent spray combustion. With this in mind, laminar spray-combustion models are formulated for both non-premixed and partially premixed systems. The laminar mixing layer separating a hot-air stream from a monodisperse spray carried by either an inert gas or air is investigated numerically and analytically in an effort to increase understanding of the ignition process leading to stabilization of high-speed spray combustion. The problem is formulated in an Eulerian framework, with the conservation equations written in the boundary-layer approximation and with a one-step Arrhenius model adopted for the chemistry description. The numerical integrations unveil two different types of ignition behaviour depending on the fuel availability in the reaction kernel, which in turn depends on the rates of droplet vaporization and fuel-vapour diffusion. When sufficient fuel is available near the hot boundary, as occurs when the thermochemical properties of heptane are employed for the fuel in the integrations, combustion is established through a precipitous temperature increase at a well-defined thermal-runaway location, a phenomenon that is amenable to a theoretical analysis based on activation-energy asymptotics, presented here, following earlier ideas developed in describing unsteady gaseous ignition in mixing layers. By way of contrast, when the amount of fuel vapour reaching the hot boundary is small, as is observed in the computations employing the thermochemical properties of methanol, the incipient chemical reaction gives rise to a slowly developing lean deflagration that consumes the available fuel as it propagates across the mixing layer towards the spray. The flame structure that develops downstream from the ignition point depends on the fuel considered and also on the spray carrier gas, with fuel sprays carried by air displaying either a lean deflagration bounding a region of distributed reaction or a distinct double-flame structure with a rich premixed flame on the spray side and a diffusion flame on the air side. Results are calculated for the distributions of mixture fraction and scalar dissipation rate across the mixing layer that reveal complexities that serve to identify differences between spray-flamelet and gaseous-flamelet problems.

Critical radius for hot-jet ignition of hydrogen-air mixtures

This study addresses deflagration initiation of lean and stoichiometric hydrogen–air mixtures by the sudden discharge of a hot jet of their adiabatic combustion products. The objective is to compute the minimum jet radius required for ignition, a relevant quantity of interest for safety and technological applications. For sufficiently small discharge velocities, the numerical solution of the problem requires integration of the axisymmetric Navier–Stokes equations for chemically reacting ideal-gas mixtures, supplemented by standard descriptions of the molecular transport terms and a suitably reduced chemical-kinetic mechanism for the chemistry description. The computations provide the variation of the critical radius for hot-jet ignition with both the jet velocity and the equivalence ratio of the mixture, giving values that vary between a few tens microns to a few hundred microns in the range of conditions explored. For a given equivalence ratio, the critical radius is found to increase with increasing injection velocities, although the increase is only moderately large. On the other hand, for a given injection velocity, the smallest critical radius is found at stoichiometric conditions.

Estudo de balística interna

O conhecimento e a compreensão dos processos que ocorrem no interior do tubo de uma arma de fogo, desde a ignição da carga propulsora, até à saída do projétil, é importante no desenvolvimento do armamento, de uma forma económica e segura. Com a modelação matemática destes processos, que é uma abordagem muito utilizada atualmente, é possível otimizar a carga explosiva e os materiais utilizados. Este estudo foi realizado no âmbito do projeto FIREND, resultante da colaboração entre a Academia Militar e o Instituto Superior Técnico O modelo desenvolvido foi aplicado a um sistema, arma, carga propulsora e projétil, já existente, tendo os resultados obtidos sido validados com o software PRODAS e tabelas referentes ao presente sistema. Para melhor compreender a importância das variáveis envolvidas, é feita uma análise de sensibilidade a diversos parâmetros balísticos, mantendo constante as dimensões da arma em estudo. Na análise dos resultados verifica-se que a cinta de travamento é um elemento muito importante, alterando significativamente os valores da pressão e da velocidade. Verificou-se também que com cargas propulsoras de maior taxa de queima é possível obter valores mais elevados de pressão máxima e velocidade à saída. Palavras chave: Balística interna; Projétil de Artilharia; Pressão; Velocidade; Modelação matemática; Análise de sensibilidade.

Elements of electricity and electro-chemistry : /

In some copies, two additional plates showing the deflagration of wires are inserted.

Three-dimensional simulations of gravitationally confined detonations compared to observations of SN 1991T

The gravitationally confined detonation (GCD) model has been proposed as a possible explosion mechanism for Type Ia supernovae in the single-degenerate evolution channel. It starts with ignition of a deflagration in a single off-centre bubble in a near-Chandrasekhar-mass white dwarf. Driven by buoyancy, the deflagration flame rises in a narrow cone towards the surface. For the most part, the main component of the flow of the expanding ashes remains radial, but upon reaching the outer, low-pressure layers of the white dwarf, an additional lateral component develops. This causes the deflagration ashes to converge again at the opposite side, where the compression heats fuel and a detonation may be launched. We first performed five three-dimensional hydrodynamic simulations of the deflagration phase in 1.4 M⊙ carbon/oxygen white dwarfs at intermediate-resolution (2563computational zones). We confirm that the closer the initial deflagration is ignited to the centre, the slower the buoyant rise and the longer the deflagration ashes takes to break out and close in on the opposite pole to collide. To test the GCD explosion model, we then performed a high-resolution (5123 computational zones) simulation for a model with an ignition spot offset near the upper limit of what is still justifiable, 200 km. This high-resolution simulation met our deliberately optimistic detonation criteria, and we initiated a detonation. The detonation burned through the white dwarf and led to its complete disruption. For this model, we determined detailed nucleosynthetic yields by post-processing 106 tracer particles with a 384 nuclide reaction network, and we present multi-band light curves and time-dependent optical spectra. We find that our synthetic observables show a prominent viewing-angle sensitivity in ultraviolet and blue wavelength bands, which contradicts observed SNe Ia. The strong dependence on the viewing angle is caused by the asymmetric distribution of the deflagration ashes in the outer ejecta layers. Finally, we compared our model to SN 1991T. The overall flux level of the model is slightly too low, and the model predicts pre-maximum light spectral features due to Ca, S, and Si that are too strong. Furthermore, the model chemical abundance stratification qualitatively disagrees with recent abundance tomography results in two key areas: our model lacks low-velocity stable Fe and instead has copious amounts of high-velocity 56Ni and stable Fe. We therefore do not find good agreement of the model with SN 1991T.

LES of flame acceleration and DDT in hydrogen-air mixture using artificially thickened flame approach and detailed chemical kinetics

A large eddy simulation is performed to study the deflagration to detonation transition phenomenon in an obstructed channel containing premixed stoichiometric hydrogen–air mixture. Two-dimensional filtered reactive Navier–Stokes equations are solved utilizing the artificially thickened flame approach (ATF) for modeling sub-grid scale combustion. To include the effect of induction time, a 27-step detailed mechanism is utilized along with an in situ adaptive tabulation (ISAT) method to reduce the computational cost due to the detailed chemistry. The results show that in the slow flame propagation regime, the flame–vortex interaction and the resulting flame folding and wrinkling are the main mechanisms for the increase of the flame surface and consequently acceleration of the flame. Furthermore, at high speed, the major mechanisms responsible for flame propagation are repeated reflected shock–flame interactions and the resulting baroclinic vorticity. These interactions intensify the rate of heat release and maintain the turbulence and flame speed at high level. During the flame acceleration, it is seen that the turbulent flame enters the ‘thickened reaction zones’ regime. Therefore, it is necessary to utilize the chemistry based combustion model with detailed chemical kinetics to properly capture the salient features of the fast deflagration propagation.