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Media coverage of non-suicidal self-injury (NSSI) ranges from providing helpful education to displaying graphic images. We offer the first research-informed, consensus-based guidelines for the responsible reporting and depicting of NSSI in the media, while also advising on ideas for dissemination and collaboration between media professionals and healthcare experts.
Gene × environment (G × E) interactions in eating pathology have been increasingly investigated, however studies have been limited by sample size due to the difficulty of obtaining genetic data.
To synthesize existing G × E research in the eating disorders (ED) field and provide a clear picture of the current state of knowledge with analyses of larger samples.
Complete data from seven studies investigating community (n = 1750, 64.5% female) and clinical (n = 426, 100% female) populations, identified via systematic review, were included. Data were combined to perform five analyses: 5-HTTLPR × Traumatic Life Events (0–17 events) to predict ED status (n = 909), 5-HTTLPR × Sexual and Physical Abuse (n = 1097) to predict bulimic symptoms, 5-HTLPR × Depression to predict bulimic symptoms (n = 1256), and 5-HTTLPR × Impulsivity to predict disordered eating (n = 1149).
The low function (s) allele of 5-HTTLPR interacted with number of traumatic life events (P < .01) and sexual and physical abuse (P < .05) to predict increased likelihood of an ED in females but not males (Fig. 1). No other G × E interactions were significant, possibly due to the medium to low compatibility between datasets (Fig. 1).
Early promising results suggest that increased knowledge of G × E interactions could be achieved if studies increased uniformity of measuring ED and environmental variables, allowing for continued collaboration to overcome the restrictions of obtaining genetic samples.
Disclosure of interest
The authors have not supplied their declaration of competing interest.
Given the common view that pre-exercise nutrition/breakfast is important for performance, the present study investigated whether breakfast influences resistance exercise performance via a physiological or psychological effect. Twenty-two resistance-trained, breakfast-consuming men completed three experimental trials, consuming water-only (WAT), or semi-solid breakfasts containing 0 g/kg (PLA) or 1·5 g/kg (CHO) maltodextrin. PLA and CHO meals contained xanthan gum and low-energy flavouring (approximately 122 kJ), and subjects were told both ‘contained energy’. At 2 h post-meal, subjects completed four sets of back squat and bench press to failure at 90 % ten repetition maximum. Blood samples were taken pre-meal, 45 min and 105 min post-meal to measure serum/plasma glucose, insulin, ghrelin, glucagon-like peptide-1 and peptide tyrosine-tyrosine concentrations. Subjective hunger/fullness was also measured. Total back squat repetitions were greater in CHO (44 (sd 10) repetitions) and PLA (43 (sd 10) repetitions) than WAT (38 (sd 10) repetitions; P < 0·001). Total bench press repetitions were similar between trials (WAT 37 (sd 7) repetitions; CHO 39 (sd 7) repetitions; PLA 38 (sd 7) repetitions; P = 0·130). Performance was similar between CHO and PLA trials. Hunger was suppressed and fullness increased similarly in PLA and CHO, relative to WAT (P < 0·001). During CHO, plasma glucose was elevated at 45 min (P < 0·05), whilst serum insulin was elevated (P < 0·05) and plasma ghrelin suppressed at 45 and 105 min (P < 0·05). These results suggest that breakfast/pre-exercise nutrition enhances resistance exercise performance via a psychological effect, although a potential mediating role of hunger cannot be discounted.
This collection of essays, by leading scholars and practitioners from a range of countries, pays homage to a pre-eminent figure in the field of intellectual property: Sam Ricketson. Inspired by the breadth of Ricketson’s work, the contributions explore issues from a perspective that looks across the field – in particular, across the regimes, jurisdictions, disciplines and professions of IP. Topics explored across the regimes include the nature of IP subject matter, overlaps in protection, historical connections between copyright and patents and the transplantation of civil law moral rights to common law copyright. In across jurisdictions, chapters address, inter alia, the application of private international law to cross-border IP disputes, the Berne Convention and AI-authored works, how countries might exit the Berne Convention and dispute settlement under TRIPS. The intersection of copyright and privacy laws, the relationship between privacy, personality and trade mark laws, the teaching of IP and human rights and the conduct of empirical and historical research in IP are among the matters considered across disciplines. Contributions across professions include the participation of scholars in IP policy making, the IP textbook in legal practice, and the role of expert evidence in IP litigation.
Using as a starting point the work of internationally-renowned Australian scholar Sam Ricketson, whose contributions to intellectual property (IP) law and practice have been extensive and richly diverse, this volume examines topical and fundamental issues from across IP law. With authors from the US, UK, Europe, Asia, Australia and New Zealand, the book is structured in four parts, which move across IP regimes, jurisdictions, disciplines and professions, addressing issues that include what exactly is protected by IP regimes; regime differences, overlaps and transplants; copyright authorship and artificial intelligence; internationalization of IP through public and private international law; IP intersections with historical and empirical research, human rights, privacy, personality and cultural identity; IP scholars and universities, and the influence of treatises and textbooks. This work should be read by anyone interested in understanding the central issues in the evolving field of IP law.
Sleep disturbances are prevalent in cancer patients, especially those with advanced disease. There are few published intervention studies that address sleep issues in advanced cancer patients during the course of treatment. This study assesses the impact of a multidisciplinary quality of life (QOL) intervention on subjective sleep difficulties in patients with advanced cancer.
