Radio modelling of the brightest and most luminous non-thermal colliding-wind binary Apep

Stars and planetary system

Radio modelling of the brightest and most luminous non-thermal colliding-wind binary Apep

Stars and planetary system

Evolutionary-enhanced quantum supervised learning model

Quantum supervised learning, utilizing variational circuits, stands out as a promising technology for NISQ devices due to its efficiency in hardware resource utilization during the creation of quantum feature maps and the implementation of hardware-efficient ansatz with trainable parameters. Despite these advantages, the training of quantum models encounters challenges, notably the barren plateau phenomenon, leading to stagnation in learning during optimization iterations. This study proposes an innovative approach: an evolutionary-enhanced ansatz-free supervised learning model. In contrast to parametrized circuits, our model employs circuits with variable topology that evolves through an elitist method, mitigating the barren plateau issue. Additionally, we introduce a novel concept, the superposition of multi-hot encodings, facilitating the treatment of multi-classification problems. Our framework successfully avoids barren plateaus, resulting in enhanced model accuracy. Comparative analysis with variational quantum classifiers from the technology's state-of-the-art reveal a substantial improvement in training efficiency and precision. Furthermore, we conduct tests on a challenging dataset class, traditionally problematic for conventional kernel machines, demonstrating a potential alternative path for achieving quantum advantage in supervised learning for NISQ era

A review of phytic acid sources, obtention, and applications

Phytic acid (PA), extracted from oilseeds, legumes, cereals, nuts, and pollen by acid solutions under heating and/or stirring and then purified, has shown beneficial health and physiological effects due to its pronounced antioxidant activity and ability to chelate Fe3+ ions. Publications on PA have increased, especially the ones reporting its effect on disease prevention and treatment. Moreover, recent studies have suggested the PA efficacy as a foodborne pathogens inhibitor. Therefore, due to its countless proven properties, phytic acid has gained greater attention than its common classification as just an antinutrient. Past and current studies have been reviewed to provide an overview on PA structure, sources, biosynthesis, extraction, purification, and applications.The authors would like to thank the financial support of CNPq, CAPES (finance code 001) and Fundação Araucária (project code 3462014). Joana S. Amaral is thankful to the Foundation for Science and Technology (FCT, Portugal) for their financial support by national funds FCT/MCTES to CIMO (UIDB/00690/2020).This work was supported by the CNPq; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior [001]; Fundação Araucária [3462014]; Foundation for Science and Technology [UIDB/00690/2020].info:eu-repo/semantics/publishedVersio

Comparing hypervelocity star populations from the Large Magellanic Cloud and the Milky Way

Galaxie

Ensino de Ciências e Matemática: elementos didáticos para teoria e experimentação

O livro Ensino de Ciências e Matemática — elementos didáticos para teoria e experimentação visa ser um referencial para professores e estudantes destas duas áreas do conhecimento pautado na ideia da busca de novas práticas pedagógicas para o desenvolvimento de competências por meio da aprendizagem dialógica, cuja base é o correto trabalho da teoria e da experimentação — elementos norteadores do pensamento científico. Seu conteúdo é resultante de notas de aula da Especialização em Ensino de Ciências e Matemática ofertada por docentes da Universidade Federal da Integração Latino-Americana (UNILA) como curso de formação continuada (Comfor/MEC) para professores da educação básica no Oeste do Paraná

Phytic acid against clostridium perfringens type a: a food matrix study

This study evaluated the inhibitory effect of phytic acid (PA) on the spore germination and vegetative cells growth of Clostridium perfringens type A, as well as its effect in combination with maltodextrin (MD) in cooked sausages. The addition of 1% PA showed a satisfactory inhibition of spores’ germination and vegetative cells growth of C. perfringens in BHI media. The inhibitory effect of 1% PA on vegetative cells was similar to the additive sodium sorbate (SS) at 10%. Subsequently, a mixture of PA-MD (1:1; w/w) was evaluated for the inhibition of C. perfringens spores in cooked sausages. The PA-MD 1.5% and 2.5% had a similar performance to SS 10% and a similar or higher performance than 0.015% NO2 (p < 0.05). In an unprecedented way, the present study demonstrated that PA inhibited spore germination and vegetative cells growth of C. perfringens, highlighting its potential use as an alternative and natural preservative for the meat industry.This research was financed in part by the Coordenação de Aperfeiçoamento de Pessoal de Nível Superior-Brazil (CAPES)-Finance Code 001, Conselho Nacional de Desenvolvimento Científico e Tecnológico-Brazil (CNPq), and Fundação Araucária-Brazil-Programa Universal Pesquisa Básica e Aplicada (Edital 05/2011, Agreement 346/2014). J.S. Amaral is grateful to the Foundation for Science and Technology (FCT, Portugal) for financial support by national funds FCT/MCTES to CIMO (UIDB/00690/2020).info:eu-repo/semantics/publishedVersio

V-LoTSS: The circularly polarised LOFAR Two-metre Sky Survey

We present the detection of 68 sources from the most sensitive radio survey in circular polarisation conducted to date. We used the second data release of the 144 MHz LOFAR Two-metre Sky Survey to produce circularly polarised maps with a median noise of 140 µJy beam−1 and resolution of 20″ for ≈27% of the northern sky (5634 deg2). The leakage of total intensity into circular polarisation is measured to be ≈0.06%, and our survey is complete at flux densities ≥1 mJy. A detection is considered reliable when the circularly polarised fraction exceeds 1%. We find the population of circularly polarised sources is composed of four distinct classes: stellar systems, pulsars, active galactic nuclei, and sources unidentified in the literature. The stellar systems can be further separated into chromospherically active stars, M dwarfs, and brown dwarfs. Based on the circularly polarised fraction and lack of an optical counterpart, we show it is possible to infer whether the unidentified sources are likely unknown pulsars or brown dwarfs. By the completion of this survey of the northern sky, we expect to detect 300±100 circularly polarised sources

Exoplanet interior retrievals:core masses and metallicities from atmospheric abundances

The mass and distribution of metals in the interiors of exoplanets are essential for constraining their formation and evolution processes. Never the less, with only masses and radii measured, the determination of exoplanet interior structures is degenerate, and so far simplified assumptions have mostly been used to derive planetary metallicities. In this work, we present a method based on a state-of-The-Art interior code, recently used for Jupiter, and a Bayesian framework, to explore the possibility of retrieving the interior structure of exoplanets. We use masses, radii, equilibrium temperatures, and measured atmospheric metallicities to retrieve planetary bulk metallicities and core masses. Following results on the giant planets in the Solar system and recent development in planet formation, we implement two interior structure models: one with a homogeneous envelope and one with an inhomogeneous one. Our method is first evaluated using a test planet and then applied to a sample of 37 giant exoplanets with observed atmospheric metallicities from the pre-JWST era. Although neither internal structure model is preferred with the current data, it is possible to obtain information on the interior properties of the planets, such as the core mass, through atmospheric measurements in both cases. We present updated metal mass fractions, in agreement with recent results on giant planets in the Solar system.</p