IMPACT OF PHYSICAL EXERCISE ON PSYCHOLOGICAL WELL-BEING AND PSYCHIATRIC DISORDERS

Background: Physical exercise is one of the major features of human health, as it is involved in several physiological processes and related to major benefits in reducing body fat, myocardial infarction, hypertension and insulin resistance risk. Physical exercise also plays a positive role in achieving psychological well-being that can be defined as a state of happiness and serenity, with low levels of distress, overall good physical and mental health and outlook and a good quality of life. Aim of the paper: To review the positive effects of physical activity on psychological well-being and its possible neurobiological underpinnings, as well as its impact on several neuropsychiatric disorders, such as depression, anxiety, eating disorders, obsessive-compulsive disorder, post-traumatic stress disorder, attention-deficit/hyperactivity disorder, autism spectrum disorders, schizophrenia and some neurodegenerative disorders such as Alzheimer’s and Parkinson’s disease. Methods: The PubMed, Scopus, Embase, PsycINFO and Google Scholar databases were searched for full text articles published in the latest thirty years on the benefits that physical activity exerts on psychological well-being. Objectives: This study aims to identify the common and differential elements of the DLD (SLI) and LD through a quantitative and qualitative analysis. Results: An impressive amount of data support the positive role of physical activity on psychological well-being and a large amount of research has focused on its beneficial effects in improving the symptoms of the main neuropsychiatric disorders, while highlighting its usefulness as an adjuvant option to psychopharmacological treatments and psychotherapy. In particular, exercise would deeply affect CNS morphology and function, through heterogeneous mechanisms including, amongst the others, the production of hormones, neurotransmitters and neurotrophins, the promotion of angiogenesis and neuroplasticity, and the regulation of gene expression. Conclusion: Literature indicates that the promotion of physical activity may work like an adjunctive and/or augmentation strategy to enhance drugs or psychological treatments, or even as an alternative option in major depression

Standards in semen examination:publishing reproducible and reliable data based on high-quality methodology

Biomedical science is rapidly developing in terms of more transparency, openness and reproducibility of scientific publications. This is even more important for all studies that are based on results from basic semen examination. Recently two concordant documents have been published: the 6th edition of the WHO Laboratory Manual for the Examination and Processing of Human Semen, and the International Standard ISO 23162:2021. With these tools, we propose that authors should be instructed to follow these laboratory methods in order to publish studies in peer-reviewed journals, preferable by using a checklist as suggested in an Appendix to this article.Peer reviewe

Tracking the X-ray Polarization of the Black Hole Transient Swift J1727.8-1613 during a State Transition

We report on a campaign on the bright black hole X-ray binary Swift J1727.8$-$1613 centered around five observations by the Imaging X-ray Polarimetry Explorer (IXPE). This is the first time it has been possible to trace the evolution of the X-ray polarization of a black hole X-ray binary across a hard to soft state transition. The 2--8 keV polarization degree slowly decreased from $\sim$4\% to $\sim$3\% across the five observations, but remained in the North-South direction throughout. Using the Australia Telescope Compact Array (ATCA), we measure the intrinsic 7.25 GHz radio polarization to align in the same direction. Assuming the radio polarization aligns with the jet direction (which can be tested in the future with resolved jet images), this implies that the X-ray corona is extended in the disk plane, rather than along the jet axis, for the entire hard intermediate state. This in turn implies that the long ($\gtrsim$10 ms) soft lags that we measure with the Neutron star Interior Composition ExploreR (NICER) are dominated by processes other than pure light-crossing delays. Moreover, we find that the evolution of the soft lag amplitude with spectral state differs from the common trend seen for other sources, implying that Swift J1727.8$-$1613 is a member of a hitherto under-sampled sub-population.Comment: Submitted to ApJ. 20 pages, 8 figure

SARS-CoV-2 susceptibility and COVID-19 disease severity are associated with genetic variants affecting gene expression in a variety of tissues

Variability in SARS-CoV-2 susceptibility and COVID-19 disease severity between individuals is partly due to genetic factors. Here, we identify 4 genomic loci with suggestive associations for SARS-CoV-2 susceptibility and 19 for COVID-19 disease severity. Four of these 23 loci likely have an ethnicity-specific component. Genome-wide association study (GWAS) signals in 11 loci colocalize with expression quantitative trait loci (eQTLs) associated with the expression of 20 genes in 62 tissues/cell types (range: 1:43 tissues/gene), including lung, brain, heart, muscle, and skin as well as the digestive system and immune system. We perform genetic fine mapping to compute 99% credible SNP sets, which identify 10 GWAS loci that have eight or fewer SNPs in the credible set, including three loci with one single likely causal SNP. Our study suggests that the diverse symptoms and disease severity of COVID-19 observed between individuals is associated with variants across the genome, affecting gene expression levels in a wide variety of tissue types

Crecer en familia hoy: El desafío de la pluralidad.

