10 research outputs found

    Prevalence, associated factors and outcomes of pressure injuries in adult intensive care unit patients: the DecubICUs study

    Get PDF
    Funder: European Society of Intensive Care Medicine; doi: http://dx.doi.org/10.13039/501100013347Funder: Flemish Society for Critical Care NursesAbstract: Purpose: Intensive care unit (ICU) patients are particularly susceptible to developing pressure injuries. Epidemiologic data is however unavailable. We aimed to provide an international picture of the extent of pressure injuries and factors associated with ICU-acquired pressure injuries in adult ICU patients. Methods: International 1-day point-prevalence study; follow-up for outcome assessment until hospital discharge (maximum 12 weeks). Factors associated with ICU-acquired pressure injury and hospital mortality were assessed by generalised linear mixed-effects regression analysis. Results: Data from 13,254 patients in 1117 ICUs (90 countries) revealed 6747 pressure injuries; 3997 (59.2%) were ICU-acquired. Overall prevalence was 26.6% (95% confidence interval [CI] 25.9–27.3). ICU-acquired prevalence was 16.2% (95% CI 15.6–16.8). Sacrum (37%) and heels (19.5%) were most affected. Factors independently associated with ICU-acquired pressure injuries were older age, male sex, being underweight, emergency surgery, higher Simplified Acute Physiology Score II, Braden score 3 days, comorbidities (chronic obstructive pulmonary disease, immunodeficiency), organ support (renal replacement, mechanical ventilation on ICU admission), and being in a low or lower-middle income-economy. Gradually increasing associations with mortality were identified for increasing severity of pressure injury: stage I (odds ratio [OR] 1.5; 95% CI 1.2–1.8), stage II (OR 1.6; 95% CI 1.4–1.9), and stage III or worse (OR 2.8; 95% CI 2.3–3.3). Conclusion: Pressure injuries are common in adult ICU patients. ICU-acquired pressure injuries are associated with mainly intrinsic factors and mortality. Optimal care standards, increased awareness, appropriate resource allocation, and further research into optimal prevention are pivotal to tackle this important patient safety threat

    Time evolution of slowly rotating neutron stars in general relativity

    No full text
    Kompakte stellare Objekte wie Neutronensterne sind vielversprechende Quellen von Gravitationswellen. Zur Interpretation der möglicherweise in naher Zukunft zu erwartenden Messdaten ist es wichtig, die Frequenzen der axialen und polaren Schwingungsmoden theoretisch zu bestimmen. Die vorliegende Arbeit untersucht die numerische Zeitentwicklung der linearisierten Einsteinschen Feldgleichungen für langsam rotierende Neutronensterne ohne die bisher meist zugrunde gelegte Cowling-Näherung bzw. inverse Cowling-Näherung. Hierfür werden sowohl Lösungen für fluide als auch raumzeitliche, metrische Störungen berechnet. Die gekoppelten hyperbolischen Differenzialgleichungen erster Ordnung werden im Rahmen des Arnowitt-Deser-Misner-Formalismus und unter Verwendung der Battiston-Cazzola-Lucaroni-Eichung hergeleitet. Durch die Berücksichtigung der Metrikstörungen ist es möglich, eine explizit berechnete Fehlertoleranz der Cowling-Näherung anzugeben und eine höhere Genauigkeit der resultierenden Frequenzen zu erzielen. Die zeitliche Entwicklung wird sowohl für polytrope Sternmodelle als auch für realistische Zustandsgleichungen berechnet, insbesondere für die Zustandsgleichung MPA (Machleidt Potential A). Anhand des Spektrums können die f-, die p- und die w-Moden identifiziert und deren Frequenzen bestimmt werden, sowie eingeschränkt auch die der r-Mode. Für die vollrelativistische Zeitentwicklung sind dies die ersten Ergebnisse für die Zustandsgleichung MPA, die in guter Übereinstimmung mit bisher bekannten Ergebnissen der Modenanalyse dieser Zustandsgleichung stehen. Die Berücksichtigung der Kopplungen zwischen axialen und polaren Moden liefert eine bessere Einsicht in das Schwingungsverhalten von Neutronensternen. Darüberhinaus wird in dieser Arbeit für realistische Zustandsgleichungen ein empirisches Skalierungsverhalten der fluiden sowie der räumlichen Moden angegeben, welches in guter Übereinstimmung mit dem in der Modenanalyse ermittelten Skalierungsverhalten steht.Compact stellar objects like neutron stars are promising candidates for gravitational wave sources. For measuring purpose it is important to determine first theoretically the frequencies of the axial and polar oscillation modes. The present work investigates the numerical time evolution of the linearized Einstein field equations for slowly rotating neutron stars without the frequently used Cowling approximation. For that case solutions for the metric perturbations are calculated for fluid and spacetime parts. The set of coupled wave equations, a first-order hyperbolic evolution system, is derived in the frame of the ADM (Arnowitt-Deser-Misner) formalism in the BCL (Battiston-Cazzola-Lucaroni) gauge. By including also the metric perturbations we are able to determine the error of the Cowling approximation and increase the accuracy of the resulting frequencies. Results for various polytropic and realistic stellar models in particular for the realistic equation of state MPA (Machleidt Potential A) are presented. We identify the resulting f-, p- and w-modes from the spectra and thus the corresponding frequencies as well as the r-modes in limited cases. For the equation of state MPA these are the first results which are obtained by the method of numerical time evolution within the framework of general relativity. The resulting frequencies are in good accordance with the frequencies obtained in the mode calculations. By considering the coupling between axial and polar modes a better insight in the oscillation characteristics of neutron stars is gained. Furthermore we show empirical scaling relations for the axial and polar modes for realistic equations of state which are also in good agreement with empirical relations found in latest mode calculations

