Theoretical models of planetary system formation: mass vs. semi-major axis

Context. Planet formation models have been developed during the past years to try to reproduce what has been observed of both the solar system and the extrasolar planets. Some of these models have partially succeeded, but they focus on massive planets and, for the sake of simplicity, exclude planets belonging to planetary systems. However, more and more planets are now found in planetary systems. This tendency, which is a result of radial velocity, transit, and direct imaging surveys, seems to be even more pronounced for low-mass planets. These new observations require improving planet formation models, including new physics, and considering the formation of systems. Aims: In a recent series of papers, we have presented some improvements in the physics of our models, focussing in particular on the internal structure of forming planets, and on the computation of the excitation state of planetesimals and their resulting accretion rate. In this paper, we focus on the concurrent effect of the formation of more than one planet in the same protoplanetary disc and show the effect, in terms of architecture and composition of this multiplicity. Methods: We used an N-body calculation including collision detection to compute the orbital evolution of a planetary system. Moreover, we describe the effect of competition for accretion of gas and solids, as well as the effect of gravitational interactions between planets. Results: We show that the masses and semi-major axes of planets are modified by both the effect of competition and gravitational interactions. We also present the effect of the assumed number of forming planets in the same system (a free parameter of the model), as well as the effect of the inclination and eccentricity damping. We find that the fraction of ejected planets increases from nearly 0 to 8% as we change the number of embryos we seed the system with from 2 to 20 planetary embryos. Moreover, our calculations show that, when considering planets more massive than ~5 M⊕, simulations with 10 or 20 planetary embryos statistically give the same results in terms of mass function and period distribution.

Growth of tin oxide single crystals in porcelain tunnel kilns

Single crystals of tin oxide have been grown under conditions obtained in oil fired porcelain tunnel kilns. It was noted that the reducing conditions in the kilns help in the growth of SnO2 crystals at much lower temperatures (1300°C). The growth seems to more pronounced in presence of silicon carbide. The crystals grow as long fibres of 0.1 to 0.5 mm dia. and 10 to 50 mm length. The crystals exhibit rutile structure and the direction of growth seems to be favoured in any one of the major axes a and c.

A unified view of energetic efficiency in active drag reduction, thrust generation and self-propulsion through a loss coefficient with some applications

An analysis of the energy budget for the general case of a body translating in a stationary fluid under the action of an external force is used to define a power loss coefficient. This universal definition of power loss coefficient gives a measure of the energy lost in the wake of the translating body and, in general, is applicable to a variety of flow configurations including active drag reduction, self-propulsion and thrust generation. The utility of the power loss coefficient is demonstrated on a model bluff body flow problem concerning a two-dimensional elliptical cylinder in a uniform cross-flow. The upper and lower boundaries of the elliptic cylinder undergo continuous motion due to a prescribed reflectionally symmetric constant tangential surface velocity. It is shown that a decrease in drag resulting from an increase in the strength of tangential surface velocity leads to an initial reduction and eventual rise in the power loss coefficient. A maximum in energetic efficiency is attained for a drag reducing tangential surface velocity which minimizes the power loss coefficient. The effect of the tangential surface velocity on drag reduction and self-propulsion of both bluff and streamlined bodies is explored through a variation in the thickness ratio (ratio of the minor and major axes) of the elliptical cylinders.

Administração pública e poder discricionário no Brasil: contribuição para uma nova teoria do poder discricionário sob uma perspectiva responsiva

O presente trabalho busca examinar, em perspectiva histórica, aspectos sociopolíticos e jurídicos relacionados à formação da Administração Pública no Brasil e às suas características, notadamente no que concerne ao processo de legitimação do exercício do poder pelo aparelho burocrático e ao seu potencial controle pelos cidadãos. Argumenta-se que, se por um lado tais características revelam a resistência de um modelo associado ao legado ibérico, de outro evidenciam uma peculiar e progressiva abertura ao controle democrático, especialmente após a redemocratização e a promulgação da Constituição Federal de 1988. Adotando o exercício do poder administrativo discricionário como categoria de análise, os aspectos inerentes ao processo de transformação daquele modelo são examinadas a partir de quatro eixos, a saber: a singular tensão entre Iberismo e Americanismo no Brasil; a renovação teórica acerca da democracia representativa e das perspectivas sobre o controle democrático; o pós-positivismo e sua potencial conexão com uma concepção responsiva do direito e, finalmente, a queda de velhos paradigmas de legitimação do exercício do poder discricionário estatal, em âmbito mundial, a partir dos anos 1980, o que teria dado ensejo ao crescimento e fortalecimento de um escrutínio pragmático e consequencialista das decisões discricionárias da administração pública também no Brasil.

