Limits on WWZ and WW\gamma couplings from p\bar{p}\to e\nu jj X events at \sqrt{s} = 1.8 TeV

We present limits on anomalous WWZ and WW-gamma couplings from a search for WW and WZ production in p-bar p collisions at sqrt(s)=1.8 TeV. We use p-bar p -> e-nu jjX events recorded with the D0 detector at the Fermilab Tevatron Collider during the 1992-1995 run. The data sample corresponds to an integrated luminosity of 96.0+-5.1 pb^(-1). Assuming identical WWZ and WW-gamma coupling parameters, the 95% CL limits on the CP-conserving couplings are -0.33<lambda<0.36 (Delta-kappa=0) and -0.43<Delta-kappa<0.59 (lambda=0), for a form factor scale Lambda = 2.0 TeV. Limits based on other assumptions are also presented.Comment: 11 pages, 2 figures, 2 table

Estimates of the absolute and relative strengths of diverse alcoholic drinks by young people

There was low but significant concordance between participants' rank-orderings of drinks by strength, and the correlation of mean ranks with correct ranks was also significant. However, their explicit estimates of the numbers of "units" in the drinks, and their % ABV values, often diverged dramatically from actual values. Participants tended to overestimate the unit contents of spirit-based drinks but underestimated the unit contents of beers and wine; women were consistently less accurate than men, typically making greater underestimates for commonly-consumed drinks. Over one-third of the sample reported that strength influenced drink choice, but its importance ranked below flavor and cost; drink strength might contribute to drink choice depending on the drinking situation. Conclusion/Importance: Young drinkers (women especially) have a poor awareness of the alcohol contents of different drinks, particularly wines and beers, but they make better judgments of relative strength