With completion expected in 2011, the IceCube Neutrino Observatory is approaching the 1 km 3 scale required for high energy neutrino astronomy. Before completion, the data taken with the deployed strings of the IceCube detector allows the testing of different procedures of searching for high energy
A strategy for discovering heavy neutrinos
β Scribed by C.A. Heusch; P. Minkowski
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 306 KB
- Volume
- 374
- Category
- Article
- ISSN
- 0370-2693
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π SIMILAR VOLUMES
The Monte Carlo generator MAJOR 1.5 simulates the production and decay of heavy Majorana neutrinos via lepton mixing or exchange of 'light' right-handed W-bosons in deep inelastic scattering, i.e. eΒ±p -, NX -~ eΒ±W~X or uΒ’ZX. Physics and programming aspects are described in this manual.
The standard Big Bang cosmology predicts that the universe is abundantly populated with neutrinos. As expected there are at least 114 neutrinos per cubic centimeter averaged over the whole space. Like the cosmic background radiation the cosmic neutrinos at present posses a very small kinetic energy