1 |
Measurement of the absolute energy scale of MINOS and background measurements of NEMO-IIIJenner, Leo James January 2006 (has links)
No description available.
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2 |
Quantum gravity phenomenology and high-energy neutrinosMorgan, Dean Robert January 2005 (has links)
No description available.
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3 |
The separation of CC and NC events in the Sudbury Neutrino ObservatoryDunmore, Jessica A. January 2004 (has links)
No description available.
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4 |
New technology for imaging atmospheric Cherenkov telescopes and underwater neutrino detectorsWhite, Richard James January 2007 (has links)
No description available.
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5 |
Atmospheric neutrino predictions and the influence of hadron productionRobbins, Simon January 2004 (has links)
No description available.
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6 |
Systematic comparison of the MINOS near & far detector readout systemsSerra, Anatael Enrique Cabrera January 2005 (has links)
No description available.
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7 |
A measurement of the â¸B solar neutrino energy spectrum at the Sudbury Neutrino ObservatoryWilson, Jeanne R. January 2004 (has links)
No description available.
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8 |
Measurement of charged hadron yields for atmospheric neutrino studiesPattison, Charles Andrew Xavier January 2006 (has links)
No description available.
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9 |
Probing supernova shock waves via neutrino oscillationsHarries, Nicholas January 2008 (has links)
The time dependent neutrino oscillation signals due to the passage of a shock wave through the supernovae are analyzed for the case of three active neutrinos and also for the case that there are two additional sterile neutrinos. I re-examine the Landau-Zenner formula, which gives the level crossing probability at a MSW resonance, probing the deviations with specific application to the supernova shock wave. I use these results to examine phase effects which could be present due to multiple resonance crossings at the forward and reverse shocks.
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10 |
Measurement of the Flux of 8B Solar Neutrinos at the Sudbury Neutrino ObservatoryLoach, James Chilton January 2008 (has links)
The Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector that had the unique ability to measure both the total il active flux of solar neutrino, using a neutral current (NC) interaction, and the flux of electron neutrinos, using a charged current (CC) interaction. The experiment has demonstrated that neutrinos 3 change flavour and that the total neutrino flux is consistent with the prediction of solar models.
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