趋磁细菌AMB-1培养条件优化及磁小体变化过程研究

趋磁细菌(Magnetotactic bacteria)的研究是国际微生物学研究热点之一。趋磁细菌体内含有纳米单磁畴的氧化铁/硫化铁(Fe3O4或Fe3S4)晶体，称为磁小体。由于趋磁细菌营养条件要求苛刻，在环境中需要微好氧条件，且营养类型属于化能自养，使得培养趋磁细菌时常遇到问题。 本研究首先通过正交试验优化趋磁细菌AMB-1菌株培养条件，在培养条件铁源为奎尼酸铁0.02 mmol/L，装瓶量75% ，pH值6.7，温度25 ℃时，AMB-1 OD600达到0.440(1.166×109 cells/ml)。同时运用磁收集传代法，使带有磁小体的AMB-1细胞比例占95％以上(Cmag值稳定在1.9-2.0)。 在AMB-1具有较好的生物量，同时又具有较好的含磁小体细胞比例后，研究磁小体的变化过程。通过透射电镜观察磁小体变化过程，发现培养24 h细菌体内已有较小晶体形成(平均27 nm，n=188)且沿长轴分布；48 h晶体长大(平均43 nm，n=203)且形成分段链沿长轴排列；72 h晶体进一步成熟(平均50 nm，n=191)仍以分段链沿长轴排列；随后细菌逐渐衰亡磁小体变小，168 h可见部分自溶细菌中仍有磁小体链(平均37 nm，n=186)；192 h细菌自溶磁小体链(平均33 nm，n=184)分散到环境中。 通过透射电镜在细胞水平上研究趋磁细菌细胞分裂时发现，磁小体在细菌分裂时采用两种分离方式：一种为磁小体分配到两个子细胞；另一种为磁小体只分配到一个子细胞。无磁小体的子细胞，在随后的生长过程又分为两种情况：一种为细胞逐渐产生磁小体，另一种为不再产生磁小体。这种现象的发现，解释了随着传代次数的增多，细菌磁性有所下降的原因(Cmag值降低)。 在对趋磁细菌磁小体合成机制的研究中，常使用基因敲除的办法获得缺陷型，并与野生型对比进行研究。但是，利用基因敲除获得缺陷型不仅操作繁琐并且所得缺陷型不稳定。本研究利用特殊的磁富集传代法，先将带有磁小体的菌体收集并连续传代，筛选获得了高磁菌株；利用这种方法，收集不含磁小体的菌体并连续传代，筛选获得了无磁菌株。 趋磁细菌磁小体在医疗、环保等领域具有广阔应用价值，但是目前由于趋磁细菌难以大规模培养，并且磁小体纯化存在成本高等原因，将磁小体真正实际应用尚有一段距离。通过研究磁小体在趋磁细菌中的变化过程发现，AMB-1菌株在培养192 h后自溶，并且磁小体随着细胞的破碎释放到环境中去。

CCD photometry of distant comets II

R band CCD photometric observations of short period Jupiter family comets in the heliocentric region of 2.11 AU less than or equal to R-h less than or equal to 5.63 AU were performed using the 4.2 m William Herschel Telescope on La Palma in December 1998. 22 comets were targeted, including the comet- asteroid transition object 49P/Arend-Rigaux. Out of a total of ten detected comets. six were seen to display substantial outgassing (48P, 65P, 74P, 103Pt 128P, and 139P), with the remaining four comets (7P. 9P, 22P. and 49P) being stellar in appearance. Nuclear radius measurements and relative dust production rates in terms of Af rho were measured for these comets, along with upper limits for the remaining twelve undetected comets (6P, 44P, 51P, 54P, 57P: 63P, 71P, 73P, 79P, 86P, 87P, and 100P). The inactive comets had nuclear radii in the range 1.8 km less than or equal to r(N) less than or equal to 4.4 km, while upper limits for the active and undetected comets (assuming they all lay within the held of view) were between 0.6 km and 12.7 km, for an assumed albedo of 0.04. Even if one applies the previously measured maximum axis ratio of 2.6:1 and the minimum measured albedo of 0.02 to the undetected comets. their projected semi-major axes are all constrained to below 8 km. For the active comets, photometric profiles of their dust comae were measured and are consistent with those of steady state coma models.

