The angular scale of homogeneity with SDSS-IV DR16 Luminous Red Galaxies

We report measurements of the angular scale of cosmic homogeneity ($\theta_{H}$) using the recently released luminous red galaxy sample of the sixteenth data release of the Sloan Digital Sky Survey (SDSS-IV LRG DR16). It consists of a model-independent method, as we only use the celestial coordinates of these objects to carry out such an analysis. The observational data is divided into thin redshift bins, namely $0.67<z<0.68$, $0.70<z<0.71$, and $0.73<z<0.74$, in order to avoid projection biases, and we estimate our uncertainties through a bootstrap method and a suite of mock catalogues. We find that the LRGs exhibit an angular scale of homogeneity consistent with the predictions of the standard cosmology within the redshift interval studied. Considering the bootstrap method, in which the measurements are obtained in a model-independent way, we found at 1$\sigma$ level that $\theta_H^{boot}(0.675) = 7.57 \pm 2.91$ deg, $\theta_H^{boot} (0.705) = 7.49 \pm 2.63$ deg and $\theta_H^{boot} (0.735) = 8.88 \pm 2.81$ deg. Such results are in good agreement with the ones obtained using mock catalogues built under the assumption of the standard cosmological model.Comment: 13 pages, 4 figures, 3 tables. References updated; matches version published in JCA

Cosmological model-independent constraints on the baryon fraction in the IGM from fast radio bursts and supernovae data

Fast Radio Bursts (FRBs) are millisecond-duration radio transients with an observed dispersion measure ($DM$) greater than the expected Milky Way contribution, which suggests that such events are of extragalactic origin. Although some models have been proposed to explain the physics of the pulse, the mechanism behind the FRBs emission is still unknown. From FRBs data with known host galaxies, the redshift is directly measured and can be combined with estimates of the $DM$ to constrain the cosmological parameters, such as the baryon number density and the Hubble constant. However, the poor knowledge of the fraction of baryonic mass in the intergalactic medium ($f_{IGM}$) and its degeneracy with the cosmological parameters impose limits on the cosmological application of FRBs. In this work we present a cosmological model-independent method to determine the evolution of $f_{IGM}$ combining the latest FRBs observations with localized host galaxy and current supernovae data. We consider constant and time-dependent $f_{IGM}$ parameterizations and show, through a Bayesian model selection analysis, that a conclusive answer about the time-evolution of $f_{IGM}$ depend strongly on the $DM$ fluctuations due to the spatial variation in cosmic electron density ($\delta$). In particular, our analysis show that the evidence varies from strong (in favor of a growing evolution of $f_{IGM}$ with redshift) to inconclusive, as larger values of $\delta$ are considered.Comment: 8 pages, 3 figure

Forecasting constraints on the baryon mass fraction in the IGM from fast radio bursts and type Ia supernovae

Fast Radio Bursts (FRBs) are transient events with a high energy and short duration in the radio frequency. By identifying the origin of the pulse, it is possible to measure the redshift of the host galaxy, which can be used to constrain cosmological and astrophysical parameters and test aspects of fundamental physics when combined with the observed dispersion measure ($DM$). However, some factors limit the application of FRBs in cosmology: (i) the current poor modelling of the fluctuations in the $DM$ due to spatial variation in the cosmic electrons density; (ii) the fact that the fraction of baryon mass in the intergalactic medium ($f_{IGM}$) is degenerated with some cosmological parameters; (iii) the limited current knowledge about host galaxy contribution ($DM_{host}$). In this work, we investigate the impact of different redshift distribution models of FRBs to constrain the baryon fraction in the IGM and host galaxy contribution. We use a cosmological model-independent method developed in previous work \cite{Lemos2023} to perform the analysis and combine simulated FRB data from Monte Carlo simulation and supernovae data. Since the physical mechanism responsible for the burst is still unknown, we assume four distribution models for the FRBs, namely gamma-ray bursts (GRB), star formation rate (SFR), uniform and equidistant (ED). Also, we consider samples with $N = 15$, 30, 100 and 500 points and three different values of the fluctuations of electron density in the $DM$, $\delta = 0, 10, 100$ pc/cm$^{3}$. Our analysis shows that the GRB, SFR and Uniform distribution models present consistent results within $2\sigma$ for the free parameters $f_{IGM}$ and $DM_{host,0}$ and highlights the crucial role of $DM$ fluctuations in obtaining more precise measurements.Comment: 9 pages, 2 figure

Digital transformation : construct definition challenges and scenarios for a research agenda

