Maggie Chon

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The Sudbury Neutrino Observatory is a second generation water Cerenkov detector designed to determine whether the currently observed solar neutrino deecit is a result of neutrino oscillations. The detector is unique in its use of D 2 O as a detection medium, permitting it to make a solar modellindependent test of the neutrino oscillation hypothesis by(More)
B. Aharmim, S. N. Ahmed, T. C. Andersen, A. E. Anthony, N. Barros, E.W. Beier, A. Bellerive, B. Beltran, M. Bergevin, S. D. Biller, K. Boudjemline, M.G. Boulay, T. H. Burritt, B. Cai, Y. D. Chan, M. Chen, M.C. Chon, B. T. Cleveland, G.A. Cox-Mobrand, C. A. Currat, X. Dai, F. Dalnoki-Veress, H. Deng, J. Detwiler, P. J. Doe, R. S. Dosanjh, G. Doucas, P.-L.(More)
Solar neutrinos from (8)B decay have been detected at the Sudbury Neutrino Observatory via the charged current (CC) reaction on deuterium and the elastic scattering (ES) of electrons. The flux of nu(e)'s is measured by the CC reaction rate to be straight phi(CC)(nu(e)) = 1.75 +/- 0.07(stat)(+0.12)(-0.11)(syst) +/- 0.05(theor) x 10(6) cm(-2) s(-1).(More)
This Article examines the ways that contemporary creativity challenges copyright's fixation requirement. In this Article, we identify concrete problems with the fixation requirement, both practically and in light of the fundamental purpose and policy behind copyright law, and argue for a change that would amend the fixation requirement to better function in(More)
In 1994, over 150 nations converged in Punta del Este, Uruguay, and completed what was, at that time, the most ambitious multilateral intellectual property (IP) agreement ever negotiated. Built on the cornerstone of the “Great Conventions,”1 the World Trade Organization’s (WTO) Agreement on TradeRelated Aspects of Intellectual Property Rights (TRIPS(More)
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