Vincoli cosmologici da supernovae ad alto redshift

Le SNe Ia vengono utilizzate in cosmologia come indicatori di distanza. Nel 1998 due team di ricerca, il Supernova Cosmology Project e l'High-z Supernova Search Team compirono degli studi su un campione di SNe in galassie lontane a z=0.2-0.9. Da questi lavori emerse che le luminosità apparenti erano tipicamente inferiori del 25% rispetto ai valori attesi. Questo indica che tali oggetti si trovano ad una distanza di luminosità superiore a quella prevista da modelli d'Universo dominati da materia. Venne quindi determinata per la prima volta l'evidenza di un Universo in condizione di espansione accelerata. Lo scopo del presente lavoro di tesi è quello di analizzare i vincoli cosmologici imposti da SNe Ia ad alto redshift. È stato compiuto uno studio sui moduli di distanza osservativi di un campione di 580 SNe Ia al fine di trovare i parametri cosmologici che meglio descrivono il loro andamento in funzione del redshift nell'ambito dei modelli cosmologici standard con costante cosmologica positiva. Nella prima parte si illustreranno i modelli d’Universo di Friedmann, introducendo i concetti di redshift, di fattore di scala e i vari tipi di distanza. Nella seconda parte si descriverà cosa sono le Supernovae, e in particolare, le SNe di tipo Ia, le proprietà che le rendono candele standard e l'importanza che hanno assunto in cosmologia. Nella terza parte verranno presentanti i risultati prodotti per i due modelli studiati, verrà inoltre discussa la compatibilità con i parametri prodotti nei lavori compiuti dai due team di ricerca.

The peculiar Type Ia supernova iPTF14atg: Chandrasekhar-mass explosion or violent merger?

iPTF14atg, a subluminous peculiar Type Ia supernova (SN Ia) similar to SN 2002es, is the first SN Ia for which a strong UV flash was observed in the early-time light curves. This has been interpreted as evidence for a single-degenerate (SD) progenitor system, where such a signal is expected from interactions between the SN ejecta and the non-degenerate companion star. Here, we compare synthetic observables of multidimensional state-of-the-art explosion models for different progenitor scenarios to the light curves and spectra of iPTF14atg. From our models, we have difficulties explaining the spectral evolution of iPTF14atg within the SD progenitor channel. In contrast, we find that a violent merger of two carbon-oxygen white dwarfs with 0.9 and 0.76 M⊙, respectively, provides an excellent match to the spectral evolution of iPTF14atg from 10 d before to several weeks after maximum light. Our merger model does not naturally explain the initial UV flash of iPTF14atg. We discuss several possibilities like interactions of the SN ejecta with the circumstellar medium and surface radioactivity from an He-ignited merger that may be able to account for the early UV emission in violent merger models.

Dynamics and constraints of the massive graviton dark matter flat cosmologies

We discuss the dynamics of the Universe within the framework of the massive graviton cold dark matter scenario (MGCDM) in which gravitons are geometrically treated as massive particles. In this modified gravity theory, the main effect of the gravitons is to alter the density evolution of the cold dark matter component in such a way that the Universe evolves to an accelerating expanding regime, as presently observed. Tight constraints on the main cosmological parameters of the MGCDM model are derived by performing a joint likelihood analysis involving the recent supernovae type Ia data, the cosmic microwave background shift parameter, and the baryonic acoustic oscillations as traced by the Sloan Digital Sky Survey red luminous galaxies. The linear evolution of small density fluctuations is also analyzed in detail. It is found that the growth factor of the MGCDM model is slightly different (similar to 1-4%) from the one provided by the conventional flat Lambda CDM cosmology. The growth rate of clustering predicted by MGCDM and Lambda CDM models are confronted to the observations and the corresponding best fit values of the growth index (gamma) are also determined. By using the expectations of realistic future x-ray and Sunyaev-Zeldovich cluster surveys we derive the dark matter halo mass function and the corresponding redshift distribution of cluster-size halos for the MGCDM model. Finally, we also show that the Hubble flow differences between the MGCDM and the Lambda CDM models provide a halo redshift distribution departing significantly from the those predicted by other dark energy models. These results suggest that the MGCDM model can observationally be distinguished from Lambda CDM and also from a large number of dark energy models recently proposed in the literature.

