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Ken Clark (University of Toronto)31/07/2015, 14:00NU-INOral contributionScientists have created the world's largest neutrino telescope, the IceCube Neutrino Observatory, in one of the planet’s most extreme environments at South Pole Station Antarctica. Completed in 2010, and instrumenting more than a cubic-kilometre of ice, IceCube also includes a low-energy detector array, called DeepCore, that has performed world-leading indirect dark matter searches and very...Go to contribution page
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Paolo Piattelli (INFN)31/07/2015, 14:18NU-INOral contributionThe recent discovery by the IceCube collaboration of a high-energy neutrino flux of extra-terrestrial origin has opened a new observational window on the Universe. However, unambiguous identification of the emitting neutrino sources will require next generation neutrino telescopes with full sky coverage. The KM3NeT Collaboration aims at building a research infrastructure in the depths of the...Go to contribution page
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Juergen Brunner (CPPM)31/07/2015, 14:36NU-INOral contributionThe atmospheric flux of neutrinos has traditionally been seen as a background to the detection of an astrophysical neutrino signal. In recent years however, it has been realised that in the few-GeV range, this flux holds the key to resolving a fundamental question of particle physics: that of the neutrino mass hierarchy, i.e. whether the mass eigenstate $\nu_3$ is heavier (normal hierarchy) or...Go to contribution page
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Erik Blaufuss (University Of Maryland)31/07/2015, 14:54NU-INOral contributionGiven recent observations of an astrophysical flux of neutrinos by the IceCube neutrino observatory, the design of the next generation Antarctic neutrino observatory is well underway. The IceCube Gen2 high-energy array will instrument a $\sim10\,\mathrm{km}^3$ volume of clear glacial ice at the South Pole to deliver substantial increases in the observed astrophysical neutrino sample for all...Go to contribution page
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Prof. George Wei-Shu Hou (National Taiwan University)31/07/2015, 15:12NU-INOral contributionBy separating $\nu_{\tau}\to\tau$ conversion from $\tau$-shower generation, the Earth-skimming $\nu_{\tau}$ method allows for huge target mass and detection volume simultaneously. In part motivated by recent IceCube astrophysical PeV neutrino events, the planned NTA observatory will have three site stations watching the air mass surrounded by Mauna Loa, Mauna Kea, and Hualalai on...Go to contribution page
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