This randomized trial investigated the comparative effects of a multidisciplinary QOL intervention (n = 54) vs. standard care (n = 63) on sleep quality in patients with advanced cancer receiving radiation therapy as a secondary endpoint. The intervention group attended six intervention sessions, while the standard care group received informational material only. Sleep quality was assessed using the Pittsburgh Sleep Quality Index (PSQI) and Epworth Sleepiness Scale (ESS), administered at baseline and weeks 4 (post-intervention), 27, and 52.
The intervention group had a statistically significant improvement in the PSQI total score and two components of sleep quality and daytime dysfunction than the control group at week 4. At week 27, although both groups showed improvements in sleep measures from baseline, there were no statistically significant differences between groups in any of the PSQI total and component scores, or ESS. At week 52, the intervention group used less sleep medication than control patients compared to baseline (p = 0.04) and had a lower ESS score (7.6 vs. 9.3, p = 0.03).
Significance of results
A multidisciplinary intervention to improve QOL can also improve sleep quality of advanced cancer patients undergoing radiation therapy. Those patients who completed the intervention also reported the use of less sleep medication.
The US Navy utilizes numerous resources to encourage smoking cessation. Despite these efforts, cigarette smoking among service members remains high. Electronic cigarettes (EC) have provided an additional cessation resource. Little is known regarding the utilization efficacy of these cessation resources in the US Navy.
This study sought to explore the utilization and efficacy of ECs and other smoking cessation resources.
An anonymous cross-sectional survey was conducted at a military clinic from 2015 to 2016. Participants were active duty in the US Navy and reported demographics, smoking behaviors, and utilization of cessation resources.
Of the 977 participants in the study, 14.9% were current and 39.4% were former smokers. Most current smokers (83.6%) previously attempted cessation, smoked an average of 2–5 cigarettes per day (34.7%), and smoked every day of the month (26.4%). The number of daily cigarettes smoked and number of days cigarettes were smoked per month was not significantly different between cigarette-only smokers and EC dual users (p = 0.92, p = 0.75, respectively). Resources used by current and former smokers include: ‘cold turkey’ (44.6%, 57.1%, respectively), ECs (22.3%, 24.7%), nicotine patch (8.3%, 1.3%), medicine (6.6%, 3.9%), nicotine gum (5.8%, 10.4%), and quit programs (2.5%, 2.6).
Current and former cigarette smokers utilized similar resources to quit smoking. Electronic cigarettes are being used for cessation but do not significantly reduce the number of cigarettes smoked on a daily or monthly basis. Future studies may benefit from exploring the use of cessation resources and ECs within the military as a whole.
Eta Carinae is the most massive active binary within 10,000 light-years. While famous for the largest non-terminal stellar explosion ever recorded, observations reveal a supermassive (∼120 M⊙) binary consisting of an LBV and either a WR or extreme O star in a very eccentric orbit (e=0.9) with a 5.54-year period. Dramatic changes across multiple wavelengths are routinely observed as the stars move about in their highly elliptical orbits, especially around periastron when the hot (∼40 kK) companion star delves deep into the denser and much cooler (∼15 kK) extended wind photosphere of the LBV primary. Many of these changes are due to a dynamic wind-wind collision region (WWCR) that forms between the stars, plus expanding radiation-illuminated fossil WWCRs formed one, two, and three 5.54-year orbital cycles ago. These fossil WWCRs have been spatially and spectrally resolved by the Hubble Space Telescope/Space Telescope Imaging Spectrograph (HST/STIS) at multiple epochs, resulting in data cubes that spatially map Eta Carinae’s innermost WWCRs and follow temporal changes in several forbidden emission lines (e.g. [Fe iii] 4659 Å, [Fe ii] 4815 Å) across the 5.54-year cycle. We present initial results of 3D time-dependent hydrodynamical and radiative-transfer simulations of the Eta Carinae binary and its WWCRs with the goal of producing synthetic data cubes of forbidden emission lines for comparison to the available HST/STIS observations. Comparison of the theoretical models to the observations reveals important details about the binary’s orbital motion, photoionization properties, and recent (5–15year) mass loss history. Such an analysis also provides a baseline for following future changes in Eta Carinae, essential for understanding the late-stage evolution of a nearby supernova progenitor. Our modeling methods can also be adapted to a number of other colliding wind binary systems (e.g. WR 140) that are scheduled to be studied with future observatories (e.g. the James Webb Space Telescope).
The stellar winds of hot stars have an important impact on both stellar and galactic evolution, yet their structure and internal processes are not fully understood in detail. One of the best nearby laboratories for studying such massive stellar winds is the O4I(n)fp star ζ Pup. After briefly discussing existing X-ray observations from Chandra and XMM, we present a simulation of X-ray emission line profile measurements for the upcoming 840 kilosecond Chandra HETGS observation. This simulation indicates that the increased S/N of this new observation will allow several major steps forward in the understanding of massive stellar winds. By measuring X-ray emission line strengths and profiles, we should be able to differentiate between various stellar wind models and map the entire wind structure in temperature and density. This legacy X-ray spectrum of ζ Pup will be a useful benchmark for future X-ray missions.