¿Qué es lo que entendemos por familia hoy en día y qué contribuye a formarla? En otras palabras, ¿qué es lo que hace familia en la actualidad? En diciembre del 2018, una veintena de profesionales de la educación provenientes de cuatro países (España, Francia, Italia y Rumanía) se reunieron en Barcelona durante una semana para compartir con los investigadores una serie de actividades y aprendizajes en torno a esta cuestión. Fue el comienzo de una prolongada y compleja investigación llevada a cabo por un grupo multilingüe, multiprofesional e interdisciplinario cuyo resultado es esta primera producción intelectual. ¿Qué transformaciones están experimentando las familias? ¿Cómo han cambiado los modelos familiares en los últimos cincuenta años? ¿Cuáles son los principales retos a los que se enfrentan las familias y los profesionales que las acompañan? Las preguntas aquí planteadas no tratan de moldear una nueva definición de familia; más bien, se centran en el proceso de “crecer en familia” para saber qué lugar ocupan los niños y las niñas en la vida familiar y comunitaria. A pesar de que es posible identificar tendencias transversales a nivel europeo, es en la pluralidad donde hemos identificado el principal desafío. La diversificación de los modelos familiares, la multiplicidad legislativa en la que se basa el derecho de familia y los procesos de acompañamiento, que implican una constelación de actores y vulnerabilidades, constituyen la base sobre la que se cimienta esta pluralidad. Tal y como dice el proverbio africano, para educar a un niño hace falta la tribu entera. Por ello, desde una visión ecológica del desarrollo humano y desde la parentalidad entendida como una fenómeno complejo, dinámico y multifactorial, nos hemos basado en nuestras experiencias personales y profesionales para reflexionar sobre aquellos lugares, prácticas, personas, instituciones y redes que forman parte del desarrollo la infancia. La pregunta “¿Qué hace hoy a una familia?” se aborda, por tanto, desde el punto de vista específico de los profesionales e investigadores que trabajan en los servicios sociales o en las universidades con el objetivo de brindar el mayor apoyo posible a los progenitores y a las comunidades locales en la educación y en el desarrollo de niños y niñas. A partir de las diferencias contextuales que caracterizan a los cuatro países participantes, la puesta en conjunto nos ha permitido adquirir, en un intercambio fructífero de prácticas y herramientas, una visión panorámica que va de lo específico a lo general

First Sagittarius A* Event Horizon Telescope results. II. EHT and multiwavelength observations, data processing, and calibration

We present Event Horizon Telescope (EHT) 1.3 mm measurements of the radio source located at the position of the supermassive black hole Sagittarius A* (Sgr A*), collected during the 2017 April 5–11 campaign. The observations were carried out with eight facilities at six locations across the globe. Novel calibration methods are employed to account for Sgr A*'s flux variability. The majority of the 1.3 mm emission arises from horizon scales, where intrinsic structural source variability is detected on timescales of minutes to hours. The effects of interstellar scattering on the image and its variability are found to be subdominant to intrinsic source structure. The calibrated visibility amplitudes, particularly the locations of the visibility minima, are broadly consistent with a blurred ring with a diameter of ∼50 μas, as determined in later works in this series. Contemporaneous multiwavelength monitoring of Sgr A* was performed at 22, 43, and 86 GHz and at near-infrared and X-ray wavelengths. Several X-ray flares from Sgr A* are detected by Chandra, one at low significance jointly with Swift on 2017 April 7 and the other at higher significance jointly with NuSTAR on 2017 April 11. The brighter April 11 flare is not observed simultaneously by the EHT but is followed by a significant increase in millimeter flux variability immediately after the X-ray outburst, indicating a likely connection in the emission physics near the event horizon. We compare Sgr A*'s broadband flux during the EHT campaign to its historical spectral energy distribution and find that both the quiescent emission and flare emission are consistent with its long-term behavior.http://iopscience.iop.org/2041-8205Physic

First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multiwavelength Observations, Data Processing, and Calibration

We present Event Horizon Telescope (EHT) 1.3 mm measurements of the radio source located at the position of the supermassive black hole Sagittarius A* (Sgr A*), collected during the 2017 April 5–11 campaign. The observations were carried out with eight facilities at six locations across the globe. Novel calibration methods are employed to account for Sgr A*'s flux variability. The majority of the 1.3 mm emission arises from horizon scales, where intrinsic structural source variability is detected on timescales of minutes to hours. The effects of interstellar scattering on the image and its variability are found to be subdominant to intrinsic source structure. The calibrated visibility amplitudes, particularly the locations of the visibility minima, are broadly consistent with a blurred ring with a diameter of ∼50 μas, as determined in later works in this series. Contemporaneous multiwavelength monitoring of Sgr A* was performed at 22, 43, and 86 GHz and at near-infrared and X-ray wavelengths. Several X-ray flares from Sgr A* are detected by Chandra, one at low significance jointly with Swift on 2017 April 7 and the other at higher significance jointly with NuSTAR on 2017 April 11. The brighter April 11 flare is not observed simultaneously by the EHT but is followed by a significant increase in millimeter flux variability immediately after the X-ray outburst, indicating a likely connection in the emission physics near the event horizon. We compare Sgr A*’s broadband flux during the EHT campaign to its historical spectral energy distribution and find that both the quiescent emission and flare emission are consistent with its long-term behavior

A first update on mapping the human genetic architecture of COVID-19

peer reviewe