Cardiologie nucléaire du 21ième siècle : nouveautés et réalités

Les maladies cardio-vasculaires demeurent une cause majeure de mortalité et morbidité dans les sociétés développées. La recherche de déterminants prédictifs d’évènements vasculaires représente toujours un enjeu d’actualité face aux coûts croissants des dépenses reliées aux soins médicaux et à l’élargissement des populations concernées, notamment face à l’occidentalisation des pays émergeants comme l’Inde, le Brésil et la Chine. La cardiologie nucléaire occupe depuis trente ans, une place essentielle dans l’arsenal des méthodes diagnostiques et pronostiques des cardiopathies. De plus, de nouvelles percées permettront de dépister d’une façon plus précoce et précise, la maladie athérosclérotique cardiaque et périphérique chez les populations atteintes ainsi qu’en prévention primaire. Nous présenterons dans cette thèse, deux approches nouvelles de la cardiologie nucléaire. La dysfonction endothéliale est considérée comme le signal pathologique le plus précoce de l’athérosclérose. Les facteurs de risques cardiovasculaires traditionnels atteignent la fonction endothéliale et peuvent initier le processus d’athérosclérose même en l’absence de lésion endothéliale physique. La quantification de la fonction endothéliale coronarienne comporte donc un intérêt certain comme biomarqueur précoce de la maladie coronarienne. La pléthysmographie isotopique, méthodologie développée lors de ce cycle d’étude, permet de quantifier la fonction endothéliale périphérique, cette dernière étant corrélée à la fonction endothéliale coronarienne. Cette méthodologie est démontrée dans le premier manuscrit (Harel et. al., Physiol Meas., 2007). L’utilisation d’un radiomarquage des érythrocytes permet la mesure du flot artériel au niveau du membre supérieur pendant la réalisation d’une hyperémie réactive locale. Cette nouvelle procédure a été validée en comparaison à la pléthysmographie par jauge de contrainte sur une cohorte de 26 patients. Elle a démontré une excellente reproductibilité (coefficient de corrélation intra-classe = 0.89). De plus, la mesure du flot artérielle pendant la réaction hyperémique corrélait avec les mesure réalisées par la méthode de référence (r=0.87). Le deuxième manuscrit expose les bases de la spectroscopie infrarouge comme méthodologie de mesure du flot artériel et quantification de la réaction hyperémique (Harel et. al., Physiol Meas., 2008). Cette étude utilisa un protocole de triples mesures simultanées à l’aide de la pléthysmographie par jauge de contrainte, radio-isotopique et par spectroscopie infrarouge. La technique par spectroscopie fut démontrée précise et reproductible quant à la mesure des flots artériels au niveau de l’avant-bras. Cette nouvelle procédure a présenté des avantages indéniables quant à la diminution d’artéfact et à sa facilité d’utilisation. Le second volet de ma thèse porte sur l’analyse du synchronisme de contraction cardiaque. En effet, plus de 30% des patients recevant une thérapie de resynchronisation ne démontre pas d’amélioration clinique. De plus, ce taux de non-réponse est encore plus élevé lors de l’utilisation de critères morphologiques de réponse à la resynchronisation (réduction du volume télésystolique). Il existe donc un besoin urgent de développer une méthodologie de mesure fiable et précise de la dynamique cardiaque. Le troisième manuscrit expose les bases d’une nouvelle technique radio-isotopique permettant la quantification de la fraction d’éjection du ventricule gauche (Harel et. al. J Nucl Cardiol., 2007). L’étude portant sur 202 patients a démontré une excellente corrélation (r=0.84) avec la méthode de référence (ventriculographie planaire). La comparaison avec le logiciel QBS (Cedar-Sinai) démontrait un écart type du biais inférieur (7.44% vs 9.36%). De plus, le biais dans la mesure ne démontrait pas de corrélation avec la magnitude du paramètre pour notre méthodologie, contrairement au logiciel alterne. Le quatrième manuscrit portait sur la quantification de l’asynchronisme intra-ventriculaire gauche (Harel et. al. J Nucl Cardiol, 2008). Un nouveau paramètre tridimensionnel (CHI: contraction homogeneity index) (médiane 73.8% ; IQ 58.7% - 84.9%) permis d’intégrer les composantes d’amplitude et du synchronisme de la contraction ventriculaire. La validation de ce paramètre fut effectuée par comparaison avec la déviation standard de l’histogramme de phase (SDΦ) (médiane 28.2º ; IQ 17.5º - 46.8º) obtenu par la ventriculographie planaire lors d’une étude portant sur 235 patients. Ces quatre manuscrits, déjà publiés dans la littérature scientifique spécialisée, résument une fraction des travaux de recherche que nous avons effectués durant les trois dernières années. Ces travaux s’inscrivent dans deux axes majeurs de développement de la cardiologie du 21ième siècle.