    Visualization in the Einstein Year 2005: A Case Study on Explanatory and Illustrative Visualization of Relativity and Astrophysics

    No full text
    with relativistic and astrophysical visualization, which has been culminating in a substantial engagement for visualization in the Einstein Year 2005---the 100 anniversary of Einstein's publications on special relativity, the photoelectric effect, and Brownian motion. This paper focuses on explanatory and illustrative visualizations used to communicate aspects of the difficult theories of special and general relativity, their geometric structure, and of the related fields of cosmology and astrophysics. We discuss visualization strategies, motivated by physics education and didactics of mathematics, and describe what kind of visualization methods have proven to be useful for different types of media, such as still images in popular-science magazines, film contributions to TV shows, oral presentations, or interactive museum installations. Although our visualization tools build upon existing methods and implementations, these techniques have been improved by several novel technical contributions like image-based special relativistic rendering on GPUs, an extension of general relativistic ray tracing to manifolds described by multiple charts, GPU-based interactive visualization of gravitational light deflection, as well as planetary terrain rendering. The usefulness and effectiveness of our visualizations are demonstrated by reporting on experiences with, and feedback from, recipients of visualizations and collaborators

    Correction to: Prevalence, associated factors and outcomes of pressure injuries in adult intensive care unit patients: the DecubICUs study (Intensive Care Medicine, (2021), 47, 2, (160-169), 10.1007/s00134-020-06234-9)

    No full text
    The original version of this article unfortunately contained a mistake. The members of the ESICM Trials Group Collaborators were not shown in the article but only in the ESM. The full list of collaborators is shown below. The original article has been corrected

    Risk of COVID-19 after natural infection or vaccinationResearch in context

    No full text
    Summary: Background: While vaccines have established utility against COVID-19, phase 3 efficacy studies have generally not comprehensively evaluated protection provided by previous infection or hybrid immunity (previous infection plus vaccination). Individual patient data from US government-supported harmonized vaccine trials provide an unprecedented sample population to address this issue. We characterized the protective efficacy of previous SARS-CoV-2 infection and hybrid immunity against COVID-19 early in the pandemic over three-to six-month follow-up and compared with vaccine-associated protection. Methods: In this post-hoc cross-protocol analysis of the Moderna, AstraZeneca, Janssen, and Novavax COVID-19 vaccine clinical trials, we allocated participants into four groups based on previous-infection status at enrolment and treatment: no previous infection/placebo; previous infection/placebo; no previous infection/vaccine; and previous infection/vaccine. The main outcome was RT-PCR-confirmed COVID-19 >7–15 days (per original protocols) after final study injection. We calculated crude and adjusted efficacy measures. Findings: Previous infection/placebo participants had a 92% decreased risk of future COVID-19 compared to no previous infection/placebo participants (overall hazard ratio [HR] ratio: 0.08; 95% CI: 0.05–0.13). Among single-dose Janssen participants, hybrid immunity conferred greater protection than vaccine alone (HR: 0.03; 95% CI: 0.01–0.10). Too few infections were observed to draw statistical inferences comparing hybrid immunity to vaccine alone for other trials. Vaccination, previous infection, and hybrid immunity all provided near-complete protection against severe disease. Interpretation: Previous infection, any hybrid immunity, and two-dose vaccination all provided substantial protection against symptomatic and severe COVID-19 through the early Delta period. Thus, as a surrogate for natural infection, vaccination remains the safest approach to protection. Funding: National Institutes of Health
    corecore