Gender, intoxication and the developing brain: Problematisations of drinking among young adults in Australian alcohol policy

In this article, we draw on recent scholarly work in the poststructuralist analysis of policy to consider how policy itself functions as a key site in the constitution of alcohol ‘problems’, and the political implications of these problematisations. We do this by examining Australian alcohol policy as it relates to young adults (18–24 years old). Our critical analysis focuses on three national alcohol policies (1990, 2001 and 2006) and two Victorian state alcohol policies (2008 and 2013), which together span a 25-year period. We argue that Australian alcohol policies have conspicuously ignored young adult men, despite their ongoing over-representation in the statistical ‘evidence base’ on alcohol-related harm, while increasingly problematising alcohol consumption amongst other population subgroups. We also identify the development of a new problem representation in Australian alcohol policy, that of ‘intoxication’ as the leading cause of alcohol-related harm and rising hospital admissions, and argue that changes in the classification and diagnosis of intoxication may have contributed to its prioritisation and problematisation in alcohol policy at the expense of other forms of harm. Finally, we draw attention to how preliminary and inconclusive research on the purported association between binge drinking and brain development in those under 25 years old has been mobilised prematurely to support calls to increase the legal purchasing age from 18 to 21 years. Our critical analysis of the treatment of these three issues – gender, intoxication, and brain development – is intended to highlight the ways in which policy functions as a key site in the constitution of alcohol ‘problems’

Scattering of Nucleons in the Classical Skyrme Model

Classically spinning B = 1 Skyrmions can be regarded as approximations to nucleons with quantised spin. Here, we investigate nucleon–nucleon scattering through numerical collisions of spinning Skyrmions. We identify the dineutron/diproton and dibaryon short-lived resonance states, and also the stable deuteron state. Our simulations lead to predictions for the polarisation states occurring in right angle scattering

The use of transillumination in mapping demarcated enamel opacities in anterior teeth:A cross-sectional study

Background: Despite intensive efforts for categorizing demarcated enamel opacities, often related to molar incisor hypomineralization (MIH), there is a lack of descriptive criteria aiming to describe them physically outside the scope of color and size. This is most likely due to the indices focusing on molar, not anterior, teeth. Aim: To map and classify demarcated lesions on permanent anterior teeth using reflected and transilluminated light. The association between classification and related lesion characteristics was also examined. Design: Permanent anterior teeth with demarcated opacities related to MIH were selected. For each tooth, standardized photographs were taken using transmitted and reflected light. Each lesion was mapped and classified according to its color, lesion size, surface integrity, and type. The data were analyzed using the chi-square and Fisher's exact tests. A logistic regression analysis was performed to identify the risk of PEB. Results: There were significant relationships between lesion size, color, and type with surface integrity. Lesion type and size were more important than lesion color for assessing the risk of PEB. There was also a significant relationship between lesion size and lesion color. Conclusions: Lesion size and type are significant clinical parameters for assessing the risk of PEB on enamel opacities related to MIH

The influence of lesion characteristics on application time of an infiltrate applied to MIH lesions on anterior teeth:An exploratory in vivo pilot study

Objectives: To evaluate the factors that influences the kinetics of resin infiltration of molar incisor hypomineralisation (MIH) lesions on permanent anterior teeth. Methods: Demarcated MIH lesions with homogeneous and heterogeneous lesion body appearance, Types 1 (n = 14) and 2 (n = 18), respectively, were selected. After removal of the lesion surface layer using a tapered diamond finishing bur, the lesions were etched and ethanol was applied to the lesions and it was determined if the lesion was still visible or not. Images were taken just prior infiltrant (Icon; DMG) application (T0), during the infiltration process (Tx) and when infiltration had ceased progressing or opacity disappearance was clinically apparent (Tmax). Surface-area measurements of the opacity and infiltrated area were calculated and the infiltration proportion (IPx) was calculated over the infiltration time. Results: Type 1 and positive ethanol test lesions showed significantly lower mean Tmax (3.4 min) in comparison with Type 2 and negative ethanol test lesions (9.9 min) [Student t-test/Fisher's exact test; p <.01]. A non-linear correlation was observed (R2 = 0.88) indicating that the IPx was rapid at the beginning of resin application, decreasing over time. Conclusion: In comparison with Type 1 and positive ethanol test lesions, Type 2 and negative ethanol test lesions require longer application time to infiltrate. Clinical significance: MIH-lesion type and the ‘ethanol test’ were reliable predictive factors for the application time required for infiltrating MIH lesions on permanent anterior teeth