Écriture autobiographique et sceau cicatriciel dans L’Ascension du Haut Mal de David B.

Le présent mémoire vise à détailler les particularités du discours autobiographique dans L’Ascension du Haut Mal afin de saisir la poétique de David B. comme un sceau cicatriciel permettant de rendre compte de la maladie fraternelle et d’y faire face, au moyen de stratégies autobiographiques qui consolident textuellement et visuellement l’identité de l’auteur-personnage au sein du récit. Le premier chapitre consiste en une étude sur les récits de soi en bande dessinée. Un survol historique de l’évolution de la bande dessinée autobiographique dans la francophonie européenne inscrit L’Ascension du Haut Mal dans le mouvement de contestation mené par les maisons d’édition alternatives du début des années 1990. Puis, l’état des lieux en matière de théories portant sur l’autobiographie en bande dessinée établit les critères selon lesquels cette œuvre répond au genre autobiographique. Les deux chapitres suivants correspondent aux grands axes du discours autoréférentiel de L’Ascension du Haut Mal: le postulat d’un pacte autobiographique et le récit de la construction identitaire de l’auteur. Le deuxième chapitre explique par quels moyens l’hybridité formelle, la dimension fantasmatique et le foisonnement intertextuel de l’œuvre étudiée altèrent le pacte autobiographique sans toutefois le rompre. Le troisième chapitre démontre que le développement identitaire du personnage de David B. répond à une logique d’opposition, en regard de son frère, de la société et même de la réalité, visible jusque dans l’esthétique de l’auteur. L’analyse des marques graphiques et thématiques symptomatiques des défenses élevées par David B. contre la tyrannie du Haut Mal, l’épilepsie, est effectuée.

La presse satirique illustrée française et la colonisation (1829-1990)

- Thèse réalisée en cotutelle entre les Université de Montréal et Paris Ouest Nanterre la Défense. -Thèse construite à partir de logiciels libres et gratuits : Ubuntu, Lyx, LibreOffice, Zotero, The Gimp.

Multi-instrument ground-based observations of a travelling convection vortices event

A coordinated ground-based observational campaign using the IMAGE magnetometer network, EISCAT radars and optical instruments on Svalbard has made possible detailed studies of a travelling convection vortices (TCV) event on 6 January 1992. Combining the data from these facilities allows us to draw a very detailed picture of the features and dynamics of this TCV event. On the way from the noon to the drawn meridian, the vortices went through a remarkable development. The propagation velocity in the ionosphere increased from 2.5 to 7.4 km s−1, and the orientation of the major axes of the vortices rotated from being almost parallel to the magnetic meridian near noon to essentially perpendicular at dawn. By combining electric fields obtained by EISCAT and ionospheric currents deduced from magnetic field recordings, conductivities associated with the vortices could be estimated. Contrary to expectations we found higher conductivities below the downward field aligned current (FAC) filament than below the upward directed. Unexpected results also emerged from the optical observations. For most of the time there were no discrete aurora at 557.7 nm associated with the TCVs. Only once did a discrete form appear at the foot of the upward FAC. This aurora subsequently expanded eastward and westward leaving its centre at the same longitude while the TCV continued to travel westward. Also we try to identify the source regions of TCVs in the magnetosphere and discuss possible generation mechanisms.

