Bayesian analysis and constraints on kinematic models from union SNIa

The kinematic expansion history of the universe is investigated by using the 307 supernovae type Ia from the Union Compilation set. Three simple model parameterizations for the deceleration parameter ( constant, linear and abrupt transition) and two different models that are explicitly parametrized by the cosmic jerk parameter ( constant and variable) are considered. Likelihood and Bayesian analyses are employed to find best fit parameters and compare models among themselves and with the flat Lambda CDM model. Analytical expressions and estimates for the deceleration and cosmic jerk parameters today (q(0) and j(0)) and for the transition redshift (z(t)) between a past phase of cosmic deceleration to a current phase of acceleration are given. All models characterize an accelerated expansion for the universe today and largely indicate that it was decelerating in the past, having a transition redshift around 0.5. The cosmic jerk is not strongly constrained by the present supernovae data. For the most realistic kinematic models the 1 sigma confidence limits imply the following ranges of values: q(0) is an element of [-0.96, -0.46], j(0) is an element of [-3.2,-0.3] and z(t) is an element of [0.36, 0.84], which are compatible with the Lambda CDM predictions, q(0) = -0.57 +/- 0.04, j(0) = -1 and z(t) = 0.71 +/- 0.08. We find that even very simple kinematic models are equally good to describe the data compared to the concordance Lambda CDM model, and that the current observations are not powerful enough to discriminate among all of them.

CDM accelerating cosmology as an alternative to Lambda CDM model

A new accelerating cosmology driven only by baryons plus cold dark matter (CDM) is proposed in the framework of general relativity. In this scenario the present accelerating stage of the Universe is powered by the negative pressure describing the gravitationally-induced particle production of cold dark matter particles. This kind of scenario has only one free parameter and the differential equation governing the evolution of the scale factor is exactly the same of the Lambda CDM model. For a spatially flat Universe, as predicted by inflation (Omega(dm) + Omega(baryon) = 1), it is found that the effectively observed matter density parameter is Omega(meff) = 1 - alpha, where alpha is the constant parameter specifying the CDM particle creation rate. The supernovae test based on the Union data (2008) requires alpha similar to 0.71 so that Omega(meff) similar to 0.29 as independently derived from weak gravitational lensing, the large scale structure and other complementary observations.

Type Ia Supernova Cosmology : Quantitative Spectral Analysis

Type Ia supernovae have been successfully used as standardized candles to study the expansion history of the Universe. In the past few years, these studies led to the exciting result of an accelerated expansion caused by the repelling action of some sort of dark energy. This result has been confirmed by measurements of cosmic microwave background radiation, the large-scale structure, and the dynamics of galaxy clusters. The combination of all these experiments points to a “concordance model” of the Universe with flat large-scale geometry and a dominant component of dark energy. However, there are several points related to supernova measurements which need careful analysis in order to doubtlessly establish the validity of the concordance model. As the amount and quality of data increases, the need of controlling possible systematic effects which may bias the results becomes crucial. Also important is the improvement of our knowledge of the physics of supernovae events to assure and possibly refine their calibration as standardized candle. This thesis addresses some of those issues through the quantitative analysis of supernova spectra. The stress is put on a careful treatment of the data and on the definition of spectral measurement methods. The comparison of measurements for a large set of spectra from nearby supernovae is used to study the homogeneity and to search for spectral parameters which may further refine the calibration of the standardized candle. One such parameter is found to reduce the dispersion in the distance estimation of a sample of supernovae to below 6%, a precision which is comparable with the current lightcurve-based calibration, and is obtained in an independent manner. Finally, the comparison of spectral measurements from nearby and distant objects is used to test the possibility of evolution with cosmic time of the intrinsic brightness of type Ia supernovae.

Consequences of dark matter-dark energy interaction on cosmological parameters derived from type Ia supernova data

Models where the dark matter component of the Universe interacts with the dark energy field have been proposed as a solution to the cosmic coincidence problem, since in the attractor regime both dark energy and dark matter scale in the same way. In these models the mass of the cold dark matter particles is a function of the dark energy field responsible for the present acceleration of the Universe, and different scenarios can be parametrized by how the mass of the cold dark matter particles evolves with time. In this article we study the impact of a constant coupling delta between dark energy and dark matter on the determination of a redshift dependent dark energy equation of state w(DE)(z) and on the dark matter density today from SNIa data. We derive an analytical expression for the luminosity distance in this case. In particular, we show that the presence of such a coupling increases the tension between the cosmic microwave background data from the analysis of the shift parameter in models with constant w(DE) and SNIa data for realistic values of the present dark matter density fraction. Thus, an independent measurement of the present dark matter density can place constraints on models with interacting dark energy.

