4,943 research outputs found

    Possibilities and pitfalls? Moderate drinking and alcohol abstinence at home since the COVID-19 lockdown

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    The global ‘lockdowns’ and social distancing measures triggered by the COVID-19 pandemic have brought about unprecedented social changes, including the sudden, temporary closure of licensed venues and significant modifications to leisure and drinking practices. In this piece, we argue that these changes invite researchers to consider the short and longer-term consequences in terms of continuities and changes to the practices and symbolism of alcohol consumption both within and beyond domestic spaces. We do this by drawing on illustrations from our emergent qualitative research involving internet-mediated semi-structured and focus group interviews with 20 participants from the UK (aged 26-65) concerning experiences of drinking in and beyond ‘lockdown’. In sharing these early findings, we hope to highlight themes relevant to understanding drinking behaviour during the COVID-19 pandemic and to stimulate dialogue for immediate research priorities in this area. Key topic areas in our data appear to concern; variability in heavy/moderate/light/non-drinking practices while drinking at home, lockdown as an opportunity to reassess relationships with alcohol, and the symbolic role of alcohol in internet-mediated communications and interactions. Longstanding policymaker and practitioner concerns with managing public drinking and public order may have been unsettled by a growth in home-based drinking, although, as we argue, such changes were in motion before the global pandemic. We propose that a greater understanding of the challenges and opportunities the pandemic presents for (re)negotiating relationships with alcohol may offer wider lessons around how individuals and communities might be supported via innovative policy measures to change their relationships with alcohol both during and beyond lockdown

    All in this together?

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    Almost daily news reports point to how lockdown, ‘the new normal’ for most, is influencing behaviours relevant to physical health like alcohol consumption and taking physical activity. But how is health behaviour changing, among whom, and will any changes last post-lockdown? We argue that health polarisations are tied with broader social inequalities with implications for whether any lifestyle changes will endure. Psychological and social science research must respond with creative, collaborative and innovative research to guide health policy and practice in the post-lockdown world serving the interests of all citizens

    Function-based Intersubject Alignment of Human Cortical Anatomy

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    Making conclusions about the functional neuroanatomical organization of the human brain requires methods for relating the functional anatomy of an individual's brain to population variability. We have developed a method for aligning the functional neuroanatomy of individual brains based on the patterns of neural activity that are elicited by viewing a movie. Instead of basing alignment on functionally defined areas, whose location is defined as the center of mass or the local maximum response, the alignment is based on patterns of response as they are distributed spatially both within and across cortical areas. The method is implemented in the two-dimensional manifold of an inflated, spherical cortical surface. The method, although developed using movie data, generalizes successfully to data obtained with another cognitive activation paradigm—viewing static images of objects and faces—and improves group statistics in that experiment as measured by a standard general linear model (GLM) analysis

    Violent quenching : Molecular Gas Blown to 1000 km s -1 during a Major Merger

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    Accepted for publication in ApJ LettersWe present Atacama Large Millimeter/submillimeter Array observations of a massive () compact ( pc) merger remnant at z = 0.66 that is driving a 1000 km s -1 outflow of cool gas, with no observational trace of an active galactic nucleus (AGN). We resolve molecular gas on scales of approximately 1-2 kpc, and our main finding is the discovery of a wing of blueshifted CO J(2 → 1) emission out to-1000 km s -1 relative to the stars. We argue that this is the molecular component of a multiphase outflow, expelled from the central starburst within the past 5 Myr through stellar feedback, although we cannot rule out previous AGN activity as a launching mechanism. If the latter is true, then this is an example of a relic multiphase AGN outflow. We estimate a molecular mass outflow rate of approximately 300 M o yr -1, or about one third of the 10 Myr-Averaged star formation rate. This system epitomizes the multiphase "blowout" episode following a dissipational major merger-a process that has violently quenched central star formation and supermassive black hole growth.Peer reviewedFinal Accepted Versio

    Achievement goals, self-handicapping, and performance: A 2 × 2 achievement goal perspective

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    Elliot and colleagues (2006) examined the effects of experimentally induced achievement goals, proposed by the trichotomous model, on self-handicapping and performance in physical education. Our study replicated and extended the work of Elliot et al. by experimentally promoting all four goals proposed by the 262 model (Elliot & McGregor, 2001), measuring the participants’ own situational achievement goals, using a relatively novel task, and testing the participants in a group setting. We used a randomized experimental design with four conditions that aimed to induce one of the four goals advanced by the 262 model. The participants (nÂŒ138) were undergraduates who engaged in a dart-throwing task. The results pertaining to self-handicapping partly replicated Elliot and colleagues’ findings by showing that experimentally promoted performance-avoidance goals resulted in less practice. In contrast, the promotion of mastery-avoidance goals did not result in less practice compared with either of the approach goals. Dart-throwing performance did not differ among the four goal conditions. Personal achievement goals did not moderate the effects of experimentally induced goals on selfhandicapping and performance. The extent to which mastery-avoidance goals are maladaptive is discussed, as well as the interplay between personal and experimentally induced goals

    The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. VII. Properties of the Host Galaxy and Constraints on the Merger Timescale

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    We present the properties of NGC 4993, the host galaxy of GW170817, the first gravitational wave (GW) event from the merger of a binary neutron star (BNS) system and the first with an electromagnetic (EM) counterpart. We use both archival photometry and new optical/near-IR imaging and spectroscopy, together with stellar population synthesis models to infer the global properties of the host galaxy. We infer a star formation history peaked at ≳10\gtrsim 10 Gyr ago, with subsequent exponential decline leading to a low current star formation rate of 0.01 M⊙_{\odot} yr−1^{-1}, which we convert into a binary merger timescale probability distribution. We find a median merger timescale of 11.2−1.4+0.711.2^{+0.7}_{-1.4} Gyr, with a 90% confidence range of 6.8−13.66.8-13.6 Gyr. This in turn indicates an initial binary separation of ≈4.5\approx 4.5 R⊙_{\odot}, comparable to the inferred values for Galactic BNS systems. We also use new and archival HubbleHubble SpaceSpace TelescopeTelescope images to measure a projected offset of the optical counterpart of 2.12.1 kpc (0.64rer_{e}) from the center of NGC 4993 and to place a limit of Mr≳−7.2M_{r} \gtrsim -7.2 mag on any pre-existing emission, which rules out the brighter half of the globular cluster luminosity function. Finally, the age and offset of the system indicates it experienced a modest natal kick with an upper limit of ∌200\sim 200 km s−1^{-1}. Future GW−-EM observations of BNS mergers will enable measurement of their population delay time distribution, which will directly inform their viability as the dominant source of rr-process enrichment in the Universe.Comment: 9 Pages, 3 Figures, 2 Tables, ApJL, In Press. Keywords: GW170817, LV
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