Alfabetização de crianças e jovens: superando desafios da inclusão escolar

This work has its genesis in the life of a teacher. It contemplates the report of a great story that expresses the political will of anonymous people who sought/seek to overcome challenges and prejudices, a joint effort to make real the right to literacy. The reported story was developed in the Pedagogic Clinic Teacher Heitor Carrilho, Natal-RN which, concerned about the sentence of 'unable to learn the written language' attributed to children and young public school students, decided to invest in overcoming prejudices and fight against school failure of these underprivileged. The problem that motivated the study was thus set up: What particularities characterize a pedagogical practice which aims to teach literacy to children and youth from public schools, considered not capable of learning the written language? What theoretical and methodological procedures are shown as a boost to literacy in the development of a pedagogical practice systematically targeted to reflect the perspective of educating those students in public schools? Aiming to answer these questions, we conducted a qualitative research having as methodology, Life Stories and Research/Formation. For the construction of the data, it was decided to use the participative observation, semi-structured interviews and document analysis. Guided by the principles of content analysis the data analysis was built, from which emerged two categories: theoretical and methodological procedures aligned to the major axes of literacy and Procedures of the specific theoretical and methodological fundamentals of literacy. As subsets of the transverse procedures others were seized: didactic-pedagogic procedures; social affective procedures. Regarding these ones, the research shows the importance of the teacher to build a relationship of listening to the students and their families in order to organize the pedagogical work, looking at multiple dimensions of the subject: the intellect, the creative, the affective, moral, noting that between the methodology and didactics or as part of it, the links built represent great opportunities to promote literacy. Regarding the specific procedures, others were built: procedures that emphasize oral communication, procedures that favor writing and procedures that privilege reading. Under these procedures, the results of research show that you can only promote literacy if the teacher provides the students effective conditions of understanding the principles of alphabetical notation from the use of various kinds of texts, leading them to comprehend and use them in different contexts. Therefore, instructors must meet the learners' prior knowledge, their language, and the learning real needs that will bring new challenges consistent with their possibilities. The research confirms the importance of the Educational Support extra school. However, it is essential to emphasize that it is a function of the school to promote literacy for all students in the early years of schooling. It is recorded, however, that for the implementation of this desire, we must break the school model characterized by a rigid tradition, in which there is only room for those who learn the content taught in a minimum time. Unfortunately, despite the discourse of inclusion and ensuring the right to education, the school remains exclusive and selective separating the school learning of interpersonal relations and social integration and performance. On the one hand, research showed the difficulties of conducting studies and/or strategies that address the particularities of children and young people believed not capable of learning. On the other hand, the political commitment and motivation have increased the perception that it is possible to mitigate the existing deficits in the educational context, beginning with the everyday teaching practice, in which new knowledge can be learned, methodologies can be improved and, despite everything, the educational success can be built

Possible effects of secular resonances in Phobos and Triton

Due to the tides, the orbits of Phobos and Triton are contracting. While their semi major axes are decreasing, several possibilities of secular resonances involving node, argument of the pericenter and mean motion of the Sun will take place. In the case of Mars, if the obliquity (epsilon), during the passage through some resonances, is not so small, very significant variations of the inclination will appear. In one case, capture is almost certain provided that epsilon greater than or equal to 20degrees. For Triton there are also similar situations, but capture seems to be not possible, mainly because in S-1 state, Triton's orbit is sufficiently inclined (far) with respect to the Neptune's equator. Following Chyba et al. (Astron. Astrophys. 219 (1989) 123), a simplified equation that gives the evolution of the inclination versus the semi major axis, is derived. The time needed for Triton crash onto Neptune is longer than that one obtained by these authors, but the main difference is due to the new data used here. In general, even in the case of non-capture passages, some significant jumps in inclination and in eccentricities are possible. (C) 2002 Elsevier B.V. Ltd. All rights reserved.

Inner satellites of Neptune: I the disturbing function

In this work, we focus our attention to the expansion of the disturbing function (R) which governs the dynamics of a satellite (natural or artificial) in the Neptune-Triton system. What makes this problem quite unusual, is the fact that a small inner satellite can be strongly disturbed by Triton which is moving in a highly inclined and retrograde orbit. These features are unique in our solar system. Although a lot of retrograde satellites are currently known, all of them have negligible mass and the), do not offer almost any perturbation on the others satellites. However, in the case of the inner satellites of Neptune, Triton is an interesting exception. In a highly inclined orbit, the perturbation it exerts on the neighbouring satellites of Neptune cannot be ignored even for the present scenario. However, in the future, this perturbation will be much more important because due to the tides, the orbit of Triton is contracting, whereas the semi major axes of the remaining inner satellites of Neptune will remain almost unaffected by the tides. In this work we first obtain the disturbing function in the retrograde case. After that, we generalize R for arbitrary inclination. Several numerical tests are presented and a possible future case of resonant configuration is briefly discussed as well. (c) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.

Study of the potential of irregular shaped bodies and orbits around a non-spherical body

In the present work we show the expressions of the gravitational potential of homogeneous bodies with non-spherical three-dimensional shapes in order to study the trajectories around these bodies. The potentials of a prolate and an oblate ellipsoids with different values of semi-major axis are presented. Their results are validated with a test using a spherical body in order to guarantee the approximation of any body as a polyhedral model of the body. With these expressions we study trajectories of a point of mass around the three-dimensional bodies and the results indicated that there is a group of orbits around those bodies and the polyhedral form of the object does work very well. Copyright IAF/IAA. All rights reserved.

Estudos sobre as defasagens de Prometeu e Pandora

Pós-graduação em Física - FEG