“That's cool, you’re a musician and you drink”: Exploring entertainers’ accounts of their unique workplace relationship with alcohol

This qualitative research investigates the alcohol experiences of entertainers who perform within licensed premises. Previous, mainly quantitative, studies have found that entertainers, specifically musicians, are an occupational group who drink excessively. This qualitative study draws on a wider sample of entertainers to examine their accounts of drinking in the workplace and the explanations they provide for this. We conducted individual semi-structured interviews (n = 24) with band-members, variety acts and DJs in Glasgow, Scotland. This revealed a workplace characterised by continual opportunities for often free alcohol consumption. Unlike most occupations, for entertainers ‘drinking-on-the-job’ was normative, expected, and sometimes encouraged by peers, the public, employers or sponsors. Entertainers also experienced performance-related incentives to drink before, during and/or after a show; including anxiety, matching their intoxication level to the audience's, and ‘reward-drinking’. This qualitative research confirms the unique nature of the entertainer-alcohol link, even in comparison to that found within other leisure industry occupations. While providing some explanation as to why entertainers might drink excessively, participants’ accounts also suggested potential strategies for avoiding the negative outcomes of workplace drinking

‘I can spot them a mile off’: community shopkeepers’ experience of alcohol test-purchasing

Aims: Test-purchasing (using volunteers to attempt an apparent under-age purchase) can be used as an enforcement intervention against retailers who sell alcohol to minors. This article will investigate whether community shopkeepers, familiar with alcohol test-purchasing protocols, are able to distinguish volunteers from genuine under-age customers.<p></p> Methods: Thirty-six qualitative interviews were conducted with community shopkeepers, the retailers most often associated with under-age sales, working in convenience stores located in socially-contrasting areas of Glasgow, Scotland, 24 of which were licensed to sell alcohol.<p></p> Findings: Interviewees provided details of the strategies they used to prevent under-age sales. Robust age-verification, set 7.5 above legal-age of purchase, was felt to be particularly effective. Although, they were apprehensive of test-purchases, experienced retailers reported that they always knew when one was taking place in their shop, because volunteers were not sourced locally and, in contrast to real under-age customers, they were honest and compliant.<p></p> Conclusions: Although making retailers more aware of their responsibilities, increased familiarity with the protocols of test-purchasing can allow vendors to be certain who real under-age customers are, potentially making low-risk sales to minors possible. Test-purchasing protocols (e.g. volunteers ages) should be re-oriented to keep pace with more robust age-verification checks.<p></p&gt

Search for gravitational waves from Scorpius X-1 with a hidden Markov model in O3 LIGO data

Results are presented for a semicoherent search for continuous gravitational waves from the low-mass x-ray binary Scorpius X-1, using a hidden Markov model (HMM) to allow for spin wandering. This search improves on previous HMM-based searches of Laser Interferometer Gravitational-Wave Observatory data by including the orbital period in the search template grid, and by analyzing data from the latest (third) observing run. In the frequency range searched, from 60 to 500 Hz, we find no evidence of gravitational radiation. This is the most sensitive search for Scorpius X-1 using a HMM to date. For the most sensitive subband, starting at 256.06 Hz, we report an upper limit on gravitational wave strain (at 95% confidence) of h 95 % 0 = 6.16 × 10 − 26 , assuming the orbital inclination angle takes its electromagnetically restricted value ι = 4 4 ° . The upper limits on gravitational wave strain reported here are on average a factor of ∼ 3 lower than in the second observing run HMM search. This is the first Scorpius X-1 HMM search with upper limits that reach below the indirect torque-balance limit for certain subbands, assuming ι = 4 4 °

Search for intermediate-mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo

International audienceIntermediate-mass black holes (IMBHs) span the approximate mass range 100−105 M⊙, between black holes (BHs) that formed by stellar collapse and the supermassive BHs at the centers of galaxies. Mergers of IMBH binaries are the most energetic gravitational-wave sources accessible by the terrestrial detector network. Searches of the first two observing runs of Advanced LIGO and Advanced Virgo did not yield any significant IMBH binary signals. In the third observing run (O3), the increased network sensitivity enabled the detection of GW190521, a signal consistent with a binary merger of mass ∼150 M⊙ providing direct evidence of IMBH formation. Here, we report on a dedicated search of O3 data for further IMBH binary mergers, combining both modeled (matched filter) and model-independent search methods. We find some marginal candidates, but none are sufficiently significant to indicate detection of further IMBH mergers. We quantify the sensitivity of the individual search methods and of the combined search using a suite of IMBH binary signals obtained via numerical relativity, including the effects of spins misaligned with the binary orbital axis, and present the resulting upper limits on astrophysical merger rates. Our most stringent limit is for equal mass and aligned spin BH binary of total mass 200 M⊙ and effective aligned spin 0.8 at 0.056 Gpc−3 yr−1 (90% confidence), a factor of 3.5 more constraining than previous LIGO-Virgo limits. We also update the estimated rate of mergers similar to GW190521 to 0.08 Gpc−3 yr−1.Key words: gravitational waves / stars: black holes / black hole physicsCorresponding author: W. Del Pozzo, e-mail: [email protected]† Deceased, August 2020