Constraining the dark energy and smoothness parameter with type Ia supernovae and gamma-ray bursts

The existence of inhomogeneities in the observed Universe modifies the distance-redshift relations thereby affecting the results of cosmological tests in comparison to the ones derived assuming spatially uniform models. By modeling the inhomogeneities through a Zeldovich-Kantowski-Dyer-Roeder approach which is phenomenologically characterized by a smoothness parameter alpha, we rediscuss the constraints on the cosmic parameters based on type Ia supernovae (SNe Ia) and gamma-ray bursts (GRBs) data. The present analysis is restricted to a flat Lambda CDM model with the reasonable assumption that Lambda does not clump. A chi(2) analysis using 557 SNe Ia data from the Union2 compilation data (R. Amanullah et al., Astrophys. J. 716, 712 (2010).) constrains the pair of parameters (Omega(m), alpha) to Omega(m) = 0.27(-0.03)(+0.08) (2 sigma) and alpha >= 0.25. A similar analysis based only on 59 Hymnium GRBs (H. Wei, J. Cosmol. Astropart. Phys. 08 (2010) 020.) constrains the matter density parameter to be Omega(m) = 0.35(-0.24)(+0.62) (2 sigma) while all values for the smoothness parameter are allowed. By performing a joint analysis, it is found that Omega(m) = 0.27(-0.06)(+0.06) and alpha >= 0.52. As a general result, although considering that current GRB data alone cannot constrain the smoothness alpha parameter, our analysis provides an interesting cosmological probe for dark energy even in the presence of inhomogeneities.

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.

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.

Type Ia supernovae from violent mergers of carbon-oxygen white dwarfs: polarization signatures

The violent merger of two carbon-oxygen white dwarfs has been proposed as a viable progenitor for some Type Ia supernovae. However, it has been argued that the strong ejecta asymmetries produced by this model might be inconsistent with the low degree of polarization typically observed in Type Ia supernova explosions. Here, we test this claim by carrying out a spectropolarimetric analysis for the model proposed by Pakmor et al. for an explosion triggered during the merger of a 1.1 and 0.9 M⊙ carbon-oxygen white dwarf binary system. Owing to the asymmetries of the ejecta, the polarization signal varies significantly with viewing angle. We find that polarization levels for observers in the equatorial plane are modest (≲1 per cent) and show clear evidence for a dominant axis, as a consequence of the ejecta symmetry about the orbital plane. In contrast, orientations out of the plane are associated with higher degrees of polarization and departures from a dominant axis. While the particular model studied here gives a good match to highly polarized events such as SN 2004dt, it has difficulties in reproducing the low polarization levels commonly observed in normal Type Ia supernovae. Specifically, we find that significant asymmetries in the element distribution result in a wealth of strong polarization features that are not observed in the majority of currently available spectropolarimetric data of Type Ia supernovae. Future studies will map out the parameter space of the merger scenario to investigate if alternative models can provide better agreement with observations.

Searching for swept-up hydrogen and helium in the late-time spectra of 11 nearby Type Ia supernovae

The direct detection of a stellar system that explodes as a Type Ia supernova (SN Ia) has not yet been successful. Various indirect methods have been used to investigate SN Ia progenitor systems but none have produced conclusive results. A prediction of single-degenerate models is that H- (or He-) rich material from the envelope of the companion star should be swept up by the SN ejecta in the explosion. Seven SNe Ia have been analysed to date looking for signs of H-rich material in their late-time spectra and none were detected. We present results from new late-time spectra of 11 SNe Ia obtained at the Very Large Telescope using XShooter and FORS2. We present the tentative detection of Hα emission for SN 2013ct, corresponding to ∼0.007 M_⊙ of stripped/ablated companion star material (under the assumptions of the spectral modelling). This mass is significantly lower than expected for single-degenerate scenarios, suggesting that >0.1 M_⊙ of H-rich is present but not observed. We do not detect Hα emission in the other 10 SNe Ia. This brings the total sample of normal SNe Ia with non-detections (<0.001–0.058 M_⊙) of H-rich material to 17 events. The simplest explanation for these non-detections is that these objects did not result from the explosion of a CO white dwarf accreting matter from a H-rich companion star via Roche lobe overflow or symbiotic channels. However, further spectral modelling is needed to confirm this. We also find no evidence of He-emission features, but models with He-rich companion stars are not available to place mass limits.

