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  • About
  • The Global ETD Search service is a free service for researchers to find electronic theses and dissertations. This service is provided by the Networked Digital Library of Theses and Dissertations.
    Our metadata is collected from universities around the world. If you manage a university/consortium/country archive and want to be added, details can be found on the NDLTD website.
1

Measurement of the absolute energy scale of MINOS and background measurements of NEMO-III

Jenner, Leo James January 2006 (has links)
No description available.
2

Quantum gravity phenomenology and high-energy neutrinos

Morgan, Dean Robert January 2005 (has links)
No description available.
3

The separation of CC and NC events in the Sudbury Neutrino Observatory

Dunmore, Jessica A. January 2004 (has links)
No description available.
4

New technology for imaging atmospheric Cherenkov telescopes and underwater neutrino detectors

White, Richard James January 2007 (has links)
No description available.
5

Atmospheric neutrino predictions and the influence of hadron production

Robbins, Simon January 2004 (has links)
No description available.
6

Systematic comparison of the MINOS near & far detector readout systems

Serra, Anatael Enrique Cabrera January 2005 (has links)
No description available.
7

A measurement of the ⁸B solar neutrino energy spectrum at the Sudbury Neutrino Observatory

Wilson, Jeanne R. January 2004 (has links)
No description available.
8

Measurement of charged hadron yields for atmospheric neutrino studies

Pattison, Charles Andrew Xavier January 2006 (has links)
No description available.
9

Probing supernova shock waves via neutrino oscillations

Harries, 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.
10

Measurement of the Flux of 8B Solar Neutrinos at the Sudbury Neutrino Observatory

Loach, 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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