5–7 Aug 2013
AlbaNova University Center
Europe/Stockholm timezone

Session

Physics, Reconstruction, and Software III.

PRS3
6 Aug 2013, 11:00
AlbaNova University Center

AlbaNova University Center

Presentation materials

There are no materials yet.

  1. Mr Samuel Flis (Stockholms Universitet)
    06/08/2013, 11:00
    Physics, Reconstruction, and Software
    The cubic-kilometer sized IceCube neutrino observatory, constructed in the glacial ice at the South Pole, offers new opportunities for neutrino physics to reach lower neutrino energies with its in-fill array “DeepCore”. A set of analysis techniques where the outer layers of IceCube are used as a veto makes it possible to reject atmospheric muons and thereby allows low-energy neutrino...
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  2. Dr Imre Bartos (Columbia University)
    06/08/2013, 11:25
    Physics, Reconstruction, and Software
    Jet reheating via nuclear collisions has recently been proposed as the main mechanism for gamma-ray burst (GRB) emission. In addition to producing the observed gamma rays, collisional heating must generate 10–100 GeV neutrinos, implying a close relation between the neutrino and gamma-ray luminosities. We exploit this theoretical relation to make predictions for possible GRB detections...
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  3. Andreas Gross (TUM)
    06/08/2013, 11:50
    Physics, Reconstruction, and Software
    The determination of the neutrino mass hierarchy is among the most fundamental questions in particle physics. The recent measurement of a large mixing angle between the first and the third neutrino mass eigenstate and the first observation of atmospheric neutrino oscillations at tens of GeV with neutrino telescopes opens the intriguing new possibility to exploit matter effects in neutrino...
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