72 research outputs found
Butt-joint bonding of timber as a key technology for point-supported, biaxial load bearing flat slabs made of cross-laminated timber
An efficient butt-joint bonding technology allows to build new types of timber structures. Under the name Timber Structures 3.0 a connection has been developed which connects timber elements with an end-grain to end-grain butt joint bonding. Therefore, it is now possible to build continuous, point supported flat slabs in cross laminated timber (CLT). Multiple CLT slabs are connected rigidly together and are only supported by columns. Some major challenges had to be solved in terms of bending strength of the glued connection and shear resistance of the part of the slab above the column. The research in both topics is successful and more projects were built in the last two years using this technology. Starting point was a real scale structure at ETH Zurich, followed by a working platform for a timber construction company and finally four three storey residential buildings. The research team is continuing to optimize the different elements of this innovative technology and will soon provide engineers with guidelines to design their own biaxial, point supported timber flat slabs
Regular frequency patterns in the young delta Scuti star HD 261711 observed by the CoRoT and MOST satellites
We concentrate on an asteroseismological study of HD 261711, a rather hot
delta Scuti type pulsating member of the young open cluster NGC 2264 located at
the blue border of the instability region. HD 261711 was discovered to be a
pre-main sequence delta Scuti star using the time series photometry obtained by
the MOST satellite in 2006. High-precision, time-series photometry of HD 261711
was obtained by the MOST and CoRoT satellites in 4 separate new observing runs
that are put into context with the star's fundamental atmospheric parameters
obtained from spectroscopy. With the new MOST data set from 2011/12 and the two
CoRoT light curves from 2008 and 2011/12, the delta Scuti variability was
confirmed and regular groups of frequencies were discovered. The two pulsation
frequencies identified in the data from the first MOST observing run in 2006
are confirmed and 23 new delta Scuti-type frequencies were discovered using the
CoRoT data. Weighted average frequencies for each group are related to l=0 and
l=1 p-modes. Evidence for amplitude modulation of the frequencies in two groups
is seen. The effective temperature was derived to be 8600200 K, log g is
4.10.2, and the projected rotational velocity is 531km/s. Using our
Teff value and the radius of 1.80.5 Rsun derived from SED fitting, we get
a log L/Lsun of 1.200.14 which agrees well to the seismologically
determined values of 1.65 Rsun and, hence, a log L/Lsun of 1.13. The radial
velocity of 142 km/s we derived for HD 261711, confirms the star's
membership to NGC 2264. Our asteroseismic models suggest that HD 261711 is a
delta Scuti-type star close to the zero-age main sequence (ZAMS) with a mass of
1.8 to 1.9Msun. HD 261711 is either a young ZAMS star or a late PMS star just
before the onset of hydrogen-core burning.Comment: 12 pages, 13 figures, A&A accepte
Echography of young stars reveals their evolution
We demonstrate that a seismic analysis of stars in their earliest
evolutionary phases is a powerful method to identify young stars and
distinguish their evolutionary states. The early star that is born from the
gravitational collapse of a molecular cloud reaches at some point sufficient
temperature, mass and luminosity to be detected. Accretion stops and the
pre-main sequence star that emerges is nearly fully convective and chemically
homogeneous. It will continue to contract gravitationally until the density and
temperature in the core are high enough to start nuclear burning of hydrogen.
We show that there is a relationship between detected pulsation properties for
a sample of young stars and their evolutionary status illustrating the
potential of asteroseismology for the early evolutionary phases.Comment: 23 pages, 9 figures, includes Supplementary Material. Science,
published in Science Express on July 3, 201
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The vulnerability, impacts, adaptation and climate services advisory board (VIACS AB v1.0) contribution to CMIP6
This paper describes the motivation for the creation of the Vulnerability, Impacts, Adaptation and Climate Services (VIACS) Advisory Board for the Sixth Phase of the Coupled Model Intercomparison Project (CMIP6), its initial activities, and its plans to serve as a bridge between climate change applications experts and climate modelers. The climate change application community comprises researchers and other specialists who use climate information (alongside socioeconomic and other environmental information) to analyze vulnerability, impacts and adaptation of natural systems and society in relation to past, ongoing and projected future climate change. Much of this activity is directed toward the co-development of information needed by decision-makers for managing projected risks. CMIP6 provides a unique opportunity to facilitate a two-way dialogue between climate modelers and VIACS experts who are looking to apply CMIP6 results for a wide array of research and climate services objectives. The VIACS Advisory Board convenes leaders of major impact sectors, international programs, and climate services to solicit community feedback that increases applications relevance of the CMIP6-Endorsed Model Intercomparison Projects (MIPs). As an illustration of its potential, the VIACS community provided CMIP6 leadership with a list of prioritized climate model variables and MIP experiments of greatest interest to the climate model applications community, indicating the applicability and societal relevance of climate model simulation outputs. The VIACS Advisory Board also recommended an impacts version of Obs4MIPs, and indicated user needs for the gridding and processing of model output
Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi
Over the course of its history, the Milky Way has ingested multiple smaller satellite galaxies1. Although these accreted stellar populations can be forensically identified as kinematically distinct structures within the Galaxy, it is difficult in general to date precisely the age at which any one merger occurred. Recent results have revealed a population of stars that were accreted via the collision of a dwarf galaxy, called Gaia–Enceladus1, leading to substantial pollution of the chemical and dynamical properties of the Milky Way. Here we identify the very bright, naked-eye star ν Indi as an indicator of the age of the early in situ population of the Galaxy. We combine asteroseismic, spectroscopic, astrometric and kinematic observations to show that this metal-poor, alpha-element-rich star was an indigenous member of the halo, and we measure its age to be 11.0 ± 0.7 (stat) ± 0.8 (sys) billion years. The star bears hallmarks consistent with having been kinematically heated by the Gaia–Enceladus collision. Its age implies that the earliest the merger could have begun was 11.6 and 13.2 billion years ago, at 68% and 95% confidence, respectively. Computations based on hierarchical cosmological models slightly reduce the above limits
Stakeholders' views and experiences of care and interventions for addressing frailty and pre-frailty:a meta-synthesis of qualitative evidence
Frailty is a common condition in older age and is a public health concern which requires integrated care and involves different stakeholders. This meta-synthesis focuses on experiences, understanding, and attitudes towards screening, care, intervention and prevention for frailty across frail and healthy older persons, caregivers, health and social care practitioners. Studies published since 2001 were identified through search of electronic databases; 81 eligible papers were identified and read in full, and 45 papers were finally included and synthesized. The synthesis was conducted with a meta-ethnographic approach. We identified four key themes: Uncertainty about malleability of frailty; Strategies to prevent or to respond to frailty; Capacity to care and person and family-centred service provision; Power and choice. A bottom-up approach which emphasises and works in synchrony with frail older people's and their families' values, goals, resources and optimisation strategies is necessary. A greater employment of psychological skills, enhancing communication abilities and tools to overcome disempowering attitudes should inform care organisation, resulting in more efficient and satisfactory use of services. Public health communication about prevention and management of frailty should be founded on a paradigm of resilience, balanced acceptance, and coping. Addressing stakeholders' views about the preventability of frailty was seen as a salient need
Ansiedade frente ao tratamento odontolĂłgico: prevalĂŞncia e fatores predictores em brasileiros
Empirical evidence of the relationship between parental and child dental fear: a structured review and meta-analysis
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