Confronting dark energy models using galaxy cluster number counts

The mass function of cluster-size halos and their redshift distribution are computed for 12 distinct accelerating cosmological scenarios and confronted to the predictions of the conventional flat Lambda CDM model. The comparison with Lambda CDM is performed by a two-step process. First, we determine the free parameters of all models through a joint analysis involving the latest cosmological data, using supernovae type Ia, the cosmic microwave background shift parameter, and baryon acoustic oscillations. Apart from a braneworld inspired cosmology, it is found that the derived Hubble relation of the remaining models reproduces the Lambda CDM results approximately with the same degree of statistical confidence. Second, in order to attempt to distinguish the different dark energy models from the expectations of Lambda CDM, we analyze the predicted cluster-size halo redshift distribution on the basis of two future cluster surveys: (i) an X-ray survey based on the eROSITA satellite, and (ii) a Sunayev-Zeldovich survey based on the South Pole Telescope. As a result, we find that the predictions of 8 out of 12 dark energy models can be clearly distinguished from the Lambda CDM cosmology, while the predictions of 4 models are statistically equivalent to those of the Lambda CDM model, as far as the expected cluster mass function and redshift distribution are concerned. The present analysis suggests that such a technique appears to be very competitive to independent tests probing the late time evolution of the Universe and the associated dark energy effects.

Possible evidence of asymmetry in SN 2007rt, a type IIn supernova

An optical photometric and spectroscopic analysis of the slowly-evolving type IIn SN 2007rt is presented, covering a duration of 481 days after discovery. Its earliest spectrum, taken approximately 100 days after the explosion epoch, indicates the presence of a dense circumstellar medium, with which the supernova ejecta is interacting. This is supported by the slowly-evolving light curve. A notable feature in the spectrum of SN 2007rt is the presence of a broad He I 5875 line, not usually detected in type IIn supernovae. This may imply that the progenitor star has a high He/H ratio, having shed a significant portion of its hydrogen shell via mass-loss. An intermediate resolution spectrum reveals a narrow H(alpha) P-Cygni profile, the absorption component of which has a width of 128 km s (1). This slow velocity suggests that the progenitor of SN 2007rt recently underwent mass-loss with wind speeds comparable to the lower limits of those detected in luminous blue variables. Asymmetries in the line profiles of H and He at early phases bears some resemblance to double-peaked features observed in a number of Ib/c spectra. These asymmetries may be indicative of an asymmetric or bipolar outflow or alternatively dust formation in the fast expanding ejecta. In addition, the late time spectrum, at over 240 days post-explosion, shows clear evidence for the presence of newly formed dust.

A estrat??gia de Lisboa e as suas implica????es para a reforma institucional da Uni??o Europ??ia

Como manter a estrat??gia europ??ia de desenvolvimento atualizada, e ?? luz dos valores europeus, para reagir aos novos desafios decorrentes da globaliza????o, da mudan??a tecnol??gica e do envelhecimento das popula????es? Um novo paradigma emerge, em que o conhecimento e a inova????o s??o as principais fontes de riqueza e tamb??m de diferen??as entre as na????es, as empresas e as pessoas. Era preciso definir a via europ??ia de transi????o para essa economia baseada na inova????o e no conhecimento, com marcas distintas que v??o da salvaguarda da coes??o social e da diversidade cultural ??s pr??prias escolhas tecnol??gicas. Criar uma nova plataforma competitiva ?? fundamental para sustentar o modelo social europeu, que tamb??m dever?? ser renovado. Este artigo nos traz o debate dos pa??ses membros da Uni??o Europ??ia que precedeu a Cimeira de Lisboa (23 e 24 de Mar??o de 2000).

Competitive interactions between species of freshwater snails: I. Laboratory: Ia. General methodology

For the development of laboratory experiments on the competitive interacitons between freshwater snail populations, special snail rooms were set up in the main building of the Research Center "Aggeu Magalhães". In the current paper, the first of a series on this subject, the general methodology of the laboratory work is described in detail. Using indoor cement channels in which a uniform seminatural environment was created, interactions of freshwater snail populations can be studied with minimal interference of the usual variables. Controlled indoor environmental techniques, as described in the current paper, may also be utilized in different types of experiments in malacology, and represent a substantial technical advance in malacological work.

Heterogeneity of Ia antigen expression on myeloblastic leukaemias: correlation with stage of maturation defined by cytochemical markers.

