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Showing 1 to 5 of 5 for “"High energy neutrino"”.

  1. Design and feasibility studies for a high energy neutrino detector / Janice Reid.

    This thesis develops the design of a high energy neutrino detector intended to observe astrophysical point sources.

    adelaide Repository record for Design and feasibility studies for a high energy neutrino detector / Janice Reid. (opens in a new tab)

  2. Phenomenology of a Low-Energy Neutrino Factory and Related Experiments

    The discovery of neutrino oscillations is one of the most important in the recent history of particle physics, being the first evidence of physics beyond the Standard Model. We describe the theoretical framework of the neutrino oscillation model, motivate the necessity for a new generation of …

    durham Repository record for Phenomenology of a Low-Energy Neutrino Factory and Related Experiments (opens in a new tab)

  3. A Search for Muon Neutrinos from Gamma-Ray Bursts wih the IceCube 22-String Detector

    Two searches are conducted for muon neutrinos from Gamma-Ray Bursts (GRBs) using the IceCube detector. Gamma-Ray Bursts are brief and transient emissions of keV/MeV radiation occuring with a rate of a few per day uniformly in the sky. Swift and other satellites of the Third Interplanetary Network …

    maryland Repository record for A Search for Muon Neutrinos from Gamma-Ray Bursts wih the IceCube 22-String Detector (opens in a new tab)

  4. Development of reconstruction algorithms for large volume neutrino telescopes and their application to the KM3NeT detector

    Neutrino-astronomy is one of the most interesting frontiers of the astro-particle physics. Neutrino telescopes detect neutrinos indirectly through charged leptons produced in weak charged current interaction. In transparent media, tracks of relativistic particles can be reconstructed detecting …

    catania Repository record for Development of reconstruction algorithms for large volume neutrino telescopes and their application to the KM3NeT detector (opens in a new tab)

  5. Procedure di modellizzazione rapide per la caratterizzazione di Supernovae Core Collapse e di transienti similari

    Le Supernovae da Collasso Gravitazionale (Core Collapse Supernovae, CC-SNe) rappresentano la fase finale dell'evoluzione di stelle sufficientemente massive (M_{ZAMS} > 8-10 M_\odot). Questi eventi sono tra i fenomeni più energetici dell'Universo (con energie di esplosione tipiche dell'ordine di …

    catania Repository record for Procedure di modellizzazione rapide per la caratterizzazione di Supernovae Core Collapse e di transienti similari (opens in a new tab)