54 research outputs found
Níveis de treonina digestível em dietas para fêmeas suínas lactantes de médio potencial genético
Metanálise da relação entre espessura de toicinho e variáveis nutricionais de porcas gestantes e lactantes
Níveis de treonina digestível em dietas para fêmeas suínas de alto potencial genético em lactação sob condições de alta temperatura ambiente Digestible threonine levels of high-producing lactating sows maintained under high temperature environment conditions
Foram utilizadas 52 fêmeas suínas em lactação distribuídas em delineamento experimental de blocos ao acaso, composto de quatro níveis de treonina digestível (0,64; 0,67; 0,70 e 0,73%) na dieta e 13 repetições, em que cada unidade experimental foi constituída por uma fêmea. A temperatura do ar no interior das salas foi de 29,7 ± 2,5ºC. Não houve efeito dos níveis de treonina digestível na dieta sobre o peso das fêmeas ao desmame. As perdas total e percentual de peso das fêmeas durante a lactação reduziram de forma linear com o aumento dos níveis de treonina digestível na dieta. Os níveis de treonina digestível influenciaram a espessura de toucinho (ET) ao desmame e afetaram as variações total e percentual de espessura de toucinho. As composições de gordura e proteína corporal à desmama não foram influenciadas pelos níveis de treonina digestível na dieta. Verificou-se redução linear das mobilizações total e percentual de gordura corporal conforme aumentaram os níveis de treonina digestível na dieta. A mobilização de proteína corporal, a produção de leite e o intervalo desmama-estro não foram influenciados pelos níveis de treonina digestível da dieta. Os níveis de treonina digestível não afetaram os consumos de ração, de lisina e de energia digestível. Contudo, verificou-se aumento linear do consumo de treonina digestível conforme aumentou o nível deste aminoácido na dieta. Os níveis de treonina digestível não influenciaram a eficiência energética das fêmeas e o desempenho dos leitões e das leitegadas. Fêmeas suínas de alto potencial genético em lactação sob condições de temperaturas ambientais elevadas exigem 0,73% de treonina digestível, correspondente ao consumo diário de 32,5 g e à relação treonina digestível:lisina digestível de 73%.<br>Fifty and two lactating sows were allotted to a randomized complete blocks experimental design with four digestible threonine levels (0.64; 0.67; 0.70 and 0.73%) and 13 replications, and each experimental unit was consisted by a female. The temperature inside in the room was of 29.7 ± 2.5°C. There was no effect of digestible threonine levels in the diet on the weight of the sows at weaning. The total and percentage sow weight losses linearly reduced with the increase of digestible threonine level in the diet during the lactation period. Digestible threonine level in the diets influenced fat thickness (FT) at weaning, and affected the total and percentage variation of FT. The compositions of fat and corporal protein at weaning were not influenced by digestible threonine levels in the diet. A linear reduction for total and percentage of corporal fat mobilizations was observed as digestible threonine levels increased in the diet. The mobilization of corporal protein, milk production and the interval weaning time-estrus were not influenced by digestible threonine levels in the diet. Digestible threonine leveld in the diet had no effect on intake of diet, of lysine and of digestible energy. However, a linear increase was observed for the intake of digestible threonine as the levels of it increased in the diet. Digestible threonine levels in the diet had not influenced the energy efficiency of the females, the performance of the piglets and the litters. High-producing lactating sows under high temperature environmental conditions require 0.73% of digestible threonine, corresponding to a daily intake of 32.5g and the digestible threonine:digestible lysine ratio of 73%
Do target and non-target ethnic group adolescents process advertisements differently?
Research on ethnic advertisements has identified attitudinal differences between target and non-target groups. However, investigators have largely failed to explain the reasons behind these differences. Accordingly, this study examines the process by which target and non-target group adolescents build attitudes towards ethnically focused advertisements. The Elaboration Likelihood Model and Dual Mediation Hypothesis models are used as theoretical and operational frameworks. This study uses a modified DMH model that incorporates ethnic identity strength and self-reference as important antecedents of ad attitude and ad cognition in the context of ethnic advertising. The data are analysed with the help of structural equation modelling procedures. The results suggest that non-target ethnic group adolescents generally process advertisements in a peripheral manner, whereas target ethnic group adolescents tend to engage in both central and peripheral processing. More importantly, for both majority and minority groups, the strength of subjects’ ethnic identity and self-reference impact their response to ethnic advertisements when the advertisement is compatible with their ethnic background
Missing Components in ΛCDM from DESI Y1 BAO Measurements: Insights from Redshift Remapping
International audienceWe explore transformations of the Friedman-Lemaître-Robertson-Walker (FLRW) metric and cosmological parameters that align with observational data, aiming to gain insights into potential extensions of standard cosmological models. We modify the FLRW metric by introducing a scaling factor, (the cosmological scaling function, CSF), which alters the standard relationship between cosmological redshift and the cosmic scale factor without affecting angular measurements or Cosmic Microwave Background (CMB) anisotropies. Using data from DESI Year 1, Pantheon+ supernovae, and the Planck CMB temperature power spectrum, we constrain both the CSF and cosmological parameters through a Markov Chain Monte Carlo approach. Our results indicate that the CSF model fits observational data with a lower Hubble constant (although it is compatible with the value given by Planck 2018 within 1) and is predominantly dark-matter-dominated. Additionally, the CSF model produces temperature and lensing power spectra similar to those predicted by the standard model, though with lower values in the CSF model at large scales. We have also checked that when fitting a CSF model without dark energy to the data, we obtain a more negative conformal function. This suggests that the CSF model may offer hints about missing elements and opens up a new avenue for exploring physical interpretations of cosmic acceleration
DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics
International audienceWe present the samples of galaxies and quasars used for DESI 2024 cosmological analyses, drawn from the DESI Data Release 1 (DR1). We describe the construction of large-scale structure (LSS) catalogs from these samples, which include matched sets of synthetic reference `randoms' and weights that account for variations in the observed density of the samples due to experimental design and varying instrument performance. We detail how we correct for variations in observational completeness, the input `target' densities due to imaging systematics, and the ability to confidently measure redshifts from DESI spectra. We then summarize how remaining uncertainties in the corrections can be translated to systematic uncertainties for particular analyses. We describe the weights added to maximize the signal-to-noise of DESI DR1 2-point clustering measurements. We detail measurement pipelines applied to the LSS catalogs that obtain 2-point clustering measurements in configuration and Fourier space. The resulting 2-point measurements depend on window functions and normalization constraints particular to each sample, and we present the corrections required to match models to the data. We compare the configuration- and Fourier-space 2-point clustering of the data samples to that recovered from simulations of DESI DR1 and find they are, generally, in statistical agreement to within 2% in the inferred real-space over-density field. The LSS catalogs, 2-point measurements, and their covariance matrices will be released publicly with DESI DR1
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