The expression of Ia-like antigen (Ia) has been studied in 55 cases of acute myeloid leukaemia (AML) in correlation with the expression of both Sudan Black (SB) and naphthol AS-D chloroacetate esterase (NCAE) stains. Operationally the AML cases were divided into three groups using only NCAE expression on the leukaemic cells: the first group with early maturation stage (MS1) consisted of 30 cases with less than 10% NCAE positive cells (SB: 15-100%): the MS2 group of 14 cases with 10-70% NCAE positive cells (SB: 65-100%) and the MS3 group of 11 cases with 70-100% NCAE positive cells (SB: 89-100%). Ia expression was determined by complement-dependent cytotoxicity, immunofluorescence and immunoperoxidase methods. A similar high percentage (80%) of patients from both group MS1 and MS2 expressed Ia on the surface of 32-100% of the cells. Furthermore, individual comparison of all cases from these two groups showed no correlation between Ia, NCAE and SB expression. Only in the 11 cases from the MS3 group, which included nine cases of promyelocytic leukaemias, was there a correlation between very low expression of Ia antigen with the high NCAE expression. Thus, for AML with a low degree of differentiation the expression of Ia seems to be independent of conventional cytochemical markers of cell maturation.

Pulsed-field gel electrophoresis, virulence determinants and antimicrobial susceptibility profiles of type Ia group B streptococci isolated from humans in Brazil

Group B streptococci (GBS) infections occur worldwide. Although serotyping has been used for epidemiologic purposes, this does not accurately characterize enough members of a genetically heterogeneous bacterial population. The aims of this work were to evaluate the genetic diversity of 45 type Ia GBS strains isolated in Brazil by pulsed-field gel electrophoresis as well as to evaluate antimicrobial susceptibility profiles and identify virulence genes. Twenty-four strains were assigned to cluster A. All strains under study contained the hylB and scpB genes. The bca gene was detected in only 10 strains and none of the streptococci carried the bac gene. Thirty-nine strains were resistant to tetracycline.

The human Ia-associated invariant chain is synthesized in Ia-negative B cell variants and is not expressed on the cell surface of both Ia-negative and Ia-positive parental cells.

The expression of Ia-associated human Invariant (In) chain glycoproteins was studied in the Raji B cells as well as in their RJ 2.2.5 Ia-negative derived variant cells by using a specific rabbit anti-human In chain antiserum. Two-dimensional gel electrophoresis of immunoprecipitates from either biosynthetically labeled or surface labeled cells were analyzed. In addition, flow microfluorometric analysis of stained cells was performed. The results indicate that the In chain is constitutively produced in the Ia-negative B cell variant. Moreover, it appears that several forms of In chain-related molecules, with different charges and distinct m.w. are equally expressed in Ia-positive and Ia-negative B cells. Finally, no evidence could be obtained that the In molecular family was expressed on the cell surface of Ia-positive Raji and Ia-negative RJ 2.2.5 cells.

[Archives de la Parole]. , Parable of the prodigal son : in Maria from Bastar (C.P) [i.e. Central Provinces] / [Sir George Grierson], éd. ; Linguistic survey of India ; [Kānā Māṛia], voix

[Traditions. Asie. Inde. Madhya Pradesh. Chhattisgarh]

[Archives de la Parole]. , A loafer's marriage : a fable in Maria from Bastar (C.P) [i.e. Central Provinces] / [Sir George Grierson], éd. ; Linguistic survey of India ; [Kānā Māṛia], voix

[Traditions. Asie. Inde. Madhya Pradesh. Chhattisgarh]

¶ LE VOYAGE et || expedition de Charles le quint em- || pereur en Africque cõtre la || ville de Argiere. || ¶ La description de larmee & voyage de || Lempereur en Africque contre la || ville de Argiere / enuoyee a || mõsieur de Langest / tra- || duicte de latin en || françois. || ¶ Mil. D. xlii [1542] || ¶ On les vend a Paris en la rue sainct Ia- || ques a lenseigne des troys Brochetz / par Be- || noist de Gourmont. In-8 de 20 f. non chiffr. de 25 lignes à la page, sign. A-E par 4, mar. br., riches entrelacs et rinceaux en mosaïque de mar. vert, citron et rouge, doublé de mar. bleu, feuillages à petits fers, dos orné, gardes de moire bleue, tr. dor., dans un étui de mar. v. (Lortic.)

Charles Quint, roi d'Espagne et empereur d'Allemagne, d'abord archiduc d'Autriche. Le Voyage et Expedition de Charles le quint en Africque contre la ville de Argiere (1542)