Indeed, digital transformation is just like the new models of the various technological devices (smartphones, tablets, smart watches) that are used without us fully mastering their resources. It is happening in an accelerated way without even having a clear understanding of the phenomenon. It is typically a situation in which reality occurs at a speed greater than its understanding, thus claiming the researchers' positioning in the face of digital contemporaneity. Just like Uber, that initially imposed itself as a “de facto” reality (in practice) before becoming a de jure standard (supported by law), the research agenda digital transformation seeks to guide the future of research in the field, but, due to the speed of changes, it may fit into the metaphor of the lantern on the ship's stern, helping to illuminate the past. Even though the organizational practice is more agile than the academy, it is still worth emphasizing the fundamental role of research in interpreting the nuances of the phenomenon through the most diverse perspectives..info:eu-repo/semantics/publishedVersio

Methodology evaluation of pin microrelief meter

The effects of natural weathering and different managements performed in agriculture may best be understood by studying the soil roughness. The aim of this study was to evaluate the optimization of the use of pin microrelief meter, an instrument used to determine the soil surface roughness, as the number of readings collected over traditional methodology proposed in the bibliography. The study was conducted in Rio Paranaiba (MG), in a Haplustox soil. The experimental design was completely randomized in a 2×3 factorial design with four replications. There were combined two types of primary tillage: conventional tillage with disc plow (PCAD) and harrow (PCGA), and three amounts of readings (100, 200, and 300 reading points) sampled in each experimental unit. Independently of the soil tillage, disc plow and harrow, the collection of 100 readings using a pin microrelief meter of a square meter, was sufficient to determine the surface roughness before and after soil preparation, without accuracy loss compared with the traditional method

Can the angular scale of cosmic homogeneity be used as a cosmological test?

In standard cosmology, the cosmic homogeneity scale is the transition scale above which the patterns arising from non-uniformities -- such as groups and clusters of galaxies, voids, and filaments -- become indistinguishable from a random distribution of sources. Recently, different groups have investigated the feasibility of using such a scale as a cosmological test and arrived at different conclusions. In this paper, we complement and extend these studies by exploring the evolution of the spatial (${\cal{R}}_H$) and angular ($\theta_H$) homogeneity scales with redshift, assuming a spatially flat, $\Lambda$-Cold Dark Matter %($\Lambda$CDM) universe and linear cosmological perturbation theory. We confirm previous results concerning the non-monotonicity of ${\cal{R}}_H$ with the matter density parameter $\Omega_{m0}$ but also show that it exhibits a monotonical behavior with the Hubble constant $H_0$ within a large redshift interval. More importantly, we find that, for $z \gtrsim 0.6$, the angular homogeneity scale not only presents a monotonical behavior with $\Omega_{m0}$ and $H_0$ but is quite sensitive to $H_0$, especially at higher redshifts. These results, therefore, raise the possibility of using $\theta_H$ as a new, model-independent way to constrain cosmological parameters.Comment: 10 pages, 24 figure

Evaluation of the Academia da Cidade program to promote physical activity in Recife, Pernambuco State, Brazil: perceptions of users and non-users

O objetivo foi descrever usuários e não-usuários do Programa Academia da Cidade de Recife, Pernambuco, Brasil. Foram selecionados quatro dos 19 pólos do programa. Para cada usuário sorteado, foi selecionado um não-usuário, que foi pareado ao usuário em termos de sexo, idade (±5 anos) e local de residência. A amostra foi composta por 277 usuários e 277 não-usuários. Entre os não-usuários, 22% referiram nunca ter ouvido falar do programa. Entre os que já ouviram falar do programa, 54,3% o conhecem por terem visto um pólo. Entre os usuários, o principal motivo para a participação no programa foi "melhorar a saúde"; o tempo médio de participação no programa foi de 27,5 meses (DP = 23,1) e 72,8% relataram grau elevado de satisfação. O percentual de pessoas com percepção de saúde regular ou ruim foi significativamente maior entre os não-usuários (45,4%) em comparação aos usuários (28,5%). Os usuários do Programa Academia da Cidade parecem estar satisfeitos. Estratégias de divulgação devem ser priorizadas para que o programa seja conhecido por um maior percentual de residentes de Recife.The aim of this study was to describe the profile of users and non-users of the Academia da Cidade Program to promote physical activity in Recife, Pernambuco State, Brazil. Four of the program's 19 units were sampled. Users (n=277) and non-users (n=277) were matched for gender, age (±5 years), and place of residence. Among non-users, 22% had never heard of the program. Among those who knew of the program, 54.3% learned about it by actually having seen one of the units. Among users, the main reason for participating in the program was to improve their health; mean participation time was 27.5 months (SD = 23.1); and 72.8% reported high satisfaction. The proportion of individuals with fair or poor self-rated health was significantly higher among non-users (45.4%) than users (28.5%). Users of the program appeared to be satisfied. Strategies to further publicize the program should be prioritized to make it known to a larger proportion of the city's population