TESTING THE DISTANCE-DUALITY RELATION WITH GALAXY CLUSTERS AND TYPE Ia SUPERNOVAE

In this Letter, we propose a new and model-independent cosmological test for the distance-duality (DD) relation, eta = D(L)(z)(1 + z)(-2)/D(A)(z) = 1, where D(L) and D(A) are, respectively, the luminosity and angular diameter distances. For D(L) we consider two sub-samples of Type Ia supernovae (SNe Ia) taken from Constitution data whereas D(A) distances are provided by two samples of galaxy clusters compiled by De Filippis et al. and Bonamente et al. by combining Sunyaev-Zeldovich effect and X-ray surface brightness. The SNe Ia redshifts of each sub-sample were carefully chosen to coincide with the ones of the associated galaxy cluster sample (Delta z < 0.005), thereby allowing a direct test of the DD relation. Since for very low redshifts, D(A)(z) approximate to D(L)(z), we have tested the DD relation by assuming that. is a function of the redshift parameterized by two different expressions: eta(z) = 1 + eta(0)z and eta(z) = 1 +eta(0)z/(1 + z), where eta(0) is a constant parameter quantifying a possible departure from the strict validity of the reciprocity relation (eta(0) = 0). In the best scenario (linear parameterization), we obtain eta(0) = -0.28(-0.44)(+0.44) (2 sigma, statistical + systematic errors) for the De Filippis et al. sample (elliptical geometry), a result only marginally compatible with the DD relation. However, for the Bonamente et al. sample (spherical geometry) the constraint is eta(0) = -0.42(-0.34)(+0.34) (3 sigma, statistical + systematic errors), which is clearly incompatible with the duality-distance relation.

Kinematic constraints to the transition redshift from supernovae type Ia union data

The kinematic approach to cosmological tests provides direct evidence to the present accelerating stage of the Universe that does not depend on the validity of general relativity, as well as on the matter-energy content of the Universe. In this context, we consider here a linear two-parameter expansion for the decelerating parameter, q(z)=q(0)+q(1)z, where q(0) and q(1) are arbitrary constants to be constrained by the union supernovae data. By assuming a flat Universe we find that the best fit to the pair of free parameters is (q(0),q(1))=(-0.73,1.5) whereas the transition redshift is z(t)=0.49(-0.07)(+0.14)(1 sigma) +0.54-0.12(2 sigma). This kinematic result is in agreement with some independent analyses and more easily accommodates many dynamical flat models (like Lambda CDM).

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.

Rôle des topoisomérases de type IA dans la ségrégation des chromosomes chez Escherichia coli

Les topoisomérases I (topA) et III (topB) sont les deux topoisomérases (topos) de type IA d’Escherichia coli. La fonction principale de la topo I est la relaxation de l’excès de surenroulement négatif, tandis que peu d’information est disponible sur le rôle de la topo III. Les cellules pour lesquelles les deux topoisomérases de type IA sont manquantes souffrent d’une croissance difficile ainsi que de défauts de ségrégation sévères. Nous démontrons que ces problèmes sont majoritairement attribuables à des mutations dans la gyrase qui empêchent l’accumulation d’excès de surenroulement négatif chez les mutants sans topA. L’augmentation de l’activité de la gyrase réalisée par le remplacement de l’allèle gyrB(Ts) par le gène de type sauvage ou par l’exposition des souches gyrB(Ts) à une température permissive, permet la correction significative de la croissance et de la ségrégation des cellules topos de type IA. Nous démontrons également que les mutants topB sont hypersensibles à l’inhibition de la gyrase par la novobiocine. La réplication non-régulée en l’absence de topA et de rnhA (RNase HI) augmente la nécessité de l’activité de la topoisomérase III. De plus, en l’absence de topA et de rnhA, la surproduction de la topoisomérase III permet de réduire la dégradation importante d’ADN qui est observée en l’absence de recA (RecA). Nous proposons un rôle pour la topoisomérase III dans la ségrégation des chromosomes lorsque l’activité de la gyrase n’est pas optimale, par la réduction des collisions fourches de réplication s’observant particulièrement en l’absence de la topo I et de la RNase HI.

