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Reducing background in the t neutrino mass limiting decay t [plus or minus] --> K [plus or minus] Ks̳p0̳̳vt̳ /Pais, Preema R. January 2006 (has links) (PDF)
Undergraduate honors paper--Mount Holyoke College, 2006. Dept. of Physics. / On t.p. s̳̳̳ and t̳ are subscript; 0̳ is superscript.
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An investigation of matter enhanced neutrino oscillation with the Sudbury Neutrino Observatory /Smith, Miles Walter Eldon. January 2002 (has links)
Thesis (Ph. D.)--University of Washington, 2002. / Vita. Includes bibliographical references (p. 125-130).
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A low energy measurement of the ⁸B solar neutrino spectrum at the Sudbury Neutrino ObservatorySeibert, Stanley Reid, January 1900 (has links)
Thesis (Ph. D.)--University of Texas at Austin, 2008. / Vita. Includes bibliographical references.
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High energy neutrino-nucleon interactions with an electron in the final stateGee, Manyee Ngai. January 1984 (has links)
Thesis (Ph. D.)--University of Wisconsin--Madison, 1984. / Typescript. Vita. eContent provider-neutral record in process. Description based on print version record. Includes bibliographical references (leaves 209-213).
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Prompt neutrino production in the 1982 beam dump experiment at CERNBostock, Paul January 1985 (has links)
Principles of beam dump experiments are reviewed and the 1982 beam dump at CERN using the Big European Bubble Chamber is described in detail. Neutrino events have been detected using both the bubble chamber and its associated electronic detectors. Prompt event rates are established for V<sub>μ</sub> , Ṽ<sub>μ</sub> , V<sub>e</sub> and Ṽ<sub>e</sub> . The prompt rates are consistent with lepton universality. The charm production cross-section required to explain the prompt electron-(anti)neutrino signal is approximately 16-105/μb per nucleon, assuming linear dependence of this cross-section on nucleon number. This range of values reflects the fact that we have not been able to find a model which is consistent with all aspects of the data. The neutral to charged current ratio for electron-neutrinos is found to be 0.23 ±0.16. The expected number of tau-neutrino events is estimated and kinematic and visual searches for tau-neutrino interactions are described. One visually detected candidate is described in detail. No positive evidence for a tau-neutrino interaction has been found. From the ratio of neutral to charged current events in the data we infer that no more than 4% of the prompt charged current events and 40% of the total prompt signal may be attributed to tau-neutrinos at 90% CL.
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Majorana Neutrinos in the Jacob-Wick phase conventionWaldman, Zachary J. January 2008 (has links)
Thesis (M.S.)--State University of New York at Binghamton, Department or Physics, Applied Physics and Astronomy, 2008. / Includes bibliographical references.
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Optical calibration of the Sudbury Neutrino Observatory and determination of the 8B solar nutrino flux in the salt phase /Grant, Darren R. January 1900 (has links)
Thesis (Ph. D.)--Carleton University, 2004. / Includes bibliographical references (p. 159-165). Also available in electronic format on the Internet.
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Measurement of the strange-antistrange asymmetry at NLO in QCD from NuTeV dimuon data /Mason, David Alexander, January 2006 (has links)
Thesis (Ph.D.)--University of Oregon, 2006. / Typescript. Includes vita and abstract. Includes bibliographical references (leaves 415-429). Also available for download via the World Wide Web; free to University of Oregon users.
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An enhanced measurement of the angular response of photomultiplier tubes at the Sudbury Neutrino Observatory /Simard, Olivier, January 1900 (has links)
Thesis (M.Sc.) - Carleton University, 2005. / Includes bibliographical references (p. 138-141). Also available in electronic format on the Internet.
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A search for periodic time variations in the solar neutrino data from the Sudbury Neutrino Observatory /Heelan, Louise January 1900 (has links)
Thesis (M.Sc.) - Carleton University, 2005. / Includes bibliographical references (p. 125-130). Also available in electronic format on the Internet.
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