Preoperative left ventricular ejection fraction and left atrium reverse remodeling after mitral regurgitation surgery

Background: Left atrium enlargement has been associated with cardiac events in patients with mitral regurgitation (MR). Left atrium reverse remodeling (LARR) occur after surgical correction of MR, but the preoperative predictors of this phenomenon are not well known. It is therefore important to identify preoperative predictors for postoperative LARR.Methods: We enrolled 62 patients with chronic severe MR (prolapse or flail leaflet) who underwent successful mitral valve surgery (repair or replacement); all with pre-and postoperative echocardiography. LARR was defined as a reduction in left atrium volume index (LAVI) of >= 25%. Stepwise multiple regression analysis was used to identify independent predictors of LARR.Results: LARR occurred in 46 patients (74.2%), with the mean LAVI decreasing from 85.5 mL/m(2) to 49.7 mL/m(2) (p = 25% with a sensitivity of 71.7% and a specificity of 56.3%.Conclusions: LARR occurs frequently after mitral valve surgery and is associated with preoperative LVEF higher than 63.5%.Inst Dante Pazzanese Cardiol, São Paulo, BrazilUniversidade Federal de São Paulo, Escola Paulista Med, São Paulo, BrazilDisciplina Cardiol, BR-04024002 São Paulo, BrazilUniversidade Federal de São Paulo, Escola Paulista Med, São Paulo, BrazilWeb of Scienc

Autenticación mediante DNA barcoding de especies de meros legalmente protegidas y en peligro de extinción, sometidas a explotación pesquera, incluyendo el mero Goliat Epinephelus itajara

Fishing strategies are constantly changing to meet the needs for new or alternative food sources. Consequently, management of fishing activities regarding rates of exploitation is essential, as a number of resources have reached situations of overexploitation. The aim of the present study was to use DNA barcoding from the goliath grouper and other exploited epinephelids in order to provide procedures for DNA authentication to be used as evidence for combating putative illegal fishing. The species studied were Epinephelus adscensionis, Mycteroperca bonaci, Mycteroperca interstitialis, Epinephelus itajara, Mycteroperca venenosa, Epinephelus mystacinus, Dermatolepis inermis, Alphestes afer, Cephalopholis fulva, Mycteroperca acutirostris, Rypticus saponaceus, Mycteroperca marginata and Epinephelus morio. Four of these species are the main epinephelids fished in the Atlantic Ocean. Differential patterns of polymerase chain reaction–restriction fragment length polymorphism were obtained from the species and additional single nucleotide polymorphisms were also detected among the four main epinephelids studied. The procedures proved very efficient and we suggest their applicability to the other fish groups as a way to control illegal capture and retail around the world, especially in cases in which filleting and other forms of de-characterization cause a lack of morpho-anatomical key characters.Las estrategias de pesca cambian constantemente para satisfacer las necesidades de fuentes de alimento nuevas o alternativas. En consecuencia, a medida que los recursos alcanzan situaciones de sobreexplotación, resulta esencial establecer procedimientos de inspección de las actividades relacionadas con las tasas de explotación pesquera. El objetivo de este estudio es proponer el uso de la técnica de DNA barcoding para establecer la verificación de la identidad del mero Goliat y otros epinefélidos, a fin de utilizarlo como evidencia para combatir la pesca ilegal cuando se sospeche su ocurrencia. Las especies aquí estudiadas fueron Alphestes afer, Cephalopholis fulva, Dermatolepis inermis, Epinephelus adscensionis, E. itajara, E. morio, E. mystacinus, Mycteroperca acutirostris, M. bonaci, M. interstitialis, M. marginata, M. venenosa y Rypticus saponaceus de las cuales cuatro constituyen las más pescadas en el Océano Atlántico. Fueron encontrados patrones diferenciables de PCR-RFLPs para todas las especies y, además, fue posible detectar SNPs adicionales entre las cuatro especies más explotadas. Los procedimientos aquí empleados fueron muy eficaces por lo que sugerimos su aplicabilidad a otros grupos de peces como medida de control de la captura y comercialización ilegal a nivel mundial, particularmente en aquellos casos en los que el fileteado y otras formas de procesamiento que alteran las características anatómicas y morfológicas impiden su identificación