Genetic studies on the role of type IA DNA topoisomerases in DNA metabolism and genome maintenance in Escherichia coli

Le surenroulement de l’ADN est important pour tous les processus cellulaires qui requièrent la séparation des brins de l’ADN. Il est régulé par l’activité enzymatique des topoisomérases. La gyrase (gyrA et gyrB) utilise l’ATP pour introduire des supertours négatifs dans l’ADN, alors que la topoisomérase I (topA) et la topoisomérase IV (parC et parE) les éliminent. Les cellules déficientes pour la topoisomérase I sont viables si elles ont des mutations compensatoires dans un des gènes codant pour une sous-unité de la gyrase. Ces mutations réduisent le niveau de surenroulement négatif du chromosome et permettent la croissance bactérienne. Une de ces mutations engendre la production d'une gyrase thermosensible. L’activité de surenroulement de la gyrase en absence de la topoisomérase I cause l’accumulation d’ADN hyper-surenroulé négativement à cause de la formation de R-loops. La surproduction de la RNase HI (rnhA), une enzyme qui dégrade l’ARN des R-loops, permet de prévenir l’accumulation d’un excès de surenroulement négatif. En absence de RNase HI, des R-loops sont aussi formés et peuvent être utilisés pour déclencher la réplication de l’ADN indépendamment du système normal oriC/DnaA, un phénomène connu sous le nom de « constitutive stable DNA replication » (cSDR). Pour mieux comprendre le lien entre la formation de R-loops et l’excès de surenroulement négatif, nous avons construit un mutant conditionnel topA rnhA gyrB(Ts) avec l’expression inductible de la RNase HI à partir d’un plasmide. Nous avons trouvé que l’ADN des cellules de ce mutant était excessivement relâché au lieu d'être hypersurenroulé négativement en conditions de pénurie de RNase HI. La relaxation de l’ADN a été montrée comme étant indépendante de l'activité de la topoisomérase IV. Les cellules du triple mutant topA rnhA gyrB(Ts) forment de très longs filaments remplis d’ADN, montrant ainsi un défaut de ségrégation des chromosomes. La surproduction de la topoisomérase III (topB), une enzyme qui peut effectuer la décaténation de l’ADN, a corrigé les problèmes de ségrégation sans toutefois restaurer le niveau de surenroulement de l’ADN. Nous avons constaté que des extraits protéiques du mutant topA rnhA gyrB(Ts) pouvaient inhiber l’activité de surenroulement négatif de la gyrase dans des extraits d’une souche sauvage, suggérant ainsi que la pénurie de RNase HI avait déclenché une réponse cellulaire d’inhibition de cette activité de la gyrase. De plus, des expériences in vivo et in vitro ont montré qu’en absence de RNase HI, l’activité ATP-dépendante de surenroulement négatif de la gyrase était inhibée, alors que l’activité ATP-indépendante de cette enzyme demeurait intacte. Des suppresseurs extragéniques du défaut de croissance du triple mutant topA rnhA gyrB(Ts) qui corrigent également les problèmes de surenroulement et de ségrégation des chromosomes ont pour la plupart été cartographiés dans des gènes impliqués dans la réplication de l’ADN, le métabolisme des R-loops, ou la formation de fimbriae. La deuxième partie de ce projet avait pour but de comprendre les rôles des topoisomérases de type IA (topoisomérase I et topoisomérase III) dans la ségrégation et la stabilité du génome de Escherichia coli. Pour étudier ces rôles, nous avons utilisé des approches de génétique combinées avec la cytométrie en flux, l’analyse de type Western blot et la microscopie. Nous avons constaté que le phénotype Par- et les défauts de ségrégation des chromosomes d’un mutant gyrB(Ts) avaient été corrigés en inactivant topA, mais uniquement en présence du gène topB. En outre, nous avons démontré que la surproduction de la topoisomérase III pouvait corriger le phénotype Par- du mutant gyrB(Ts) sans toutefois corriger les défauts de croissance de ce dernier. La surproduction de topoisomérase IV, enzyme responsable de la décaténation des chromosomes chez E. coli, ne pouvait pas remplacer la topoisomérase III. Nos résultats suggèrent que les topoisomérases de type IA jouent un rôle important dans la ségrégation des chromosomes lorsque la gyrase est inefficace. Pour étudier le rôle des topoisomérases de type IA dans la stabilité du génome, la troisième partie du projet, nous avons utilisé des approches génétiques combinées avec des tests de « spot » et la microscopie. Nous avons constaté que les cellules déficientes en topoisomérase I avaient des défauts de ségrégation de chromosomes et de croissance liés à un excès de surenroulement négatif, et que ces défauts pouvaient être corrigés en inactivant recQ, recA ou par la surproduction de la topoisomérase III. Le suppresseur extragénique oriC15::aph isolé dans la première partie du projet pouvait également corriger ces problèmes. Les cellules déficientes en topoisomérases de type IA formaient des très longs filaments remplis d’ADN d’apparence diffuse et réparti inégalement dans la cellule. Ces phénotypes pouvaient être partiellement corrigés par la surproduction de la RNase HI ou en inactivant recA, ou encore par des suppresseurs isolés dans la première partie du projet et impliques dans le cSDR (dnaT18::aph et rne59::aph). Donc, dans E. coli, les topoisomérases de type IA jouent un rôle dans la stabilité du génome en inhibant la réplication inappropriée à partir de oriC et de R-loops, et en empêchant les défauts de ségrégation liés à la recombinaison RecA-dépendante, par leur action avec RecQ. Les travaux rapportés ici révèlent que la réplication inappropriée et dérégulée est une source majeure de l’instabilité génomique. Empêcher la réplication inappropriée permet la ségrégation des chromosomes et le maintien d’un génome stable. La RNase HI et les topoisomérases de type IA jouent un rôle majeur dans la prévention de la réplication inappropriée. La RNase HI réalise cette tâche en modulant l’activité de surenroulement ATP-dependante de la gyrase, et en empêchant la réplication à partir des R-loops. Les topoisomérases de type IA assurent le maintien de la stabilité du génome en empêchant la réplication inappropriée à partir de oriC et des R-loops et en agissant avec RecQ pour résoudre des intermédiaires de recombinaison RecA-dépendants afin de permettre la ségrégation des chromosomes.