Simple dynamical models of the Sagittarius dwarf galaxy

We present two simple dynamical models for Sagittarius based on N-body simulations of the progressive disruption of a satellite galaxy orbiting for 12.5 Gyr within a realistic Galactic potential. In both models the satellite initially has observable properties similar to those of current outlying dwarfs; in one case it is purely stellar while in the other it is embedded in an extended massive halo. The purely stellar progenitor is a King model with a total velocity dispersion of 18.9 km s-1, a core radius of 0.44 kpc and a tidal radius of 3 kpc. The initial stellar distribution in the other case follows a King profile with the same core radius, a slightly larger total velocity dispersion and similar extent. Both these models are consistent with all published data on the current Sagittarius system, they match not only the observed properties of the main body of Sagittarius, but also those reported for unbound debris at larger distances.Facultad de Ciencias Astronómicas y Geofísica

Scattering of Skyrmions

In this paper, we present a detailed study of Skyrmion-Skyrmion scattering for two B=1 Skyrmions in the attractive channel where we observe two different scattering regimes. For large separation, the scattering can be approximated as interacting dipoles. We give a qualitative estimate when this approximation breaks down. For small separations we observe an additional short-range repulsion which is qualitatively similar to monopole scattering. We also observe the interesting effect of "rotation without rotating" whereby two Skyrmions, whose orientations remain constant while well-separated, change their orientation after scattering. We can explain this effect by following preimages through the scattering process, thereby measuring which part of an in-coming Skyrmion forms part of an out-going Skyrmion. This leads to a new way of visualising Skyrmions. Furthermore, we consider spinning Skyrmions and find interesting trajectories

Preparedness for dental practice in Australia:a qualitative study on the experiences of final-year students and new graduates

Background: Limited data exists regarding the perspectives of newly graduated dental practitioners (NGDPs) and final-year students (FYS) about their preparedness for dental practice. This information is crucial to inform developments in ongoing professional development for newly qualified dental practitioners and future reviews and development of accreditation standards, policies, and the professional competencies of newly qualified dental practitioners. Thus, the primary goal of this paper was to describe the perceptions of preparedness for dental practice of NGDPs and FYSs.Methods: Individual semi-structured interviews were conducted between March and July 2020. All interviews were audiotaped, transcribed, and analysed using a thematic analysis.Results: Eighteen NGDPs and four FYS from across Australia participated in the qualitative interviews. A strong theme from the data was that respondents believed they were well prepared for common challenges in dental practice and patient care. A second prominent theme was participants’ awareness of specific areas of limitation in their knowledge and specific skills including (list them). This data highlights a high level of self-awareness and potential for self-directed learning of NGDPs. It also provides specific content areas for future curriculum developers.Conclusions: Newly graduated dental practitioner and final-year student participants were satisfied with the theoretical and evidence-based information in their formal learning and teaching activities to begin practicing as dental practitioners. In some areas, NGDPs felt underprepared, mostly attributed to limited clinical treatment exposure, and other contextual elements of clinical practice, and thought transitional support may be required. The research reinforces the value of seeking and learning from students’ and NGDPs’ perspectives.</p

Scattering of Several Multiply Charged Extremal D=5 Black Holes

The moduli space metric for an arbitrary number of extremal D=5 black holes with arbitrary relatively supersymmetric charges is found.Comment: 12 pages, ReVTeX. Minor typos corrected, including an unimportant sign for which the corresponding comment was removed. One reference adde