Características epidemiológicas de pacientes com Sepse e choque séptico

A sepse ocorre quando o sistema imunitário reage radicalmente a uma infecção. Febre alta, dificuldade respiratória, ritmo cardíaco acelerado e confusão são os principais sintomas. Para a prevenção de complicações que põem em risco a vida, é fundamental a atenção médica imediata. Este estudo teve como objetivo identificar características epidemiológicas de pacientes com sepse e choque séptico. Para isso, foi realizada uma revisão integrativa de literatura, utilizando-se LILACS e Medline como bases de pesquisa. A partir da análise qualitativa dos dados, concluiu-se que os principais fatores epidemiológicos se referem ao diagnóstico de sepse, o qual pode ser de difícil execução, realizado com atraso, de modo incorreto ou superdiagnosticado, e a inobservância das recomendações (práticas de enfermagem) para os cuidados com a sepse. Esses fatores contribuem para o agravamento da sepse, o atendimento de pacientes em unidades de terapia intensiva e o aumento dos níveis de mortalidade

A relação dos fármacos agonistas de receptores GLP-1 e a proteção de doença renal para pacientes com Diabetes Mellitus

A diabetes mellitus compreende a incapacidade do organismo de desempenhar a função fisiológica da insulina, ocasionando uma grande carga de doenças, incluindo doença renal ou renal crônica e cardiovasculares. Os agonistas do receptor de GLP-1 são empregados em pacientes com diabetes tipo 2 como terapias de redução da glicose diversos à saúde destes pacientes. O objetivo deste estudo foi analisar a forma de ação dos agonistas de receptores GLP-1 como um fator de proteção à patologia renal crônica, em indivíduos portadores de diabetes mellitus do tipo 2, por meio de uma revisão bibliográfica sistemática. Os dados publicados demonstram que que agonistas do receptor GLP-1 reduzem a morte e incidência de doença renal terminal ou de insuficiência renal. Adicionalmente estes fármacos podem bloquear os mecanismos envolvidos em doenças renais, além de amenizar o estresse oxidativo e apoptose celular no rim. As terapias utilizadas com o uso de agonistas GLP-1 têm se mostrado agentes redutores da glicose e eficazes para pacientes com diabetes mellitus tipo 2, sendo recomendadas por instituições americanas e européias

Studies of the mass composition of cosmic rays and proton-proton interaction cross-sections at ultra-high energies with the Pierre Auger Observatory

In this work, we present an estimate of the cosmic-ray mass composition from the distributions of the depth of the shower maximum (Xmax) measured by the fluorescence detector of the Pierre Auger Observatory. We discuss the sensitivity of the mass composition measurements to the uncertainties in the properties of the hadronic interactions, particularly in the predictions of the particle interaction cross-sections. For this purpose, we adjust the fractions of cosmic-ray mass groups to fit the data with Xmax distributions from air shower simulations. We modify the proton-proton cross-sections at ultra-high energies, and the corresponding air shower simulations with rescaled nucleus-air cross-sections are obtained via Glauber theory. We compare the energy-dependent composition of ultra-high-energy cosmic rays obtained for the different extrapolations of the proton-proton cross-sections from low-energy accelerator data

Study of downward Terrestrial Gamma-ray Flashes with the surface detector of the Pierre Auger Observatory

The surface detector (SD) of the Pierre Auger Observatory, consisting of 1660 water-Cherenkov detectors (WCDs), covers 3000 km2 in the Argentinian pampa. Thanks to the high efficiency of WCDs in detecting gamma rays, it represents a unique instrument for studying downward Terrestrial Gamma-ray Flashes (TGFs) over a large area. Peculiar events, likely related to downward TGFs, were detected at the Auger Observatory. Their experimental signature and time evolution are very different from those of a shower produced by an ultrahigh-energy cosmic ray. They happen in coincidence with low thunderclouds and lightning, and their large deposited energy at the ground is compatible with that of a standard downward TGF with the source a few kilometers above the ground. A new trigger algorithm to increase the TGF-like event statistics was installed in the whole array. The study of the performance of the new trigger system during the lightning season is ongoing and will provide a handle to develop improved algorithms to implement in the Auger upgraded electronic boards. The available data sample, even if small, can give important clues about the TGF production models, in particular, the shape of WCD signals. Moreover, the SD allows us to observe more than one point in the TGF beam, providing information on the emission angle

The dynamic range of the upgraded surface-detector stations of AugerPrime

The detection of ultra-high-energy cosmic rays by means of giant detector arrays is often limited by the saturation of the recorded signals near the impact point of the shower core at the ground, where the particle density dramatically increases. The saturation affects in particular the highest energy events, worsening the systematic uncertainties in the reconstruction of the shower characteristics. The upgrade of the Pierre Auger Observatory, called AugerPrime, includes the installation of an 1-inch Small PhotoMultiplier Tube (SPMT) inside each water-Cherenkov station (WCD) of the surface detector array. The SPMT allows an unambiguous measurement of signals down to about 250m from the shower core, thus reducing the number of events featuring a saturated station to a negligible level. In addition, a 3.8m2 plastic scintillator (Scintillator Surface Detector, SSD) is installed on top of each WCD. The SSD is designed to match the WCD (with SPMT) dynamic range, providing a complementary measurement of the shower components up to the highest energies. In this work, the design and performances of the upgraded AugerPrime surface-detector stations in the extended dynamic range are described, highlighting the accuracy of the measurements. A first analysis employing the unsaturated signals in the event reconstruction is also presented

International Masterclasses as part of the Pierre Auger Observatory program of Outreach and Education

The Pierre Auger Observatory is committed to bringing education and knowledge of cosmic rays to the public, with a strong focus on schools and students. Over the last few years, initiatives have been developed, such as the Science Fair, virtual visits, and participation in international activities on the subject of cosmic rays, including collaborations with external groups. Modern digital tools bringing novel ways of interacting with the public have been explored at these initiatives and also locally at a renewed Visitor Center in Malargüe. The development of tools for the public release of the Auger data, including standardized data formats, analysis notebooks, and a 3D interactive event display, led to the creation of a new activity directed to high-school students called Masterclasses. The participants are challenged to perform the reconstruction and selection of events using a graphical interface with 3D effects, then combined into a smoothed, exposure-corrected sky map of arrival directions. A final discussion takes place in which the students engage with peers and scientists, looking for answers about the origin of ultra-high-energy cosmic rays. The concept had a successful debut in 2022 and was included in the 2023 edition of the International Masterclasses on Particle Physics, reaching students worldwide