Analysis of BMP signalling through the receptor type IA in embryogenesis using conditional gene inactivation in mice

Although bone morphogenetic proteins (BMPs) were initially identified for their potent bone-inducing activity, their precise roles in processes of endochondral and intramembranous bone formation are far from being clear. Tissue-specific loss-of-function experiments using the BMP receptor type IA (BMPR-IA) are particularly attractive since this receptor is thought to be essential for signaling by the closely related BMPs -2, 4, and 7. To ablate signaling through this receptor during chondrogenesis, we have generated transgenic mice expressing Cre recombinase under the control of the collagen type II (Col2a1) gene regulatory sequences. Mice lacking BMPR-IA function in chondrocytes display a number of skeletal abnormalities, including defects in bones of the chondrocranium, abnormal dorsal vertebral processes, scapulae with severe hypoplasia of dorsal elements, and shortening of the long bones. Alterations in the growth plate of long bones in mutants suggest that BMPR-IA is not required for early steps of the chondrocyte specification, but is rather important in regulation of terminal differentiation. Molecular analysis revealed noticeable downregulation of the Ihh/Ptch signalling pathway, decreased chondrocyte proliferation rate and deregulation of hypertrophy. ^ In order to elucidate the role of BMP signalling in development of the limb and intramembranous ossification, we have used mice expressing Cre recombinase under control of the Prx1 (MHox) regulatory elements (M. Logan, pers comm.). Cre activity was found in those mice in the developing limb bud mesenchyme, as well as in a subset of cranial neural crest cells. Prx1-Cre-induced conditional mutants display prominent defects in distal limb outgrowth, as well as ossification defects in a number of neural crest-derived calvarial bones. Intriguingly, mutant limbs displayed alterations in patterning along all three axes. Molecular analysis revealed ectopic anterior Shh/Ptch signalling pathway activation and expression of some Hox genes. Observed loss of Msx1 and Msx2 expression in the progress zone correlates with downregulation of Cyclin D1 and decreased distal outgrowth. Abnormal ventral localization of Lmx1b-expressing cells along with observed later morphological abnormalities suggest a novel role for BMP signalling in establishment or maintaining of the dorso-ventral polarity in the limb mesoderm. ^